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00:00 | Recording. Do you do what you do man? Got it. Okay |
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00:10 | 8 30 on the dot. So any any questions from yesterday Stephanie. |
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00:21 | I think I'm good. Okay um well I was thinking that I was |
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00:29 | through the lecture notes this morning for and I was making little corrections and |
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00:38 | like that and they're in here and highlighting them and I'm probably going to |
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00:42 | through while it's still fresh in my . I'm gonna go through yesterday's lecture |
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00:48 | you know there were little things that know that I was commenting on and |
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00:52 | gonna go back through and kind of of smooth that over a little bit |
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00:57 | I'll highlight those changes and I'll send I'll upload those and then um uh |
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01:06 | type if you don't mind moving them and that way you'll have sort of |
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01:12 | whatever an attitude version that's a little better. Um Anyways and I hope |
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01:20 | don't mind that I hope that works for you so okay so no questions |
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01:26 | let's just go move forward. Um the other class going right now you |
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01:33 | ? Yes so it's not good to talking that. Okay all right very |
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01:42 | then you don't have to um okay get started with number two cat lecture |
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01:49 | two and this morning going to talk instruments acquisition and processing so still I |
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01:59 | not as boring as theory but um you know still not really the the |
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02:09 | good stuff that we're building up to acquisition and instrumentation so uh we'll start |
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02:19 | gravity and then we'll do Magnetics just that. Well that sort of, |
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02:24 | sort of theme will be what we all through this stuff even through this |
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02:30 | and processing and anomaly enhancements. So right, so gravity surveys are carried |
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02:38 | using a gravity meter or some people groove immature doesn't matter. Um Grove |
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02:46 | is kind of, people say that in south America and europe and africa |
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02:55 | you know Southeast Asia, maybe even , a lot of people in this |
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03:00 | just say gravity meter. Um There two basic types, those that measure |
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03:08 | measurements and and those are the most and they use springs or vibrating vibrating |
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03:17 | mechanisms. And then there's uh I know of one type. I mean |
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03:24 | instrument that's an absolute measurement and it's free fall. So it just measures |
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03:30 | the timing of the, when it drops, drops a weight and it |
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03:36 | past some sensors and it measures that accurately. And then it figures |
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03:41 | you know uh what the gravitational attraction from that. So we'll start with |
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03:50 | relative measurement instruments. The zero the very first one was Lacosta, |
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03:57 | and Ellen are meters were invented in early 19 hundreds, 1930 ish. |
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04:05 | think. So not even 100 years . And before that people did measure |
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04:12 | gravity instruments, we, as we in our historical observations, but they |
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04:18 | a Tarzan balance which is a It's a gradient measurement. So it's |
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04:25 | the derivative of the field which is as the derivative of the potential. |
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04:33 | that idea goes back to cavendish like 7/17 century, I think. So |
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04:42 | torsion balance and now it's funny because grade geometry is now there are modern |
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04:52 | and we're not gonna talk about them you want to have that. But |
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04:55 | have material for that in the in extra lecture, we could do an |
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05:00 | lecture if you wanted to learn about geometry and heat flow at the |
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05:05 | you think about it and we'll decide of doing the exam on that on |
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05:11 | 10th. We could do that lecture the 10th and then do the exam |
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05:15 | the 14th. If you just like find that you're just in love with |
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05:19 | material that I present. So Um So the zero length string instrument |
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05:27 | characterized by an infinite period. That's it's called zero length. That kind |
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05:33 | a weird name. And the infinite of suspension entails infinite displacement theoretically. |
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05:43 | so this is why Lucien lacoste. never met him. I did see |
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05:47 | one time. Um This is why called it the zero length string and |
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05:52 | said it should be called the zero length length spring. But it's kind |
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06:00 | , you know too wordy. So equilibrium the gravitational torque on the |
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06:07 | A little figure here on the side is the spring and then uh |
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06:15 | Is this dimension um B. Is dimension along this lever that's connected to |
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06:22 | spring. D. Is the length From the point the fulcrum to um |
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06:31 | weight. Well I mean some some well to a distance that's perpendicular from |
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06:39 | mass that's attached to this lever. so of course remember your physics 102 |
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06:48 | one or whatever in Houston. Um called 13 30 I think physics or |
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06:53 | 3. It's a four hour credit least. It was when I took |
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06:56 | . So Mass MG is the gravitational . Mass times gravity. Okay so |
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07:09 | at equilibrium it's this weight times this times the co sign of of this |
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07:18 | here. So basically um Right. if you remember your physics D. |
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07:27 | this angle is the moment of right? And then the torque on |
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07:33 | string I guess torque K. I is equal to B times A. |
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07:42 | this angle. So that's the the moment of the torque I |
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07:48 | And then if you set the zero other, the cosine angles fall |
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07:53 | You just have this little formula So that's how it works. It's |
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07:58 | it's um Yeah, alright there's probably are used to be the most common |
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08:09 | instrument around and um but Eleanor through sales and restructuring etcetera etcetera. They |
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08:24 | were bought out, downsize et cetera cetera. They are now owned by |
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08:28 | company in Denver called Ed Con. they're mostly just, I don't know |
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08:35 | they're building new machines I think they be but I know that they're doing |
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08:39 | lot of service. They do a of rentals of their machines but but |
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08:44 | tracks who are based up in Toronto instruments, They make the c. |
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08:52 | think they make some more advanced ones they are far and away the most |
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08:58 | instruments they have basically taken over and their design is simpler they're easier to |
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09:06 | their, you know easy to operate carry around. They might even be |
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09:10 | . Um and and uh like that this is the most popular kind here |
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09:20 | it has these support strings as a string spring and uh yeah that's how |
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09:29 | works a little bit different. And the absolute gravity meter also there might |
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09:40 | some other instruments besides Eleanor's and syntax I don't know what they are. |
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09:47 | wouldn't surprise me if like there's a grab immature or something like that or |
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09:51 | a chinese group amateur. Okay. the absolute, this is the one |
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09:57 | know but this is it's made by company that first meeting was called Micro |
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10:02 | . Micro G. Is also owned Ed Con these days so you |
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10:06 | you know and that is not a company, you know it's a small |
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10:11 | but the whole phenomena of you know buying little companies sort of thing in |
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10:21 | case this is how it works. have a flea of free falling um |
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10:26 | chamber, it's a vacuum chamber and drops through here and it gets lifted |
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10:31 | up. Um and there's a interference and some mirrors in here and it |
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10:38 | measures the time and here is a of the uh instrument south and then |
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10:49 | guess the data, I mean the and and all the whatever this the |
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10:57 | know pC cards and things like And of course you just plug it |
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11:00 | your laptop and just do it. it's very easy. The the |
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11:05 | And R. Meter. I don't a picture one. Yeah. Here |
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11:09 | have to actually like look in this you look inside here I think and |
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11:14 | eyeball it to level it up and to see what it's doing I |
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11:22 | And then here's one um this is Prudhoe Bay and I have a little |
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11:28 | history. I'm gonna show you about these instruments in Prudhoe Bay. Of |
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11:33 | I guess that looks like a looks a fox out there to me. |
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11:38 | you know, so they're environmentally friendly guess. Okay so now there's |
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11:44 | this is a this is another relative , a borehole gravity. So there's |
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11:50 | borehole tool. And Schlumberger has these they're really big and fat so they |
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11:57 | go in a lot of holes that drilled these days. But this is |
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12:00 | a little little zero length spring mechanism there. And they can measure density |
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12:09 | because you measure some response here and response there and there's a formula that |
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12:14 | can just solve it will calculate density and they measure far into the |
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12:21 | In fact, the spacing that you your measurements over is kind of dictates |
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12:26 | far into the formation it can but but it's unaffected by mud and |
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12:35 | casing, things like that. So really useful tools um they are limited |
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12:42 | they're big and fat and plus you go too far off an angle, |
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12:48 | , like so little horizontal drilling for guys. So they are limited, |
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12:53 | are used still today, but not lot. Um people in the past |
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12:59 | been trying to develop gravity instruments that be smaller that can go into smaller |
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13:08 | and you know, survive higher temperatures . Also a limitation, I should |
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13:15 | that. So I need to add that to the, The discussion |
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13:21 | , uh make a note four hole limitation but they're trying to but there |
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13:31 | folks, there have been attempts, have spent lots of money trying to |
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13:34 | this because if you can build a instrument that could survive high temperatures and |
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13:42 | and be able to put in all sized well holes, There would be |
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13:47 | lot of money because it would because I said, they measured density deep |
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13:51 | the formation much farther than any wire tool. You know, any robi |
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13:58 | they use now because those things, know, they barely see past the |
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14:02 | . So it would be a big . So there's a lot of money |
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14:06 | be made. Um the the reason they can't be, I mean the |
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14:19 | magnetometers uh work on on a molecular . They're not mechanical at all. |
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14:29 | uh that's the reason. If you figure out how to measure gravity at |
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14:35 | molecular level, then that would be cool. But you know, the |
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14:41 | is called, you know, the main forces of nature, right |
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14:45 | electro Magnetics and the too weak and forces. Atomic forces, you |
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14:51 | that hold matter together and then the atomic forces of course radioactive decay. |
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14:57 | gravity is gravity at small scales is weak. But of course, as |
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15:02 | talked yesterday, galactic scales can actually time. So so the small scale |
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15:07 | very weak and so molecularly looks like not possible but it doesn't stop people |
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15:12 | trying. They could should still keep . So, um what is |
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15:18 | This is a one more comment on . If the stations of a borehole |
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15:22 | survey were separated by less than 70 the time between read so they could |
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15:28 | it every 18 minutes and the gravity with a borehole would measure you know |
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15:35 | micro gals. 10 micro gals is 1/100 of a millimeter. So basically |
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15:44 | they're saying for intervals greater than 20 this is a measuring density. It |
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15:49 | be point oh two grand for C. C. Her less. |
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15:56 | they're very they can measure very small differences in gravity and hence small differences |
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16:07 | density. Um I'm gonna make a also to come up with some nominal |
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16:17 | formation penetrations. I'll look at uh it later. Maybe I'll tell you |
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16:23 | I look it up anyways I'll try best to remember. Okay so now |
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16:28 | are actually instruments they have also taken and R. Meters and stuck them |
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16:33 | a stuck them in a little you know water type bell that they |
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16:42 | off boats and then um measure the at the at the water about |
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16:48 | And there's there's a whole big database you can still get. That's called |
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16:53 | Schaefer. I think it's owned by now or maybe still buy food |
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17:00 | But one or the other and it's the whole of the gulf coast and |
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17:04 | an old old database but it doesn't that data is Very good quality and |
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17:10 | a water bottom database for the many on the shelf going all the way |
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17:17 | to the 60 s government. So uh so for purposes measuring. Right |
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17:24 | it's 1/100 of a millimeter google or would be 10 micro gals. |
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17:30 | Plus or minus 10. And it's But for time land better precision. |
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17:38 | . Yeah it's very accurate. But saying it's still limited for environmental |
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17:44 | time lapse etcetera. Fair enough. They do use measure gravity, that |
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17:53 | bottom. But this is this this is kind of like an aside |
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17:58 | we're going to look at the time study on Prudhoe Bay, like I |
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18:02 | earlier. Uh Now this is so is an interesting point because all these |
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18:11 | are gonna claim just just amazing accuracy you know, Eleanor and sent |
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18:19 | They claim their accuracy is 1-5 micrograms it might be sitting on the lab |
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18:25 | the bench in the laboratory. But me, the way I view these |
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18:32 | is what is the what is the , you know, one of the |
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18:38 | wavelength and not only amplitudes that I measure um with confidence, you |
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18:49 | Um So you know, oh what I just do? Okay. |
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19:01 | Never mind. Um Yeah, in case. Right. So what that's |
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19:08 | I make, that's how I like think about it. I don't really |
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19:11 | because first of all these values are . You know, so it's like |
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19:16 | root mean square or something. And uh I don't know what that |
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19:23 | So in any case yeah, I you know, whatever they're wonderful but |
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19:29 | not I'm not sure what they mean in terms of what what I can |
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19:33 | with confidence. So that's just something think about. Okay, so here's |
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19:41 | comparison of Eleanor and Centrex meters and so you can see the scale is |
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19:52 | Micro gowns maximum and this is um see, this is a you from |
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20:00 | to 2008. Um So I get is that right? Is that that |
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20:08 | 160 days? Um So these are guess bench measurements And um 2.1 micro |
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20:20 | . 8.9 micro gals. Okay, see that's what this level is. |
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20:24 | numbers, they coincide. So the I guess of the LNR was 8.9 |
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20:32 | goals and the means the scent tracks for the most part around 2.1. |
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20:36 | guess there was some big spikes in . But This is so this this |
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20:44 | , this is 3/100 of a I mean, you know, who |
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20:53 | right. But I guess this, was published uh and uh I guess |
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20:59 | guess this was a big deal back the day for those guys. |
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21:04 | fine, fine and dandy. Uh look at magnetic instrumentation there. My |
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21:10 | ones remember victor vacuum, who worked golf and worked with with the whatever |
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21:18 | Defense Department during World War Two to this instrument, this is the flux |
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21:24 | and it has a resolution of about gamma one nano Tesla. And um |
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21:31 | here's where I added added something with highlight. I'll do the same thing |
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21:34 | the other notes. Excuse me. Okay, so they measure relative field |
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21:49 | again. So it's a three access and this is this is the |
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21:56 | So you see the coils, you that coil, you have two sets |
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21:59 | coils this way, a set of this way and a set of coils |
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22:03 | way. And and basically they're each each access consists of a pair of |
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22:12 | but opposite lee woven inductive coils. here's a little sort of sketch of |
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22:19 | . So there these are they are opposite and then they are coiled around |
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22:28 | a magnetized, saturated, you highly permeable material and there which is |
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22:38 | right? When you when you pump current through it, you're gonna saturate |
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22:44 | because remember electricity currents produce a magnetic , that kind of right hand |
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22:50 | So from your physics Physics one and one is going one way that is |
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22:56 | the other way, they're gonna cancel . And and I and this is |
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23:03 | they become sensitive to fluctuations. very bad. Um Yeah, so |
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23:11 | at this closer, here's our little figure again um we're gonna have a |
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23:18 | B one secondary B two and then an equilibrium be in equilibrium the current |
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23:28 | going to produce fields that can you know oppose each other, this |
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23:34 | in time. So they're gonna just each other in time, they're going |
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23:37 | cancel out to zero. Now if if the ambient field is not |
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23:48 | Then these two coils because their wound Lee, one is gonna work in |
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23:55 | negative way against the inducing build other going to be going to be positive |
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24:02 | . So they're not gonna be the . So when you sum them, |
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24:06 | going to have some output signal and that output signal is gonna be proportional |
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24:14 | the magnetic field. That's the And and if you want me to |
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24:23 | or back up, just jump in tell me to do that because, |
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24:27 | know, I don't want to wait go back 100 slides or something like |
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24:31 | . Okay. Alright. So that the that's the first magnetometers that were |
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24:42 | . And then when I first started the business, they were still using |
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24:46 | . In fact, they do still these but they used them for |
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24:50 | I'll explain that when we talk about . Okay, So then there's two |
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24:58 | of um uh what we call them resident uh uh magnetometers. There's |
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25:10 | it's called a pro one is called first one that was called a proton |
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25:15 | . It's a residence type magnetometer and resolution is about an order of magnitude |
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25:22 | than the flux gate. And it . And it's called a proton procession |
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25:28 | it if you look at. So right half side of the figure is |
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25:34 | of like a gravitational sort of analog the, to the magnetic side. |
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25:42 | ? And this is again at the level. Uh there's, you |
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25:48 | and so you have if you haven't take a spinning top for and you've |
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25:52 | this before, I'm sure it will process or gyrate about some axes. |
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26:02 | ? Well, that's how, that's a proton procession worse it will gyrate |
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26:09 | the Larmore frequency of protons in the rich fluid. So there's a |
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26:16 | here's the coil right here. These lines that's represented coil and then the |
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26:22 | of the coil is has to be at a high angle to the ambient |
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26:27 | direction, right to the inclination. then they they pulse, it pulse |
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26:37 | coil with some electricity and then it relax it. And as it |
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26:43 | then the the the uh the protons the in the hydrogen, which fluid |
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26:54 | will begin to process. And you and that precession can be detected with |
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27:02 | to frequency. And that frequency then turn, is related to the field |
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27:08 | , if that makes sense. here's here's a picture of one down |
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27:17 | , I've actually operated one of Um So you have a little |
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27:21 | I mean, we'll read out And you key in like your location |
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27:27 | some details. And then you just this on a stick away, you |
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27:32 | have any, you know any metal in your pockets and things like |
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27:37 | And then you make sure make sure coil is oriented at a high angle |
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27:43 | the field. Then you and you it, you take measurements and it |
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27:51 | four or 5 every second. There be interference like power lines. They |
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27:56 | a magnetic field and you know, have to be careful not to rotate |
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28:02 | sensor, but they do require a of power to operate. So, |
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28:08 | that's the thing. But proton I mean the department has one of |
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28:14 | , so, you know, um right now there's another residence type magnetometer |
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28:25 | an alkaline vapor or they're also called pumped. And they have a |
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28:30 | That's another order of magnitude better than . So two orders of magnitude better |
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28:36 | a flux gate. One order of better than a proton procession. They |
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28:44 | sample 20 hertz. So they sample times faster than the proton precession. |
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28:50 | don't need as much power. So are great, they're great instruments. |
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28:58 | and how they work is they have lamp that pulses and there's an absorption |
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29:05 | and then it goes into a photo and then that is measured. And |
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29:10 | that that response is of course proportional the earth's field strength. Um and |
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29:19 | here's like a little picture of how , how it works. So the |
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29:23 | pumped refers to the lamp, the that's pumped. Okay, so how |
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29:29 | that work? And and and how that actually work? So on this |
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29:34 | we start with some initial energy A. One, A. Two |
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29:37 | B. So this B. Is . A. One A two are |
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29:43 | here. So you have some uh have some charges which reside down |
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29:50 | And This is this is uh a . Okay. And then at two |
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29:59 | some irradiation during the radiation charges in one will jump to be But |
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30:08 | But when he returned he returned to . two As they fall, they |
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30:13 | be re excited. So the idea , you want to overpopulate one level |
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30:19 | this case a. two at the of a one. That's the |
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30:24 | Um And then once it's completed, everything has been moved from A. |
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30:29 | to A. Two. And I know all the details. I just |
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30:34 | this conceptual idea. Um And then radio frequency signal, I used to |
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30:43 | say R. F. I just out radio frequency that it takes to |
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30:51 | Back to a one always. I to go from a one to |
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30:56 | two that's proportional to the fuel So that's how it works. But |
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31:01 | the idea is that there's a there's lamp that pumps it, it excites |
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31:08 | that change in their level of uh levels. And that energy level is |
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31:18 | to the field strength, if that sense? That's how those work. |
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31:25 | , so now let's go to survey of gravity or a magnetic survey. |
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31:32 | you might want to survey an entire or an exploration play or a specific |
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31:39 | or in the case of an engineering , you know something, you |
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31:43 | some ah piece of land or something that. So there are things to |
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31:54 | . We want to consider the the of the target. Uh what sort |
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32:00 | density and magnetic susceptibility contrast you would to see what kind of rock properties |
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32:06 | expect to, what kind of resolution need to um you know, to |
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32:12 | detect the target and then um something I do a lot that's often |
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32:17 | make a feasibility model. Stick these these variables, you know, use |
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32:23 | basin size or the or the study size, target depths, rock properties |
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32:32 | then forward calculate what the what those look like and see if, if |
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32:43 | data can resolve that. So that's way to do it. So, |
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32:47 | survey method um that depends on the as well. So there may be |
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32:51 | issues, is it marine or mountainous, desert, jungle etcetera and |
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32:57 | stuff. Like is there a war on? You know, you're not |
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33:02 | be doing a gravity survey in, know, in Kiev these days. |
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33:05 | probably not gonna be, you advisable. Um And then is it |
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33:12 | to be like individual stations, are gonna dynamic? You know, you're |
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33:16 | to have a moving platform, like aircraft or or a boat or something |
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33:21 | that. And then of course the , is it gonna be you know |
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33:27 | how how are you know, what the intervals between lines or stations that |
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33:33 | you going to need to effectively you , resolve your target then? Of |
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33:39 | . How much money do you So these are ideas. These are |
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33:43 | to think about when you're going to a survey. So let's go through |
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33:48 | one on one survey resolution. It of course the size of the target |
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33:52 | its signal strength based on rock Special resolution depends on the sampling of |
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33:58 | field and of course the amplitude will on the sensitivity of the instrument, |
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34:04 | the field, the size and depth the source controls the labeling. This |
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34:08 | kind of a kind of a rule thumb thing to step the bottom in |
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34:12 | box which is important. And they be close enough together to detect the |
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34:20 | but they also you have to have of them outboard to capture the entire |
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34:24 | that the source is going to Um I should make a note on |
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34:31 | sampling sampling wide enough. Um No lost a regular sample provided that the |
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34:50 | frequency is greater than twice the highest component. I that's Nyquist right. |
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34:57 | means that the spacing of measurements must less than half the minimum wavelength. |
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35:05 | , so this is the bottom. is the rule of phone sources typically |
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35:09 | anomalies with wavelengths that are on the of four times their depth. That's |
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35:16 | four times the distance from the instrument the source. So that's important. |
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35:23 | when you're have an airborne platform because have to count the not just the |
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35:29 | below the surface, but the distance the surface to the nominal elevation that |
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35:36 | flying at. So the wavelength, lambda equals four dot Z. |
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|
35:44 | So dot the extra line station is times that. Alright, so that's |
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35:49 | important rule of thumb to remember. spatial sampling in land based surveys, |
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35:57 | grid approach is commonly used and it's know like in two orthogonal directions in |
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36:09 | surveys and airborne surveys, you'll have sort of survey line versus tile line |
|
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36:17 | . So surveying is always all about loops. You want to reoccupy stations |
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36:23 | you want to tie lines that you've or or marked out or sailed. |
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36:33 | you can minimize those missed ties between line intersections. Or you can or |
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36:39 | minimize when you re occupy a station in loops for like a land gravity |
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36:45 | , you want to re occupy one your stations so that you can tie |
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36:49 | miss ties or tie the drift of instrument. Okay, uh Special sampling |
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37:00 | um between discrete measurements sets uh sets limit on minimum wavelength. And talking |
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37:06 | that shorter wavelengths can only originate from long wavelengths can be so long wavelengths |
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37:13 | be produced by shallow or deep But that's that's really not true in |
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37:18 | real world. I mean it can your sources are, you know homogeneous |
|
|
37:23 | you know, that's just not Right? So I will show you |
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37:28 | I mean by this later. But this long wait list can be produced |
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37:33 | shallow sources is technically correct. But what happens is you have a long |
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37:39 | anomaly. Sure. But if it's shallow source there will be short wavelengths |
|
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37:45 | on that long on that broad And those short wavelengths will tell you |
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37:50 | deep the sources. So this is is really an old school idea. |
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37:56 | don't believe, I mean I need express that butter. So the choice |
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38:00 | profiles and the orientation of these They place limits. Right. So |
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38:06 | spaced lines. Mean that as I talking yesterday, even though you're sampling |
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38:11 | line for like a moving platform and or airborne, it's the spacing of |
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38:17 | lines that actually limit your resolution in of making a grid. Right? |
|
|
38:25 | then of course the orientation of your lines that that puts in a spatial |
|
|
38:32 | mutual bias into your data. So often folks like to fly for |
|
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38:39 | surveys in the dip direction because I want to enhance those features. Those |
|
|
38:45 | that they know about. But when think about it, if you know |
|
|
38:49 | them in enhancing them is only going tell you more about what you already |
|
|
38:54 | . So quite often it's good to oblique to these main structures or even |
|
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39:00 | if they're there, they're dominant, gonna come, they're gonna show up |
|
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39:05 | but you're gonna you're gonna especially, know, you're gonna especially bias against |
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39:11 | features that might be dipping in an to that and those might be |
|
|
39:16 | So those are ideas to think about terms of just survey design. |
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|
39:23 | so there are whatever 46 different types gravity surveys and that's sort of been |
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39:30 | about that indirectly. But land So so there you're out there walking |
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39:36 | or you're jumping around from using a or a helicopter or something from different |
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39:43 | and you make measurements at individual You surveyed those in, then you |
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39:49 | that data somehow. And then we borehole gravity gravity. So we can |
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39:56 | we can do borehole surveys. So are of course an individual holes. |
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|
40:03 | could, if you have a field might do these in a field and |
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|
40:07 | a really I mean I don't know I've ever seen that done. I |
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|
40:11 | I've seen a lot of literature and but I don't know if I've ever |
|
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40:15 | one where they did a bunch of measurements in the field. But I'll |
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|
40:21 | that's been done. I mean Amoco to own a borehole tool I think |
|
|
40:26 | they used to do a lot of surveys back in the day. Um |
|
|
40:33 | was bought by BP F. I maybe 20 years ago or so. |
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|
40:40 | Amoco was one of the original companies Standard, which was one of the |
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40:45 | companies. Okay, so as I this water bottom instrument. So there's |
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|
40:50 | bottom surveys and I don't know very , you know, Yeah, I |
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40:56 | know that there's this big survey. these stations that were measured on the |
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41:03 | coast uh platform out there. I'm shelf but I don't know any others |
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|
41:12 | honestly. It's not, I haven't , I could probably find some if |
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41:16 | look but I just don't know. then of course marine surveys um they |
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|
41:23 | they are all over the place. mean every passive margin, you know |
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|
41:30 | around, you know in the gulf Mexico, the east, in both |
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|
41:35 | both flanks of the central and south oceans, the north atlantic oceans around |
|
|
41:42 | um in the, you know in southeast Asia, all around Australia. |
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|
41:51 | And in fact, you know, open file marine gravity data that you |
|
|
41:56 | you can download for the world and free. So and then there's airborne |
|
|
42:05 | . Airborne gravity wasn't a thing until the 90s. I mean people were |
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|
42:12 | it in the 80s but it really wasn't viable. Wasn't just wasn't good |
|
|
42:21 | . They didn't have ways because the is that you're bouncing around on the |
|
|
42:26 | and you're producing accelerations that are just , you know, instrument just can't |
|
|
42:33 | . So you actually have to have which are a kind of gravity meter |
|
|
42:39 | that are accurate enough to correct for turbulence to be able to correct because |
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|
42:50 | the turbulence the from from the it's just like, you know, |
|
|
42:57 | and orders of magnitude greater. The acceleration of those is just far and |
|
|
43:04 | greater than the acceleration of this earth . So but since the late |
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|
43:10 | the mid to late nineties, these the instruments and the survey basically the |
|
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43:16 | , the accelerometers that they use to for the for the turbulence have are |
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|
43:24 | enough now to do that. In they're good enough now to the flight |
|
|
43:29 | after surveys. So they're taking off then there's satellite gravity. Now there's |
|
|
43:39 | there's two kinds there's where the meter actually installed on the satellite and I |
|
|
43:44 | like to grace mission that we talked yesterday but there's also granted this determined |
|
|
43:51 | I mentioned this but it's determined by the height of the ocean surface, |
|
|
43:57 | isn't, as I said, there's exponential surface or the Joyed. And |
|
|
44:02 | again, I see I keep saying , you can't forget that now. |
|
|
44:06 | and it calculates free air from that surface. Okay, the best |
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44:17 | the best data in terms of you know, in terms of amplitude |
|
|
44:22 | resolution, land gravity is the best is the second best. Um I |
|
|
44:30 | well okay borehole and borehole and and about the marine? But they're there |
|
|
44:37 | you know, they're rare. You'll see those marine is pretty good. |
|
|
44:41 | then airborne. So I think I some resolution tables. I'll show you |
|
|
44:47 | . But just here's a couple gratuitous of gravity instruments in action. These |
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|
44:55 | all relative instruments. Uh No not one. This is I guess this |
|
|
45:01 | a L. R. Meter. what my figure says here. So |
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|
45:05 | you know your your environment. This maybe maybe a pasture, maybe wooded |
|
|
45:12 | , desert area, mountainous in the I think this might be from Prudhoe |
|
|
45:19 | . So this might but they did Eleanor and Prudhoe Bay. And then |
|
|
45:22 | just somebody down there reading it, know, writing down his notes, |
|
|
45:28 | making a terrain correction. So and yeah, these are all land surveys |
|
|
45:37 | then so marine surveys, the issues because it's a moving platform. Um |
|
|
45:45 | have accelerations from the moving platform and can degrade. So um and often |
|
|
45:53 | I said that there's a ton of but at least in the industry whenever |
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|
45:59 | oil and gas companies whenever they contract is like some seismic data, some |
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46:05 | data to be acquired. As I , like over a passive margin. |
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46:13 | uh, they often will add on and magnetic instruments. And so basically |
|
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46:22 | course in there and the cost added is like, you know, pennies |
|
|
46:28 | the dollar. It's just nothing, know, it's just a few |
|
|
46:32 | So obviously, you know, with to survey design, you're just at |
|
|
46:36 | mercy of whatever they're gonna, they're go out there and shoot and that's |
|
|
46:40 | the way life is. So, know, I mean you don't have |
|
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46:45 | control over line spacing or tie lines anything like that. Um, and |
|
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46:53 | of course to deal with the ship . You know, the instruments are |
|
|
46:59 | on a gyro stabilized platform and then damped a little bit, they're out |
|
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47:05 | filter a little bit. So so gravity is basically time averaged over several |
|
|
47:12 | . So it's not, it can't nearly as good as land, you |
|
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47:17 | , letting the instruments settle down and it, measuring it as over |
|
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47:23 | And then those moving platform uh issues greater with airborne platforms and they fly |
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47:32 | from either from helicopters or from fixed . So they can do it both |
|
|
47:38 | . Now this, this is a and it's a big, it's a |
|
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47:43 | , it's a single engine aircraft but big and in that they have the |
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47:49 | instrument, but you can see at back end of that there's a little |
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47:53 | that has a magnetometer. So that there is flying gravity and Magnetics. |
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48:03 | And your notes probably say 10-15 That just shows you how long I've |
|
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48:09 | teaching this class. It should not , I'm gonna change I changed it |
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48:14 | years. So mm So airborne. they have to be in addition to |
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48:26 | the asthma and the the flightline space they have to worry about the variable |
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|
48:33 | flown. And they can fly either which is constant altitude or what we |
|
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48:39 | drape surveys or it's a constant terrain . Um If if you're a relatively |
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48:47 | area then you know you can you fly just constant parametric which is very |
|
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48:53 | to work with. But these days drapes they want to get as close |
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48:57 | the source as possible. So everyone a drape survey. And yeah, |
|
|
49:04 | I said, accelerations can be problematic grabbing. That's absolutely true. Um |
|
|
49:17 | , so here's just an example of flight lines basically. This again, |
|
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49:20 | is a caravan, there's a gravity and then of course there's the stinger |
|
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49:25 | has the magnetometer. Um for The flight path should include a similar |
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49:32 | of flight line. I mean in perfect world, you would fly the |
|
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49:36 | lines basically I've organized and I planned that way. But what people typically |
|
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49:42 | is because you know it costs money fly these things. They fly a |
|
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49:47 | of survey lines in their preferred orientation then they just tie those and the |
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49:53 | and the ratio is typically 3215 to , even as much as 10 to |
|
|
49:59 | depending on what kind of survey, know what they think they're doing. |
|
|
50:03 | um yeah and again this puts in spatial bias a spatial tuning as I'm |
|
|
50:11 | it. Okay, so airborne gravity is filtered because of these, the |
|
|
50:21 | . And so here's a little this is from, I don't even |
|
|
50:26 | the source of this, but this an old example basically Milligan's. So |
|
|
50:32 | scale here goes, you know, to 200 mg, not just |
|
|
50:36 | Y. I the biggest anomalies in world after processing are like on the |
|
|
50:42 | of 80 mg, sell them over . So having it having 100 million |
|
|
50:52 | only, that's pretty darn big. So this is this is a huge |
|
|
50:58 | and it's over. Let's see these these are in kilometers. Yeah, |
|
|
51:03 | is a 48 100. So this 40 that's 200. So this is |
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51:09 | , this is 400 kilometers across. this is this is stretched over a |
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51:14 | area, but then you just see the how the time average, the |
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51:20 | to smooth out the turbulence Flying at . That's that's pretty fast. I |
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51:28 | that's actually incredibly, I think like day like I think a caravan flight |
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51:35 | fly, they can fly on your 100 kilometers an hour, Maybe even |
|
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51:42 | little less. Maybe 100 knots. don't want transit translates. Okay, |
|
|
51:48 | how are satellite data? Said it an L. Timber. So you |
|
|
51:52 | have one of the missions was Jason question real quick on the previous side |
|
|
52:01 | like the anomaly. So what what of feature could we be looking at |
|
|
52:06 | could be that anomaly like a ridge something or No, I normally is |
|
|
52:12 | big will learn this. But basically amplitude anomalies. Remember I showed you |
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52:19 | pitfall yesterday with regard to Magnetics in Gulf of Mexico that that the big |
|
|
52:25 | amplitude anomaly. It couldn't be a because it would require like 25 km |
|
|
52:31 | throw on a fault which is not . Um same thing with gravity 200 |
|
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52:41 | anomaly could not be a fault because would the throw on. It would |
|
|
52:46 | be not physical. So that means probably compositional. So you're going from |
|
|
52:51 | sort of basement rocks that maybe, know, lower density than other basement |
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|
53:00 | next to them. And yeah, you're going from maybe whatever granted to |
|
|
53:07 | granule, like maybe there's some you know what I mean? So |
|
|
53:12 | , mostly big giant anomalies high empty are typically produced by composition not, |
|
|
53:20 | structured and it's kind of a rule thumb, but it's it's pretty |
|
|
53:24 | Yeah. Good question though. Okay. Okay. So getting back |
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|
53:29 | the how the satellite data are So All right so here's our ellipse |
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|
53:36 | R. W. G. Reference spheroid. And here's our |
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|
53:40 | Oid. And so the ge I don't know why they have a |
|
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53:46 | surface. It's the mean it is mean surface height. So I don't |
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53:50 | what's going on. Ocean surface Oh so I guess they're saying that |
|
|
53:58 | the ocean goes up I guess it's tide or something like that. But |
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|
54:04 | so the altimeter like shoots a laser down and it measures the height of |
|
|
54:10 | of the sea surface. That's a weird. I don't know if I |
|
|
54:15 | I'm going to go on that Figure this out because So what happens |
|
|
54:22 | the laser does penetrate. But I it's only like about 15cm or maybe |
|
|
54:29 | a little bit more. That's why that's why when you get into shallow |
|
|
54:34 | shallow waters, satellite data is less because the laser its interference with the |
|
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54:44 | bottle because it's penetrating. So I they make a little correction for the |
|
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54:50 | of the laser. So that's something should know I guess shouldn't um I'm |
|
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54:57 | check check um sad grab G. all timber but everything I told you |
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55:10 | correct. And my confusion ists with to this figure. It's not really |
|
|
55:16 | exactly. Okay. Alright so here's bunch of words about satellite gravity. |
|
|
55:23 | There's been there's been over the six missions Geo SAT which is a |
|
|
55:29 | . S. Navy E. S. One E. R. |
|
|
55:31 | . To cross at two. That's E. S. A. And |
|
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55:35 | Topex Poseidon and Jason one. That's Nasa. Uh C N. |
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55:43 | S. Is that that's the I don't know what the initial staff |
|
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55:52 | but it can be used. They out to average out C state C |
|
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55:57 | and sea level uh produce after removal surface disturbing factors. So I guess |
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56:04 | what that figure is showing. It's tides and currents and stuff and you |
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56:09 | those out to provide a measurement of geode. There's a horizontal gradient is |
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56:17 | by definition and the satellites are There are the satellites are about 800 |
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56:24 | above the surface and they're moving at ground speed of about 7m/s, |
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56:31 | And They're they're making an altitude measurement instantaneous C service every 10th of a |
|
|
56:41 | . And then the distance between so sampling along line is yeah right 700 |
|
|
56:47 | . So mhm. Um Then they have many other just keep orbiting the |
|
|
56:54 | and they just stack that data out same way. You would you know |
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56:58 | reflection data. Um We're not the way but the idea is the same |
|
|
57:05 | measurements are averaged over 10 the footprint the laser beam. It says here |
|
|
57:12 | about one or two kilometers but for for eight m wavelength it's raises about |
|
|
57:18 | kilometers um resolution They claim is 3-5 gals over 4-8 km. I think |
|
|
57:30 | like again like an rms thing. think if you compare the satellite data |
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|
57:36 | you compare it to uh um if can if you compare it to like |
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57:49 | data I think the numbers you get more like five Milligan's maybe plus or |
|
|
57:56 | a couple. So that they have it's pretty close. But I think |
|
|
57:59 | in terms of wavelengths I think it's like about 12 10 plus or minus |
|
|
58:06 | maybe 12 plus it's not it's not kilometers it's just now. So anyways |
|
|
58:13 | sounds like graph is beautiful because it's over the world's ocean basis. It's |
|
|
58:18 | beautiful data. Um Okay and then of course the kind like I said |
|
|
58:26 | the instruments actually in in the satellite you know as we said Grace launched |
|
|
58:34 | 2002. So it's been up there over 20 years now. And uh |
|
|
58:41 | been using this lots of papers there's a session or two on Grace data |
|
|
58:46 | the A. G. U. you can see here they're actually like |
|
|
58:50 | um Inferring changes in currents and water from measuring the surface of the ocean |
|
|
58:58 | here in these in these trade these over the north atlantic. So And |
|
|
59:04 | here are these neat figures they Remember these are like tiny, they're |
|
|
59:09 | , you know, variations. These are probably on the order of, |
|
|
59:13 | know, less than a meter, on a meter level. So these |
|
|
59:18 | enormously perturbed models. But, you , very interesting. And the same |
|
|
59:26 | goes is the same. But this a this is a satellite gradient |
|
|
59:30 | So you have uh here's the instrument that sits in the in the |
|
|
59:36 | I guess. And yeah, this , let's see, this is weaker |
|
|
59:44 | pull and stronger. Very nice, , very quantitative um launched in 2009 |
|
|
59:54 | state of the art for 2009, guess. And they're trying to infer |
|
|
59:59 | deuttel fluctuations, you know, So what's going on here. If you |
|
|
60:04 | the picture I showed you the These are where the big highs and |
|
|
60:07 | are of the G. OID. . So what is the what is |
|
|
60:15 | relative accuracy of all these all these and and and uh um data |
|
|
60:26 | So this is instrumentation. Well, it says surveys here. So I |
|
|
60:32 | we're talking about time. Yeah, . It was very, very |
|
|
60:38 | Um I'll just take it as words . So the first one was done |
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|
60:43 | long time ago now. And I Dave chappelle used to work at |
|
|
60:47 | he published a paper and he so this is going this is a |
|
|
60:52 | log and wavelength versus log in amplitude . So this is really a big |
|
|
61:01 | difference going up and across and published bars. So he doesn't have a |
|
|
61:08 | of confidence in Waveland resolution. Land or marine. I guess everyone |
|
|
61:15 | But you can see absolute measurements are absolute best of course and boreholes are |
|
|
61:24 | better than land. So um I guess I had land and borehole |
|
|
61:30 | but I did have water bottom, . And then chip born on the |
|
|
61:34 | wavelength resolution but less in terms of because because you have that vertical motion |
|
|
61:42 | the turbulence, the boat going up down that just creates a greater |
|
|
61:47 | And then airborne Up here and then here now satellite in 98 wasn't nearly |
|
|
61:54 | good as it is now. I showing you 2014, 2014 there's a |
|
|
62:02 | paper by sand. Well here it , right here, the landmark paper |
|
|
62:07 | science by land Sandwell and others. yeah, So even after fair heads |
|
|
62:15 | here in 2012 but it's the same of thing. He has great geometry |
|
|
62:20 | here, but it's again it's a log plot. Chef born and he's |
|
|
62:27 | showing arrows, showing that uh I that they are getting better. So |
|
|
62:33 | a handle that gives you a handle what the relative resolution of these things |
|
|
62:39 | but but I wouldn't take, I take any of this stuff as being |
|
|
62:45 | today. I mean I would say general trend, the placement of these |
|
|
62:49 | but I don't think this is accurate . Um slide 30 comment accuracy. |
|
|
63:02 | making a point here to comment on . Um Okay now I'm gonna show |
|
|
63:08 | this little um this little case history which basically in Prudhoe Bay remember this |
|
|
63:17 | the north slope of Alaska. So only people that have enough money to |
|
|
63:21 | for that are the biggies Exxon Um Arco from back in the day |
|
|
63:29 | was up there but you know no oil companies can they just don't have |
|
|
63:35 | cash to do that. So Okay the first survey was 1994 and then |
|
|
63:48 | reoccupied those stations, these are gravity and they reoccupied those stations three years |
|
|
63:55 | . And the idea is that there injecting gas and water into you know |
|
|
64:06 | into wells around the production wells to to you know enhance the recovery. |
|
|
64:13 | the idea. And then uh this and her last name is I can't |
|
|
64:19 | her first name but she she um think I have her name here. |
|
|
64:30 | can't find her day but she she at Exxon at that time and she |
|
|
64:39 | of this paper uh discussing this four . You know this time lapse method |
|
|
64:48 | monitor the water flood and this this a huge deal. I mean everyone |
|
|
64:52 | like whoa. I'm always talking about and her co authors were Ferguson. |
|
|
65:01 | was Ferguson is that was a professor U T. D. The other |
|
|
65:06 | authors were um uh yeah, hair there was that Exxon Ferguson and Carl |
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65:16 | were at UtD University texas Dallas and guy named brady was with our co |
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65:24 | that's with the cola of that original . Um and then, and then |
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65:34 | reoccupied that station in those same stages 6000 to 2003, 56 and |
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65:42 | And around about 2003, they started integrating this with not just Eleanor |
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65:50 | So they use Eleanor meters up to , I think 2002 or three, |
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65:56 | they introduced the absolute meter around this . And then I think they dropped |
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66:03 | towards the end when they're just using end. There's some overlap with the |
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66:08 | meter. And then they and then published papers in 2011 and 2008 2 |
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66:15 | 2008. And reporting on this this whole experiment, which was, |
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66:20 | know, just a huge deal was of talks and a lot of, |
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66:24 | know, a lot of excitement around stuff. Okay, so if you |
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66:29 | know much about the north slope, this, this is basically, there's |
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66:33 | basically this enormous sin klein and anna . So this is the kovel trough |
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66:40 | the barrel art. So this is is with the you know this these |
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66:45 | are you know situated just um Outboard the Brooks range here. Right? |
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66:51 | it's kind of like a four land of over print because this is technically |
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66:59 | margin out here. But you have four land structure, this broad sort |
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67:05 | asymmetric basin in board and a flexible out board which is the barrel arch |
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67:13 | this is the cross section through So and this paper was published in |
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67:21 | tonight. I mean it's not related this survey but it's just a really |
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67:24 | figure to show you the the regional of the of the North Social NPR |
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67:32 | and Anwar. Our NPR is the Petroleum Research Reserve area or something like |
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67:39 | . And that's where like biden's been to kind of keep gas prices down |
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67:46 | Anwar was protected but I think they're up in there now. So but |
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67:50 | was a wilderness protected area for a time. Um So the first Alaska |
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67:58 | sale was in 1960 for companies which doesn't exist anymore. I think |
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68:04 | still some gas station that's the gas with the green dinosaur, the green |
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68:10 | brachiosaurus or brontosaurus or whatever is Sinclair bp leased most of the koval trough |
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68:17 | is which is down here. But and Exxon least prudhoe bay which is |
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68:23 | here which is just on the out the you know the flank of the |
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68:28 | arch In 65. And then they the largest discovery in 68 in the |
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68:35 | arch. Um The 5000 ft Yeah the folds are five. Yeah |
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68:44 | relief is 5000 ft on these Um Of the what the hell's Mirian |
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68:53 | which is a previous recipient through lower cretaceous rocks. Okay so So then |
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69:07 | is hairs paper. So then in Hair reports on the first feasibility |
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69:12 | part one of this four part study they demonstrate the viability of the water |
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69:19 | surveillance. And they added this surveys out 94 97. So the reservoir |
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69:25 | about 8500 ft down and it dips the south right into the Colville |
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69:32 | Um In the preliminary test they had of 5 to 10 micro gals which |
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69:40 | you know five which is a well to 5, 10 5 micrograms which |
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69:51 | 5000 to 1, 1/100 of a . Now they did some feasibility |
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69:58 | Some modeling suggests that after five years water injection Um the graphic difference would |
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70:04 | about 100 micrograms. After 15 it would be about 180, Based |
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70:10 | this and the worst case inversion scenarios 10 to 15 micro gallons of |
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70:18 | So they need to, they need have they need to estimate the mass |
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70:24 | by 10-20% to make make it Right? So this paper, Heron |
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70:35 | Exxon? Yeah, same players. possible zones were modeled um to invert |
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70:44 | gravity between gravity stations. The gravity are from 762 m to 1200 |
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70:54 | So on the order of a So that's 3000 ft. Okay, |
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71:03 | . Um Okay, so then now looking at after all these surveys are |
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71:12 | , uh then they start rolling out three next papers. So after after |
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71:19 | , so they were collecting data all years, almost every year. They |
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71:25 | a year in '04. But then in 05 and six occupying the same |
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71:33 | . So in the second paper they about how they improved their their acquisition |
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71:39 | and instrumentation to achieve. Because they I mean this is they always did |
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71:45 | in january when Prudhoe Bay was iced and like they would drive around on |
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71:51 | equipment out there of course it's pretty cold and they would, you |
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71:56 | drill, drill through the ice using these augers that, you know, |
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72:02 | use for ice fishing and stuff. I remember the guys who talked these |
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72:07 | all the time what was going And they would, they were like |
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72:11 | the best way they could figure out to account for the density of the |
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72:15 | later, which is important. It like the correction because that mass |
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72:21 | you know, calculable frozen sea And they would take like a a |
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72:30 | pole like you know uh you know sticks you use when you ski for |
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72:37 | country skiing because they would have a edge, a little thing you could |
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72:42 | on that would that could when you it in the hole, it would |
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72:46 | on the bottom of the ice. could use that that length to |
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72:50 | Think so yeah, it was pretty cause they were out there. These |
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72:58 | giant track driven machine machines to go the occupy the different stations every |
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73:05 | but on the tables at the bottom left is that they have time and |
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73:10 | dependent factors. So the fact is of course latitude elevation, you |
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73:15 | and so these are the these are accuracy of the measurements, you |
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73:21 | pressure. They're worried about pressure. mean as many things as tides, |
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73:25 | course, tides are a big deal gravity corrections and uh seismic noise. |
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73:35 | then on the on the table on right single survey gravity and elevation |
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73:40 | So here's their error budget. So the tide and ocean load, one |
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73:45 | gal, they had to be within barometric pressure, one micro gal. |
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73:50 | on and so forth. Total less than 11 micro gal. So |
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73:55 | , so they said that they quoting paper, they adopted a highly redundant |
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74:00 | procedure. Kabul was statistically robust. just I'm chocolate because just like this |
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74:07 | verb age estimation of of a drift necessary to produce relative movement through. |
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74:14 | Yeah so um okay so Now with three, I haven't started any data |
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74:25 | . I'm gonna show you some Uh now this is surveys 2003-2007 And |
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74:32 | they this is using the a. , this is the absolute gravity. |
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74:38 | so they have 300 stations out That's all the little plus signs down |
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74:43 | . We have 100 and 50 square I guess. Uh surveys +3356 |
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74:53 | Um And precision they're saying is better five micro gowns. So now this |
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75:03 | Ferguson and akin that's you t d you grow and john see john |
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75:11 | I know john very well. He's consultant and then named brady again. |
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75:17 | brady was through all these papers. Well at least up to here with |
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75:23 | so he wasn't Arconada Bp because bp Arco and then um Yeah um Let |
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75:33 | see uh Polar motion. Yeah okay case of polar motion that was under |
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75:40 | sorry I'm jumping on behind. Oh okay. I'm sorry these these path |
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75:48 | a tree contours are are two ft two ft animals at 88 ft Yeah |
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76:04 | ft 2 ft. And so the the water bottom is really flat out |
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76:08 | in Prudhoe Bay. That's the point Okay let me just go on |
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76:14 | So here are results from those and you're looking at are the averages over |
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76:20 | years in the upper right? From , 2 years and B is three |
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76:27 | average and C is a four year . So 303, 206 and |
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76:39 | And then the color scale is the for all of them. And it's |
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76:43 | from looks like minus 30 to 70 plans 20 sold almost 100 Micro |
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76:52 | So a 10th of a mil igel range or just under 1/100 of a |
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77:00 | ago, I'm sorry. Yeah, are micro gowns, right? So |
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77:04 | hundreds of a miller go. So yeah, this is a tiny, |
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77:08 | range. But if you look at anomalies, they're really hang together pretty |
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77:13 | . I mean, it doesn't look just random noise, Right? I |
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77:16 | this is, I mean you do the sense that it's, there is |
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77:23 | bit of randomness in there, but definitely got signal in here. If |
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77:27 | ask me, especially with the four average. So what does this |
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77:32 | What it's higher judges that means. where I guess the water. So |
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77:38 | trying to force, that's where they're to force the, so this is |
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77:42 | arts through here and the code and trough is down here. So where |
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77:47 | the injection wells? Yeah, they're the south injection wells are down |
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77:53 | So they're right here. Oh I . So yeah, so that's that's |
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77:59 | response to the injection. So the is heavier and it's pushing things |
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78:04 | The water is accumulating down there. , that's what that means. |
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78:08 | Yeah. So that's just adding the which is higher density than than, |
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78:12 | know, oil. So and then is um uh one year and two |
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78:23 | averages. So here's just 05206. let's see the two year 032. |
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78:31 | I don't have, I have 03206 here. That's three years. |
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78:37 | so 0506 And then 0572 years and 06207. So these to add to |
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78:47 | this, I guess that makes And again it's the same color |
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78:56 | So these are pretty subtle changes. I think, I mean it doesn't |
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79:01 | that bad. I mean there's no where there's, there are some single |
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79:07 | . There are some single station which kind of like a dead giveaway |
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79:13 | you know, something's funny going on a single station anomaly is not something |
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79:18 | you want. Okay, so then the final paper Which was published later |
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79:28 | O. H. in '07 rally no age. Uh in this |
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79:35 | the authors were Ferguson again clopping from G Chen roof. You grow Siebert |
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79:41 | hair. She was a song by and brady. So brady was the |
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79:48 | the only braider and Ferguson were the authors that were in all four |
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79:56 | In any case the station is again the right the water injection. Now |
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80:01 | see now we have a really nice . So it said gas injection of |
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80:06 | blue, the Mondeo monitoring wells. bigger black ones, they had victor |
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80:13 | injection. I'm not sure what that , but that's down here. So |
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80:16 | injecting in regional areas as well. they're re injecting with gas up in |
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80:23 | . So it's pretty. And then these little gray ones, those are |
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80:27 | production wells. So this is a needed to say that is really well |
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80:35 | . Yes, it's six ft, ft contour. And yeah, they |
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80:40 | a GPS base stations to triangulate their positions. Then there's a cross section |
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80:47 | goes through here. So the water is expanding into the gas cat and |
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80:54 | the expected rate, but it's exhibiting symmetric behavior that is consistent with a |
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80:59 | degree of structural control. So that think there's some faults that are |
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81:06 | affecting the flow down there of of the injection and the flow of |
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81:11 | , you know, being able to the hydrocarbons. So again here again |
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81:21 | . Uh, some of the cumulative this time, they're talking in terms |
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81:25 | cumulative mass distributions. So they're, decided to, they've taken their |
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81:31 | their version models and now they're you know, mass and I guess |
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81:35 | is killer tons. And so the year average, I mean I mean |
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81:43 | for the two year average 03205 is A 03206 isn't being in the four |
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81:50 | 03207. So you can see the steadily increasing in a systematic way. |
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81:58 | this is very nice. I think very impressive work. Um And then |
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82:06 | here is uh uh huh. More of mass 2, 2 and one |
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82:15 | . So kind of very specific and on their integration of reflection data with |
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82:22 | Well and this gravity, this is course these structures are they're not interpreted |
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82:27 | this, this gravity inversion there you know from reflection data but I |
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82:36 | know you'd you'd be hard pressed to me that there's some there's you |
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82:43 | um strong correlations but I mean with structures these structures, but maybe maybe |
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82:51 | some Yeah, I don't know, mean is so the over is overall |
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82:58 | and a trough to the south but going to be, you know, |
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83:03 | on that. There can certainly be superimposed on that broad feature. |
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83:10 | I don't know, I don't know how you can relate this mass distribution |
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83:18 | these map structures but yeah, I know, I mean this is this |
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83:28 | a high where there's not a low these are highs that are outboard that |
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83:34 | there before and this is a high it's a low and this is so |
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83:44 | two years before. Yeah. Yeah got me. I don't get anyways |
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83:55 | this this is this is claimed to pretty pretty successful so I don't know |
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84:04 | any other times. I'm sure there . It's not something it's not uh |
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84:09 | not like in my on my radar I don't really have a dog in |
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84:15 | fight so I don't wanna be too here but in any case it is |
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84:21 | is something that's a very famous study yeah there you have it. Okay |
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84:30 | switching to Magnetics. Let's see, to Magnetics. I've been blabbing here |
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84:40 | an hour and a half. Do want to take a break or do |
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84:43 | want me to drive on? Let's like a quick break if that's |
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84:50 | Sure you wanna meet here at Channel . That'll work. Okay. Alright |
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84:57 | me just that my connecting work. about that my connection went down so |
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85:06 | I don't know what happened. Well know what happened when I connected with |
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85:10 | . Sorry about that. Um Yeah know of course it's gonna happen today |
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85:21 | while I'm teaching, luckily luckily it back and we can we can resume |
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85:32 | can room resume the festivities. Okay all of the previous sections on gravity |
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85:42 | and you know I had a little of the Kobe study. But the |
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85:51 | was, you know, kind of method is and how good they |
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85:54 | how you know what you can measure them and the resolution of them etcetera |
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86:00 | . And then. Okay, so questions about this material so far? |
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86:08 | good so far so good. I'm gonna take that as a positive |
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86:15 | . Um Okay let's let's talk about texas magnetic survey and they're quite similar |
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86:26 | there's a couple of differences. So we, you know, we can |
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86:32 | land surveys and we can do marine as well. And in marines they |
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86:38 | have the magnetometer on the boat. put it, they drag it behind |
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86:42 | boat in a and whatever. Uh know a vessel that they call a |
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86:51 | because the boat is made of metal often and there's just a lot of |
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86:56 | related to that. They also have toll marine magnetometers. There's a fair |
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87:05 | of literature out there on the results using this instrument. It's pretty |
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87:12 | especially if you're mapping. Um Sea spreading announcement. Remember I talked about |
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87:18 | Jurassic magnetic quiet zone yesterday where there , there were fluctuations between the pole |
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87:25 | versus was really fast and the field very weak. So if you measure |
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87:32 | the sea surface like out in the pacific where there are some of the |
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87:37 | , somebody's Jurassic aged magnetic crimes. know the sea floor reversal bits of |
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87:47 | atmosphere that's been reversed. Um, the surface, some of these anomalies |
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87:55 | the reversals. They just sort of and form big broad regions of highs |
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88:00 | lows. But they've done some deep experiments where they're right on top of |
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88:06 | sea floor and they can really define reversals very well. So yeah, |
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88:14 | toes is a thing. It's pretty . And of course airborne Magnetics is |
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88:19 | a big deal. Um, you do it with a fixed wing aircraft |
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88:23 | helicopters. Um, with helicopters quite they're, they're a secondary, |
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88:32 | you know, there's a lot of E. M. Surveys, especially |
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88:38 | mining purposes and to stick a magnetometer , on, on the aircraft is |
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88:46 | very simple, very easy to So they do that. And then |
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88:52 | , satellite, uh, they use flux gate and cesium vapor And of |
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88:57 | , MAg sat, I showed you , I showed you black and white |
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89:01 | of it before. But here's a image of Mag said again. You |
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89:05 | , it's just like there's a single wavelength that's percolating through this. Now |
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89:11 | map is plus or -20°20 gammas Nano where I think the one I showed |
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89:19 | last night was customized 11. So has a little bit more of a |
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89:23 | on it. I don't know what deal with that is, but the |
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89:28 | quality of magnetic anomaly data is actually , Um Next would be marine and |
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89:42 | data is more noisy than marine or . And I think that's just because |
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89:49 | so close to the source. It's . It's not intuitive but the best |
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89:56 | best magnetic data the highest quality is data. So marine service there's the |
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90:05 | he's holding uh the fish that has magnetometer inside of it. It's towed |
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90:12 | . Of course deep Tojust be the thing. Except this is down here |
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90:18 | and like a lot of marine gravity their collective with reflection data. And |
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90:23 | they're just an add on. And it's like pennies on the dollar and |
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90:27 | very much and the same caveat supply spacing, sampling um tying ties with |
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90:40 | stations as well. Um Yeah I know what the nominal distance is that |
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90:49 | drag these behind the boats is look yeah you have to make a you |
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91:00 | to make a heading correction. Yeah also with regard to, well I |
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91:08 | we'll talk about this stuff. We about processing. Okay so airborne surveys |
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91:16 | measurements clicked by aircraft since the 19 . Remember that first U. |
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91:22 | G. S. Survey was was 49 47 something like that anyways. |
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91:28 | remember the USgs made the first survey But they can they can be collected |
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91:36 | variable heights. Sometimes they fly into surveys at two elevations and done a |
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91:42 | with those calculated the gradient. Again drape and drape survey, we just |
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91:50 | of follow the train and a constant called barometric again same as before. |
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92:01 | for shallow sources, you want to close to the source. So here |
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92:05 | two planes with stingers attached. I know what kind of aircraft it looks |
|
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92:10 | a titan. This here, this here, this is a titan, |
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92:14 | Cessna titan. And this picture used hang on the big version that used |
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92:23 | hang on. It says Arrow Service the top there it was It was |
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92:30 | the lobby of Aero Service. I at Arrow Service in from 81 to |
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92:36 | . This is the first job I in Houston when I moved down here |
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92:41 | michigan and before michigan I was in army, they hired me over the |
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92:48 | because of my experience in the I was I was a photo |
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92:53 | I was. So the jets would missions for us. I was in |
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92:59 | intelligence and the jets would fly missions us and they would, you know |
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93:03 | pictures of equipment, tanks, and personnel carriers and stuff like that and |
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93:11 | would identify those those equipment. We we would mobilize the air bases, |
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93:17 | Force bases and then The you know F4s would fly our missions for us |
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93:22 | we would debrief the pilots and then the imagery and make a report. |
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93:30 | I had I had a good you know, a good experience of |
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93:33 | at airborne imagery. So they just and in those days that was before |
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93:40 | . Right. GPS didn't really take until the nineties, late eighties and |
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93:45 | um mental eating. So when they surveys over land they would take |
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93:53 | They would have a little 35 millimeter that would take pictures, you |
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93:58 | continuous, very, you know, shots. And then we would take |
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94:05 | that big long strips of film and at a light table with with a |
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94:11 | event. And and you know pick points to track the flight path on |
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94:20 | map and then read those coordinates and that would be input into the |
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94:26 | That's how they would position the data the for the for the survey in |
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94:34 | case going now going from there to before I started working for myself In |
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94:42 | and 97 I was working for my survey company. They're based out of |
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94:48 | and they this airplane, this very airplane in the lower right had |
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94:54 | you know, they ended up owning through a bunch of different company acquisitions |
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94:58 | sales and stuff. And I organized survey in Marignane base in Peru for |
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95:08 | . And they flew there. We four guys in the crew down |
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95:11 | They flew the survey and then the was finished. They mobilized that aircraft |
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95:16 | of there and they were gonna fly marignane from the Amoco base station to |
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95:22 | little jungle town called Pucallpa. That's in the in the jungle uh east |
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95:31 | the east of the Andes and the just went missing. The they don't |
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95:38 | what happened to the crew complained, just went missing. So you know |
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95:44 | those days there was a lot well little planes go missing all the |
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95:47 | down there because people that you know the drug trade down there, they |
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95:54 | little planes for that stuff. So just steel planes kill people, stuff |
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95:59 | that. So anyways that plane um known for a long time. I |
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96:04 | for a long time um that incident lost another plane down there and two |
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96:11 | were killed and then we found that that ran into the side of a |
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96:17 | . And then um the last incident that we had a pilot that was |
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96:25 | by the pool in you know after flight and he had a heart attack |
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96:33 | fell into the pool and drowned. we lost like seven guys in like |
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96:40 | months. These are all surveys that organized. It's not my fault that |
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96:46 | this bad stuff happened. That was I decided I was gonna go back |
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96:52 | school, get a PhD. So started my company And started working on |
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96:58 | at the same time in 97. anyways every time I see that photo |
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97:05 | remember that. Um So why am showing it here? I don't know |
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97:09 | there you have. Okay so um surveys just like marines, gravity |
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97:20 | you know that you're concerned with the same things in terms of the flight |
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97:25 | spacing, how much you tie And uh you know the biases was |
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97:33 | to the orientation and the spacing of lines and the altitude in terms of |
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97:39 | from the source. These are all for flying surveys. So here's some |
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97:48 | of instruments. So these are birds they also call them. So they're |
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97:55 | fish in the bird's airborne survey. here's the helicopter, they also do |
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98:02 | with fixed wing, I don't have picture of a fixed wing aircraft with |
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98:05 | of these things. And here is here is a helicopter with a Stinger |
|
|
98:14 | they fly surveys with ultralights. In . In fact, let me show |
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98:19 | something. Let me see here. is it at uh where is it |
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98:25 | here? It is this I just this this morning. So this is |
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98:32 | they're doing surveys now with with drones uh I think pretty successful. But |
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98:42 | now the F. A. So can only do them. No I |
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98:52 | only see the zoom meeting like login or something. Can you see |
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99:00 | Stephanie? No sir, not Hold it. I'll stop it. |
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99:05 | I can only see your uh I only see the zoom meeting. There |
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99:10 | go. Okay, now I can it. No, but now I |
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99:19 | now it's on the screen now. , Alright then. So this is |
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99:29 | , I found this on the internet , which is a big instrumentation company |
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99:35 | this is one of their promotional bits . You still see it? |
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99:43 | Okay, so this is there's the , it's in that little So I |
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99:54 | they're flying a mag survey over this . Yeah, now that's got to |
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100:22 | very cost effective. Okay, all right, sorry about that, |
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100:36 | sorry about it, but I just that that was kind of fun. |
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100:43 | we back out of the program Back under the slides. Not |
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100:47 | I'm still looking at Youtube. Do need to do something? Okay, |
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100:59 | I'm at the slide. Okay, . Alright, I used to have |
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101:07 | little video of this one. So a here's another drone that that they |
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101:13 | to launched with like a slingshot and it's got little hooks on the |
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101:22 | And I have this tool, this crane thing and the plane would just |
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101:29 | into it and it would, you , catch that wire and it would |
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101:35 | , you know, flip around and and land that way. But I |
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101:42 | the helicopter type drones are probably make sense to me. So yeah. |
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101:50 | , so, okay, I have little cash history of a deep toe |
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102:00 | survey uh in the in the the uh Iberia uh when they call it |
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102:13 | abyssal depths abyssal deep the I. . B. The Iberia. So |
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102:18 | is off the continent of West Iberia is Portugal and Spain. That's |
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102:24 | And they flew this they I'm sorry this is marine data. They acquired |
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102:32 | data in and around some ODP So um it's a fluctuating magnetometer and |
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102:46 | they towed it over some some magnetic and also as well as some some |
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102:55 | type, some mantle rocks which were as the basin opened. So which |
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103:02 | a which is uh which is something has a lot has had a lot |
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103:08 | attention ever since then. I mean it's been you know it's been It's |
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103:15 | over 20 years and it's still like just are in love with this |
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103:23 | Okay, so this is a reconstruction of the study area. So here's |
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103:29 | right? So there's Spain and Portugal there there's France 19 and then it's |
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103:36 | reconstruction. So it's a reconstruction of the age of the reconstruction. Um |
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103:48 | closing this Atlantic, the North Atlantic gotta be like a 60 m. |
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103:53 | reconstruction that's in 60 to 100 million , something like that. So when |
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104:01 | closed the central atlantic and the mediterranean actually have overlap in the in the |
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104:11 | sea. And I'm sorry the leprosy in the north atlantic. So um |
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104:24 | the area where they're interested in is here, it's called the uh the |
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104:33 | abyssal plain. And that area right is where they did the deep |
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104:37 | This just gives you some context for . So on the right here is |
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104:44 | map of modern present day with some contours. It looks like it looks |
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104:52 | it's 500 m, something like that . But so these are the ODP |
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104:59 | 8 97 99 we're gonna talk about and here they are in cross section |
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105:06 | 97 8 99 8 98. And are called these are prototype ridges. |
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105:16 | how those forms basically when this basin over. When you know when the |
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105:24 | central atlantic north atlantic broke apart and these passive margins. The continental crust |
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105:32 | , you know, stretched and But it's um but because this area |
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105:38 | a, is a magma star, what they call it a magmatic margin |
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105:42 | non volcanic margin. There wasn't enough to produce the ocean floor. And |
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105:50 | in many cases you have like that's lower crust but prototype that meditates |
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105:58 | upper mantle rocks. So the idea is that you stretch it so much |
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106:05 | continent breaks apart until you finally just the upper mantle, it's just, |
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106:11 | know, it's just exposed and once exposed, it hydrates because the seawater |
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106:18 | to it and prototypes can be serpent . Ized. And when there's a |
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106:23 | , they swell and that's that's the for producing these things. Okay. |
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106:31 | the altar made these Ghabra, those thing is that they think they're altered |
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106:37 | being hydrated. Um Yeah. Water depths on the order of five |
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106:56 | . So the magnetic data, here's magnetic data or that. So, |
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107:03 | here's the lines. There's well 8 99 8 99 909 01. Which |
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107:11 | the same ones is in here. , so the mag survey this is |
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107:15 | this is called the this this indenture . This is the uh Iberia abyssal |
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107:25 | . And this is what they're They're just calling the tsunami the JN |
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107:32 | an M. Zero M zero. means Mesozoic zero is I believe Right |
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107:42 | here. And that would be 100 million years ago. Right? |
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107:53 | And then just these triangles to represent they're calling a pretty tight ridge based |
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108:02 | the samples from these from these wells they that they drove through. So |
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108:11 | profile, I'm gonna show you Okay. First of all. First |
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108:17 | is this bottom one, the straight here. It goes from this |
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108:21 | Anomaly, which is a big positive the way to 901. The second |
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108:29 | , I'll show you is just this one that just goes from just inboard |
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108:33 | the J. To uh 8 So here's, What do you measure |
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108:42 | the surface? You have a the fish you're driving. And this |
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108:47 | what you measure the amplitude is plus -200 gammas. 200 nano teslas. |
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108:53 | the deep toe anomaly is much Plus or -400 nano teslas. And |
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108:59 | can see but you can see that same thing, right? This |
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109:03 | Is that one? This one is one? This one is that one |
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109:06 | on and so forth. It's just you're closer to the source. So |
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109:11 | a bigger anomalies. Now they have little model and they calculate what contribution |
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109:19 | , you know, topography on the floor would produce. So that's what |
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109:24 | is. So you subtract this one the measure deep toe. And that's |
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109:31 | that's the dotted line down here. then they made a model here uh |
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109:37 | on, based on, you these the well penetration as well as |
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109:49 | , the anomalies. So their this their calling us M. three. |
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109:55 | mrs Mesozoic crowns go from M. to M. M. 40 to |
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110:12 | . m. 42. Which coincides ages 1 20 M. A 1 |
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110:21 | M. A. Now, a . When I say Cron, Cron |
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110:28 | the actual piece of ocean crust. what it is. Okay, |
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110:34 | quite often you'll see you might read the literature. People identify an anomaly |
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110:40 | say this is crown. Right? is Crown M3. They'll say |
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110:45 | And that's just a total art. just really the anomaly over the crime |
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110:52 | I'm not trying to be nitpicky but just want to explain. And so |
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110:57 | crimes, those are bits of ocean that are created by sea floor |
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111:06 | Okay, so that means if someone identified an M. That means they |
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111:12 | that sea floor spreading process is That's that's the what I'm getting to |
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111:18 | this. M three M zero would outboard of that Because M0 is a |
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111:26 | kick. That's remember I talked about long normal. So the law Norrell |
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111:32 | between Cron C% 34 which Which ended which the beginning of the long normal start |
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111:43 | 80 M. A. & 34 was the last um reversal map |
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111:52 | the center zone. Then you You know, 40 million years of |
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111:59 | polarization. No, no magnetic field , then you had M zero M |
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112:08 | is a negative because it's right next the long normal, which is all |
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112:13 | . So M zero is out here and it's going to be a |
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112:17 | That's why I was looking at this for a minimum that I can |
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112:23 | see I can track this. So thinking this is probably M zero. |
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112:28 | this is M. Three Then that this is probably M2M2 is a positive |
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112:36 | . So what they're calling the I would call em to now. |
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112:40 | only reason I know all of this so well is because I Actually written |
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112:44 | couple of papers on this stuff with Hall, you can get them from |
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112:47 | website if you want. 2018 and . Okay so that's what's going on |
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112:55 | . So here's just an example of toast data which is obviously much better |
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113:04 | surface and then you can use it kind of sort out what's going on |
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113:09 | the In the in the in the in the basin below or in this |
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113:14 | in the exposed uh process. So the shorter one and this is uh |
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113:21 | the need to surface analogy. It's flat um the deep toe lots more |
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113:27 | in it. Basic relief. And here's the results and then here's their |
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113:31 | model of that as well. Does that make sense with your, would |
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113:38 | explain that adequately do you think? I think so. Okay. Good |
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113:45 | good. No questions and I'll move . So here is the our summary |
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113:51 | the data acquisition with regard to There are two types of gravity |
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113:57 | The relative ones those zero length springs some sort of spring then this |
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114:05 | Which is the weight drop and you collect that the platforms for grabs your |
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114:11 | wells, marine water bottom. I I think I misspelled in your copy |
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114:17 | something. That's why it's highlighted here and satellite and the precision is reported |
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114:29 | be on the order of 1 to micro gals. Um although that's not |
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114:37 | serve a resolution if you ask me . The types of instruments are flux |
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114:43 | which are vector components. And then two the two resident instruments which are |
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114:48 | scale Urz. So they don't actually the vector direction which is a |
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114:56 | And those are of course the proton in the alkaline also called the optically |
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115:02 | one. And the platforms are land , marine deep toe. See I |
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115:07 | that there are magnetic susceptibility tools that susceptibility. I don't know if they |
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115:13 | magnetic. So this is a little a little unclear. Um deep toe |
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115:18 | and satellite and precision flux A 10th a now Tesla. This should be |
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115:29 | . I started um data acquisition acquisition like 73 ah session Resolution 0 |
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115:48 | I'll make that correct. Yeah because go on orders of magnitude .01 report |
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115:56 | and .001 for optically pump. And for survey planning it depends on the |
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116:01 | of the of the survey, depends the target area. The sort the |
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116:06 | kind of contrast you expect should make feasibility study. Um under consider the |
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116:15 | spacing what kind of instruments and you the platform and then of course the |
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116:22 | , jungles, deserts, there's a going on or something like that. |
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116:28 | we were I'm gonna drive on. data processing they're for gravity corrections. |
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116:37 | are two main categories of temporal corrections then there are spatial corrections. So |
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116:44 | temporal corrections are the title corrections and drift and special. We have to |
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116:49 | with the latitude of the survey Um make two corrections with regard to |
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116:58 | , the free air and then bouquet train corrections at both correction. We |
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117:06 | talk about that, but that's for platforms, ships and airplanes. And |
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117:12 | there's mist hikers, which is basically you're processing your for leveling the |
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117:23 | So this is a really busy but let's just go through it by |
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117:28 | numbers here. So here's our little of the earth and then here's our |
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117:34 | mountains and valleys and different data. don't I don't care about this stuff |
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117:41 | much down here, I don't think important. Okay, so the latitude |
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117:48 | actually is correct for three things. attracts a correct for attraction of the |
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117:57 | as a whole. So what accounts that? It accounts for centrifugal force |
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118:06 | to the rotation of the earth. it Uh common accounts for the radius |
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118:13 | the earth because Paul is 20 the diameter is 20 km less for |
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118:20 | radius rather is 20 km less at pole, that is at the |
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118:25 | So the earth is like an old spiraling. So that's that's the main |
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118:35 | . The terrain correction, correct for near the near the instrument that are |
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118:44 | the instrument and it corrects for avoids the instrument that are below the |
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118:50 | And so there are there are charts used that we used to do these |
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118:55 | in the old days. Nowadays, can do this with D E. |
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118:58 | . S very effectively. And then free air correction just corrects for how |
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119:04 | you are above sea level, just distance from the center of the earth |
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119:09 | account for any mass around it. the elevation and the bug a correction |
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119:16 | , it corrects for that mass difference there. So that's how that |
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119:22 | Now folks still like to do static . I don't think it's a |
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119:29 | I mean, I don't like to it. I think there's a lot |
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119:33 | assumptions and there's a question of whether , you know, quite often they |
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119:40 | ice, aesthetic questions where the earth not static, it's dynamic. It's |
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119:44 | over a subduction zone or something. mean, it just defies the reason |
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119:49 | do it. But I have a have a few slides in lecture number |
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119:56 | and I'll repeat this. I'll do slide is duplicated in there. So |
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120:01 | go back to this when I start I talk about this, I talk |
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120:05 | this in interpretation because it's really an . It's not a processing thing. |
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120:11 | don't think so. Here's the processing for gravitating. I'm sorry, take |
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120:19 | gravity measurement. And the first thing need is correct for tides and the |
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120:25 | draft and then you do the spatial . This would be for land, |
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120:30 | latitude, free air bouquet and That's the flow. Now for marine |
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120:39 | airborne, it's the same except you to add this, that was |
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120:47 | So the initial bouquet, it's called simple bouquet. And then when you |
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120:53 | the train collection, that's called the bouquet. Okay, so the title |
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121:14 | . So the gravitational attraction mentioned at service includes attraction from all other celestial |
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121:22 | . So with the exception of the because it's so big and the moon |
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121:27 | it's so close, everything else are not really, you know, we |
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121:33 | we don't sense mars or venus or or anything like that. So I |
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121:39 | just need to worry about the sun the moon. Um The title correction |
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121:44 | complicated because the gravity attraction, the and the moon vary over different time |
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121:49 | daily and monthly and the vertical component tide is so you have D. |
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121:55 | . Z for the tide, it's some function of the moon. |
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122:00 | m moon as our sons. It this complex function of co sign and |
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122:09 | distances and the mass of each of . So and r. Is the |
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122:21 | of the rigid earth. So where's at there? It is right right |
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122:34 | . And alpha is the geometric angle M. S. M. |
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122:39 | Okay. Alright, so that is formula. Well what the heck does |
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122:42 | mean? So I'm sorry wow, just got Mhm. So regarding the |
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122:55 | earth, the real earth acts So the odder layers are deformed. |
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123:04 | actually it's not just the water that up and down, the actual earth |
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123:08 | up and down The earth goes up the order of 10 cm. With |
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123:15 | with the variation in the with the and moon during the attraction the sun |
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123:19 | moon. Of course that's tiny compared the size of the earth. But |
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123:23 | does amount for about I guess what the maximum time 0.3 mg girls, |
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123:29 | a six hour period. So here's it works. Here's here's our earth |
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123:34 | around and there's this angle alpha. it's a survey area, let's say |
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123:40 | survey areas right there. So that is from the center of the earth |
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123:45 | the moon and the sun. So way to really get a handle on |
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123:50 | the tide correction is. We just at maximum attractions, maximum possible attractions |
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123:58 | sticking all these values in that formula get, the maximum tide from the |
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124:03 | is 0.5 mg. So 50 So it is it is arguably |
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124:12 | The moon is even more. It's twice as much. So the maximum |
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124:16 | , the moon is .11 mil So the maximum possible attraction From the |
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124:23 | is .16 million uh approximately. So micro gap. So, um, |
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124:33 | important. But uh, you I mean if I'm saying that the |
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124:39 | the, you know, the rule thumb resolution of gravity surveys is on |
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124:45 | order one mg. It's still kind in the noise, but it needs |
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124:50 | be done. I mean we're geophysicists crying out loud. We want to |
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124:55 | solve the queen. So um, , so drift correction. Now, |
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125:00 | meters are mechanical devices. So they from temperature and, you know, |
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125:09 | fatigue, et cetera, pressure. they that instrument and even though like |
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125:16 | are very careful when they build them people are very careful when they, |
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125:19 | they take care of them. The still drift. Just just this measurement |
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125:24 | change sitting on the bench in your . So, as I said |
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125:31 | we had to repeat with the tie at the reoccupy stations. And of |
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125:36 | we always assume that it's a linear because we are some kind of physicists |
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125:42 | physicists think everything can be reduced to sort of linear linear relationship is an |
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125:50 | and we don't really know what the . But from these tests. |
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125:56 | yeah. So tests have been to been done and They think that they |
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126:04 | they can make this argument all So here's here's examples of instrument |
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126:08 | So note the scale. These are is our .05 increment of Miller |
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126:17 | So these are not great. You , they don't change a lot. |
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126:24 | are over. Yes. Was seven in the morning at two o'clock in |
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126:28 | afternoon. So 8:00 - 3:00. So here's how it works basically. |
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126:37 | you have stations, you have a occupied for the first time and then |
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126:42 | go out and you measure B. . D. E. F. |
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126:45 | you re occupy A. So there's one to a. Two and here's |
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126:49 | your other measurements. So basically you much linear. You rotate everything back |
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126:53 | the A. One and a two the same level. And that's how |
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126:57 | , that's schematically how you do Very simple. Um tide and drift |
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127:06 | tide summary. Okay, so the often the base station reoccupied but is |
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127:12 | but it means it's gonna cost more you got to keep going back very |
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127:17 | . Uh Yeah, you can only drift rates can only be computed at |
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127:24 | . This is important. You can do the tide correction after you correct |
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127:30 | the instrument makes sense. Make sure values that you measure are corrected internally |
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127:38 | you start to make tied crates. for marine data navigation C state variations |
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127:45 | it impossible to reoccupy the site. it is calculated from repeat measurements made |
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127:51 | support of embarkation, which really is drag because like you could be weeks |
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127:57 | a month. You're gonna assume a , you know, a linear |
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128:01 | And that's probably just not true. so you have to just you |
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128:06 | but quite often in the marine survey get chances to to sail some ties |
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128:13 | your survey lines and you can do misty analysis which will help reduce that |
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128:19 | error. So yeah, cross line are important for the mistake correction. |
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128:31 | , latitude correction. Um The predicted of G. Not at any particular |
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128:40 | for a sphere spherical symmetric urge is by the latitude formula. So it's |
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128:48 | so it's a function of Insigne and it has to do with the difference |
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128:55 | at the grab G. At the and A. And B. Are |
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129:01 | . I guess there are constants that the shape of the ellipse oid. |
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129:07 | , so Here is the latest 1967 for this was published in blakely |
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129:15 | It's probably a new one out by , don't. So you approach so |
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129:25 | basically attract, you subtract this equation you plug in whatever your latitude is |
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129:32 | this in this uh this lambda. you solve that. So the |
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129:37 | G. R. F. The . G. F. I'm |
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129:41 | indicates that the north south upgrading of earth's field is given by this. |
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129:45 | this is .81-2 times a sign of latitude will tell you the gradient of |
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129:54 | the uh the field changes. Yeah it's very important. It's very key |
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130:02 | know what your latitude position is. . so what does that look |
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130:08 | So here's a little uh longitude latitude all the little survey stations in there |
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130:16 | um this is that data grid it so these are the contours and the |
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130:22 | and again it's going so this is yeah blue 185 so 135-185. And |
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130:29 | is good at five million gal Here's a latitude correction. So it's |
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130:34 | a function of latitude and it's increasing it looks like it increases from whatever |
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130:41 | be almost Well it looks like 0 Whatever 32 or 33. So you |
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130:51 | that from that and down here you this. So I mean the latitude |
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130:56 | does really swamp the signal. If gotta look at gravity data and you |
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131:02 | it's just got this enormous ramp going it. You can bet that it's |
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131:07 | been corrected for electric correction has not applied and if that's the case then |
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131:14 | can bet it's probably not been processed all because correction is the first thing |
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131:20 | do then you do elevation corrections and corrections and things. Okay so the |
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131:29 | formula gives G at mean sea level means but if you're at a different |
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131:38 | , free air and boogie to do is just for the elevation, the |
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131:43 | is for the mass between that elevation the mean sea level. Just kind |
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131:50 | begs the question and this is a that I asked my colleagues a long |
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131:55 | ago. And and the answers I are very interesting. Remember the |
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132:02 | it measures the height of the sea surface. It measures the G. |
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132:06 | . If you're out there on the sailing around, you're not at mean |
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132:11 | level, you're sitting on the OID, Which maybe five or 10 |
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132:16 | above sea level or below sea level even more maybe 50 m. So |
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132:24 | wouldn't you do a free air correction that? And I asked, I've |
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132:30 | my colleagues, it turns out that people like me who interpret data say |
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132:37 | , you should do it. But people who acquire these companies that acquire |
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132:42 | data and process it and say it doesn't matter. That's funny. |
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132:49 | anyways, yeah, so the gravitational decreases as elevation increases. This is |
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132:59 | rate at third. Almost a third a milligram per meter is just because |
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133:03 | getting further away from the source. just, you know, it's just |
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133:07 | just Newton's law right further away from source. So for extreme elevations, |
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133:15 | need to add a term to correct h um to so this this is |
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133:25 | this is the term you're adding for elevations. I'm not sure what that |
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133:31 | . I mean, I'm not sure the what would be extreme mount Everest |
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133:37 | the the Mariana trench or something like in any case. Uh yeah, |
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133:45 | point. Oh, so that is . It's about 1/4 of this signature |
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133:50 | . This this value here. So effect of the free of gravity and |
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133:55 | signals is related to two factors the of elevations in the area and severity |
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134:02 | horizontal elevation. So I guess if is a clip, if you're |
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134:08 | you know, in the in the the Utah surveying around all those enormous |
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134:19 | , then maybe we need to think this sort of thing. So if |
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134:26 | are smooth, of course little impact . So three aircraft. So here's |
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134:34 | little survey again and then here's the contoured at 10 m. So it's |
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134:40 | got enough, it's got a bit relief. It looks like it's |
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134:42 | you know, going from it's about 10 to 24. Just got about |
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134:49 | and 100 and 20 m of It looks like something like that. |
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134:55 | then there's the stations on top of . If we zoom into this corner |
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135:00 | here in the southeast but we have ranged from 23-102. No, that's |
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135:06 | same. It's the same color Right, okay. And these are |
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135:09 | stations down here. Um So the meant site. So we have |
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135:17 | Okay, yeah, applying that equation the value at 23:50 should be right |
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135:24 | . The free expression is 725.21 mil . Note that the fear anomaly Contains |
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135:36 | over print of topography. This is important. three here is dominated by |
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135:42 | . So quite often bouquet corrections are by contractors in the ocean basis. |
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135:55 | when you model data in marine you don't model Blue Gate should model |
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136:02 | air because the stations are at the surface. They're not alone. The |
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136:11 | . Whereas we're in in land the stations are, you know, |
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136:16 | draped on the topography. So you to account, you need to do |
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136:20 | boo gay because you have that I mean you do bouquets and marine |
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136:24 | but you don't need to model. don't need to make a model of |
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136:28 | . You can just use free air the stations are at the sea |
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136:35 | If that makes sense to you. that make sense to you don't do |
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136:37 | need to explain a little bit Um No. Okay. Alright. |
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136:50 | . I will explain it better. when we get to doing the exercise |
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136:55 | the way. Um I talked to guys last night and she quint and |
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137:03 | trying, I told him I really to make a decision. I want |
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137:07 | do like Wednesday because um I want , I want to do the exercise |
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137:15 | . So I want to be, want you to be able to grab |
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137:18 | software and install it on you, on your machine so that we can |
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137:25 | together on the model saturday for the . So that's the plan. And |
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137:35 | I mean it's it's just a nightmare I'm working on it. I am |
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137:41 | persevering. Okay, no problem. , so for land based gravity measurements |
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137:49 | sea level, the decrease in the gravity field above sea level accompanied by |
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137:54 | traction. The material between right, is for the bug a correction and |
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137:58 | amount subtracted is due to an infinite slab. Right? This is the |
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138:03 | PG road to PG Ro H It's gamma here but it's G. |
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138:10 | the the international gravity gravitational constant or 04193 rho times H where H. |
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138:20 | a meter. So that's the big crash. But the way to think |
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138:24 | bouquet crash is not as a slab , way to think about it is |
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138:30 | you're minimizing the effect of topography. , free air data is dominated by |
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138:39 | and so what the bouquet correction does it accommodates for that surface contrast such |
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138:46 | it tries to you know, you it to be, you wanted to |
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138:51 | make it invisible so that you are at anomalies produced by the subsurface. |
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138:59 | , so there are lots of ways decide on what road to use. |
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139:04 | you know, well as core samples the last thing as we talked about |
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139:14 | it must be a representative of the that exists between the highest and |
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139:18 | So you gotta. So now some like to try to do what they |
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139:22 | a variable density bouquet, I think just nutty because you you have more |
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139:29 | a chance of producing anomalies that don't exist than you do of actually |
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139:36 | you know the effect of topography. and as usual the bouquet approximation, |
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139:43 | have low relief, just like for relief. You know these corrections don't |
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139:48 | much of an impact on the In fact for like offshore free air |
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139:54 | over like continental shelves is de facto because the shelves are pretty flat. |
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140:02 | when you do a bouquet correction over a continental shelf doesn't change the data |
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140:07 | much because the things flat. So a picture showing you what all that |
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140:13 | . So here's a here's our Here's our observed gravity. Alright? |
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140:19 | subtracted um the latitude correction, We the free air correction and now we're |
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140:27 | the bouquet all corrections and gravity subtract the measured signal. So that's just |
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140:34 | truism. Subtract. Subtract. Subtract . Remember. So here we have |
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140:43 | here's here's the sea level, say that B. And we're making a |
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140:48 | here at p at some elevation. . Right? So we got this |
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140:53 | between A and b. Well we to account for the material to complete |
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141:01 | the material that's missing here and the that's added here. And if so |
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141:13 | you have a station, if you a station here, you can see |
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141:15 | this material would add to the blue correction. I would add to the |
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141:20 | data because you have this attraction over . But what about the valley? |
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141:31 | How does that work? You need you still need to subtract it because |
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141:36 | subtracting what's already been subtracted, So you're subtracting what's already been |
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141:43 | So it's adding that right? You to you need to add in the |
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141:50 | area, you need to add this fill in it. But it still |
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141:57 | a subtraction. Yeah, I gotta about that. Huh? But the |
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142:03 | remember civil boogie is just a That complete includes the train tracks. |
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142:09 | all Deficiencies from one and 2 and from three and 4. I wasn't |
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142:16 | on purpose to be confusing but I that the book is always subtracted but |
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142:21 | is a negative so it would be less of a value anyways, Don't |
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142:30 | about it. I'm not going to you on it. So, so |
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142:34 | here. This this is a figure Nettleton 1976. It's an old figure |
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142:40 | Middleton. There's a very famous book petroleum prospecting with magnetic data and |
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142:51 | L. Nettle to louis L. was a very famous uh practitioner of |
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142:58 | magnetic p. I think he was gulf oil guy. And this and |
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143:03 | is called the Nettleton method for determining books you should use whenever you look |
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143:10 | legacy data, gravity data. This economics you can bet They're gonna use |
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143:17 | for the bouquet correction density. The formula right here the big agency right |
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143:24 | they're gonna use 2.67. It is is a universal value and actually there's |
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143:30 | no good reason for it. David I mentioned earlier I used to work |
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143:35 | Arco. He gave a talk once he really dug into this thing. |
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143:41 | was the origin of using 2.67 2.67 as I said is the density |
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143:47 | courts. But it turns out that um why it's used for bouquet is |
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143:55 | just no good reason. It's just people do. And in fact you |
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143:59 | assume that's what it is and in it's what I do. It's what |
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144:03 | do because that's what everybody else in world has always done. It's really |
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144:06 | of ridiculous. But now what? so what you can do so if |
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144:12 | get legacy data you take that and you have an area where you you |
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144:17 | think, you know you look at bouquet anomaly man and it either correlates |
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144:22 | anti correlates very well with topography. in this case the top curve here |
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144:29 | correlates and the bottom one anti correlates ? If you see that, what |
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144:36 | can do is you can strip out can you can take the topography take |
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144:42 | bouquet corrections. Formula with 1.67 and out that correction and then you can |
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144:48 | an analysis like this. You can it in three D. As |
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144:51 | You just test a bunch of bug corrections For different values until you minimize |
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144:59 | effect of topography. Remember that that's the reason we do it in |
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145:02 | first place and once you minimize it that's your boo gay density correction in |
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145:08 | case. 2.2. So this is that all of us do. We |
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145:14 | know. It's gonna be 1 We all know that to check the |
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145:21 | versus the data with gravity data. want to always check topography versus free |
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145:28 | versus books versus your residuals. You want to be checking in because because |
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145:36 | biggest density contrast that's that's measured by is the topographic surface and that is |
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145:44 | even if it's underwater, that's the density contract. The second biggest density |
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145:52 | that affects the data is the contrast the bases across the mojo. You're |
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145:58 | from 2.9 - 3.0 So that's a grams per cubic centimeter contrast. So |
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146:10 | biggest Destiny contrast. This is That's what I'm saying it over and |
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146:13 | . The biggest Destiny contrast is at surface or the water bottom. But |
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146:21 | rocks and soil meet water or air the second biggest is at the base |
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146:28 | the crust at the mojo but this the way that you can do |
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146:33 | you can apply to sort of minimize you don't want you don't need to |
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146:37 | trying to interpret anomalies that pretty much can just go out there and walk |
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146:41 | . There's no reason to try to it right. You want to get |
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146:45 | of that. You don't like look stuff that's beneath it. Okay enough |
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146:49 | me uh preaching there. So train . So the topography surrounding each site |
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146:58 | you know, doesn't conform to the . So we need to do a |
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147:01 | train corrections. And for for land . I mean even marine now everyone |
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147:08 | D. E. M. But back in the day there was |
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147:12 | was called the hammer method. And broke up circles around your station in |
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147:18 | of zones and compartments. And the was just just tedious and time consuming |
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147:26 | really just, you know, what that look like? So here are |
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147:31 | the different zones you have zones A L. And then so and then |
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147:37 | zone is broken in the compartment or . So this in this case, |
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147:43 | J. Has 16 different compartments or and zone zone B in here as |
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147:50 | radius of six 0.56 ft to 54 . Zone J 8500 and 78 to |
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148:01 | Zone M 48,000. Right? So is this is, you know, |
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148:07 | just under two miles, just under miles. So it's big. So |
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148:13 | you get out here the contribution is . You can start using contour |
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148:20 | And then so here's here's the idea that it's uh you have to pocket |
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148:27 | topography in. Each compartment is then with a flat top prison. And |
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148:35 | the mean elevation of each present is . And then you have all these |
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148:39 | and compartments. So you can you're to get a sense for what kind |
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148:43 | a nightmare this stuff is. But important because you need to really reduce |
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148:49 | the you know the external mass excesses deficiencies that affect the measurement. So |
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148:58 | again, nobody does this anymore, all done with D. M. |
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149:01 | . Now. Um But here for reference are the original hammer charts. |
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149:07 | for zones B C E F. . And it shows with with regard |
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149:14 | uh radius and I guess radius and . Right? That it uh table |
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149:25 | going to use the compartment or injured use. Okay. See for each |
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149:31 | do two undulations. Right. This okay. This correction applied to. |
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149:37 | . Yeah. Customize oh, closer eyes. This is right. This |
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149:43 | the height. Yeah. In any these are the table. These are |
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149:47 | historical value going all the way out em. So F. Y. |
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149:51 | if you ever someone ever asks you hammer, you know it um As |
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149:59 | said D. M. Another approaches mathematical functions. You can try, |
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150:04 | can try to approximate the topographic with sort of you know, Aunt or |
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150:11 | . Now, marine, what we do is we just we fill the |
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150:15 | layer with the density. So wie wir dancing is one point oh three |
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150:22 | 1.0 to 6. Just a little more dense than one. And you |
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150:30 | to. And the water bottom densities range from like 1.9 to 2.2 on |
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150:40 | order. So far less than land course. Um So what you would |
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150:45 | is you would just what I I build a three D. Model |
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150:49 | just a water layer. I like . The attraction of that layer at |
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150:55 | density of point uh 97. So assuming the water bottom density of |
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151:04 | The shallow density density is too. then so when I calculated the attraction |
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151:10 | .97 I add that to the free gravity. And I've got it. |
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151:16 | I've created a bouquet a correction of of two rather. So that would |
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151:26 | dense if I make the water layer too. And the sediment density directly |
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151:31 | it is to you see basically I that horizon. I've erased that density |
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151:38 | . So there are no anomalies. mean theoretically are being produced by that |
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151:42 | contrast. That's the idea, it's same sort of idea as I was |
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151:48 | showing you back here as sort of thing is adding density to sort of |
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151:56 | the effect of topography. That's the of bouquet. I know it's a |
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152:02 | correction, yada, yada yada. the point of it, the point |
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152:06 | the reason we do it is to topography. I hope you'll never forget |
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152:13 | now. Mm Okay, so that correction those votes harvey you want to |
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152:23 | it that is a correction that that corrects for a moving platform. |
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152:31 | so the Earth is rotating but if have a moving platform, like a |
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152:37 | a boat or an aircraft or an or helicopter, then there's gonna be |
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152:44 | scent refusal, you know, accelerations related to that. So here we're |
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152:52 | down on the Earth is rotating this um and from the north, looking |
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152:59 | from the north pole. And so have the acquisition plan. The elbows |
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153:05 | subtracts from the angular velocity. I , well the measurement, if you're |
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153:11 | on where you're flying, if you're this way, it's gonna subtract from |
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153:15 | angular velocities. Earth rotation. If flying this way or some component in |
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153:20 | direction, it's going to be act it's going to be added to the |
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153:25 | velocity of the Earth's rotation. So got to correct for that. And |
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153:33 | here's our little survey and surface up . You have this this angle lambda |
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153:40 | the center of the earth, through survey area. And you have another |
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153:46 | measurement that extends from the axis perpendicular our area. Right? So uh |
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153:54 | latter the line of longitude with with is this? This is a |
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154:01 | Let me just see if I can this out. Uh alpha alpha is |
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154:07 | heading. Okay, that's the right? That's the direction we're |
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154:10 | Okay, so you have these So this is the at most formula |
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154:16 | oh three times the velocity that you're in. That times the cosine sine |
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154:23 | of latitude sign of the heading plus velocity squared. That's the formula. |
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154:34 | I'm gonna test you on that. , I'm not kidding. But yeah |
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154:38 | how you correct for the the relative of the aircraft or or the |
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154:51 | Okay, september um let me I don't I think I'm almost |
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154:57 | We got yeah, I mean 11 . Okay, so with magnetic corrections |
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155:04 | really there's really just one. I let's just think about but first this |
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155:12 | how the magnetic field varies. It lots of variation in the field because |
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155:17 | know, it's a there's a daily and there's secular time variations and then |
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155:24 | the big correction is has to do the core field. The field that's |
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155:30 | in the earth in the Earth. and outer cores. And that correction |
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155:38 | called the I. G. F. The international geomagnetic reference |
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155:44 | Um And that is thought to be by a geodynamic dynamo. So we |
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155:51 | our measured data total intensity field and do a Daryl correction. I think |
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155:58 | is optional line leveling. If you a good job of your survey line |
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156:04 | this should go away anyways. And gotten into many animated discussions with magnetic |
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156:14 | processes about this process is you anyway, so you they would correct |
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156:22 | barrel and then correct for the main the the core field using the |
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156:27 | G. R. F. And you're just left with total intensity magnetic |
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156:31 | data D. T. Here. , so um external temporal crests. |
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156:41 | the external contributions in Earth field are small, less than 100 now tests |
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156:47 | some magnetic storms can be over 500 , especially at the polar areas. |
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156:54 | external contributions ignore originally from the Solar winds interact with the Earth's field |
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157:02 | . Can be they actually, there's there's a sunspot cycle 11 years. |
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157:07 | might have heard of this. Um they can also have very short micro |
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157:12 | stations which can dominate which kind you know, cause problems. But |
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157:19 | Mag surveys, the most important variation the daily or the diurnal variation. |
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157:26 | they can range from 5 to 50 they can even be bigger over the |
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157:32 | area over the course of the And they are caused primarily by ionic |
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157:39 | but they can also be from two currents in the earth beneath the surface |
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157:46 | . And the correction is called the because the dominant variability is linked to |
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157:52 | cycles. Even to lurks are are to daily cycles. Okay so here's |
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158:02 | comparison uh the horizontal variation mentioned Four observatories. So there are different |
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158:09 | there are different magnetic observatories around the . I don't know how many, |
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158:13 | are maybe 50 maybe 100. But are just, they measure the Earth's |
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158:19 | permanently. So quite often you'll you'll some survey David and maybe your base |
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158:26 | goes down because you have to have base station while you serve it. |
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158:30 | have to plane up capturing data and back wherever your hotel is. You |
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158:34 | a base station. They're just sits one spot and collects maG data. |
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158:39 | that's how they figure out what the variation is. Because you don't really |
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158:44 | what the declaration that you're flying along data on the dynamic platform. So |
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158:48 | can So they read out the dire base station data and that tells them |
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158:53 | if there are any storms or micro . Alright so getting back to |
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158:58 | So here is four different observatories, in Hawaii, one in Arizona, |
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159:04 | in the UK and one in And at different geomagnetic latitudes. So |
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159:13 | is 21 degrees 40 degrees 50 degrees 60 degrees all in the northern |
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159:22 | So 20° is pretty low. And and of course this range is 20 |
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159:26 | tests. See they're using the term that means nanna test. I knew |
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159:32 | was gonna happen. Um Yeah. I have notes on this slide |
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159:46 | Okay. Yeah. In any case can see that and as you go |
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159:51 | in latitude that the effect is bigger bigger and bigger over 24 hour |
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160:02 | Yeah 0 24 hours. So you see midday it goes up a lot |
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160:06 | then down a lot. Uh This at a very this is at a |
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160:11 | of 20° and then it's interesting in . It goes it goes down a |
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160:18 | lot. All right because the sun hitting these low latitudes more directly. |
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160:27 | is really interesting. It does go but it goes down first six. |
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160:31 | that's quite interesting. All right. they've actually done studies and this is |
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160:38 | study I'd like to show my friends don't like that want to process |
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160:43 | So in Australia, in this area down here in western eastern Australia. |
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160:51 | took um I got five measurements, stations and they I guess they put |
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161:00 | in the ground, They dug holes put these things on the ground and |
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161:03 | measured events from october 26 November So they measured almost a full |
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161:13 | Um All at about the same latitude or take and the same latitude give |
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161:19 | take. So this is called the area in new south Wales in |
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161:31 | I'm sorry. Uh, so, , So here's their correlations. I |
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|
161:44 | they correlate reasonably well. So this 10 nano tesla and um, this |
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|
161:52 | at one end. This is the in october variation november 23rd over looks |
|
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162:02 | 15 minutes. They're just comparing some minutes from all five of these. |
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162:09 | one is flat, this machine must broken but there is some similarity but |
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162:14 | not exactly the same. 10. you have a very eight seat. |
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162:20 | is a high, this is a . So they're not correlating exactly the |
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162:26 | . So, but the argument that make is that what's happening at the |
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162:31 | station is not necessarily happening where the is flying. That's the point I'm |
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162:37 | . And you can see they are . I mean they are significantly different |
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162:41 | some cases. I mean this to , this, you know, and |
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162:46 | , these guys are all pretty close . I mean they're all right |
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162:50 | What 25 km. I mean sometimes base, sometimes the nearest airport is |
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162:57 | km away from the survey area, 600 km away. So you know |
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163:05 | is this is pretty small. So always been my argument is that what's |
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163:10 | at the base station is not necessarily at the airplane anyways. So there's |
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163:19 | making a big deal about nothing. . But then all when you, |
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163:23 | you level the data properly those variations come out will be leveled out. |
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163:29 | saw the difference on the order of a few nano Tesla. Anyway so |
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163:36 | pulsations are another temporal uh fluctuation, small amplitude on the order of Frequency |
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163:46 | at .0123 Hz and able to is than 10. Now again these things |
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163:52 | be depending on the while they're short spans so they can contaminate the data |
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163:59 | they can have amplitudes up to tens . So this this is a good |
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164:07 | to have a base station though because may pick up these you may pick |
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164:13 | these features um at the base station still you may not but you have |
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164:19 | you still have to compare. So not arguing against the base station. |
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164:23 | still have to compare that data. you survey data, magnetic storms are |
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164:28 | different animal. Those are just bad . They can exceed 1000. They |
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164:33 | be thousands of nano Tesla and they be very localized and they're really common |
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164:40 | the northern latitudes. When I was World Geoscience that was the in between |
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164:46 | company between between between arrow service and debt that I worked at. We |
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164:53 | the north slope and we flew the thing and and of course it was |
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165:00 | was just all kinds of noise but just what we did was our strategy |
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165:05 | just put two planes up there and flew nonstop all day and all night |
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165:10 | we flew in the summer time. so there's 24 hour daylight and we |
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165:15 | and then, we basically. you , we had two processors up their |
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165:22 | the data on a daily basis and re flights nonstop. So every flight |
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165:29 | go up do some re flights then survey lines and basically and then like |
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165:35 | it to the processes to fix and did it, we did it I |
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165:38 | and ended up being ended up making . Um But that strategy because otherwise |
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165:47 | you sit around you otherwise just gonna sitting around waiting for the storm to |
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165:51 | . And then by the time you out and mold and fly and then |
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165:53 | back. So just we just decided to fly straight through so that they |
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165:58 | be pretty bad, especially at high . So here's the the the temporal |
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166:10 | processing slow. Okay so you measure data, you check the base station |
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166:18 | the diagonal. Is there any bad ? Yes. Re fly. You |
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166:23 | you say this line between this tie this tie re fly. If not |
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166:29 | you then you can if you want can apply this daily correction. But |
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166:34 | like I demonstrated with that Australia it's really not not an issue shouldn't |
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166:42 | might actually produce an at least by this thing. But in all honestly |
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166:47 | a very very it's it's over each . It's a tiny variation because we |
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166:52 | back that study results, This is minutes. So in 10 minutes I |
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167:00 | you're flying you're flying 130 knots. you know, that's that's not that |
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167:06 | of variation. It's kind of a wavelength correction in the, in the |
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167:11 | . Okay. Now the basically the required correction is the core field and |
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167:19 | removing the I G R F. the I G R F is, |
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167:23 | know, it's determined with the sort like DeAndre harmonic harmonic uh polynomial solution |
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167:33 | it's um, so it varies with to position and yeah, so the |
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167:43 | of the components of the field that geometric observatory. So we use these |
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167:47 | again and just a taylor series in and co sign. And the internationally |
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167:57 | values of the coefficients are used to a model field or the Earth coastal |
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168:04 | . Historical sets of coefficients are labeled . So every time the I G |
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168:08 | F is is updated the retired version year. The retired version. |
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168:17 | it's not thrown away. It's just D G R F with the year |
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168:22 | it was retired. So we have whole history. So, so that |
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168:27 | if you come across some legacy some old data That was acquired |
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168:34 | you know, 1975 or something. , that was using a different I |
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168:38 | R F than we're using now. there is a D. G. |
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168:42 | . F. That 1975 will fall and you can use that one. |
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168:48 | that's and that data was probably reduced most certainly reduced using that that that |
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168:57 | . Okay, so I showed these you yesterday the total field strength, |
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169:03 | inclination and the declination. I just them here because um well I just |
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169:09 | them here now. What this is is sort of getting a little |
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169:15 | But this is because this is stuff people worry about. I don't |
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169:19 | you know, I don't really worry this stuff very much. But people |
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169:23 | and this has to do with actually question yesterday about reversing fields. So |
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169:28 | people think that the earth field is by a geodynamic dynamo dynamo effect. |
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169:37 | ? So so a mono polar dynamo would be something like this. We |
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169:45 | the magnetic field going through and you a curve going through it. You |
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169:48 | some angular rotation. And so an current in here and that would produce |
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169:57 | magnetic field. Right? Like a oid from your days of studying |
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170:04 | Well, what people think what a of people think, He says you |
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170:07 | some kind of double dynamo in other , um uh it's that that would |
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170:14 | for polarity reversals and non uniform field . Right? So you have these |
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170:20 | tubular cyclones and whereas where they could alternating polarities right with the flow of |
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170:29 | altar. So you have some kind colored in the in the course some |
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170:34 | of popular flows like that. And and so this is a this is |
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170:42 | picture by Schmidt where he simulates. your here's your reversal simulation uh A |
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170:51 | year transition. So in this case have whatever the north pole is in |
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170:57 | , the south poles and blue at point things are getting kind of mixed |
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171:02 | but in the end they realign and now the blue is up here in |
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171:06 | north and the gold is here in south and these would be the flux |
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171:10 | that they're that they're modeling. It's very cool very cool sort of pictures |
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171:16 | stuff. Um So does that answer question about the field reversal? |
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171:25 | I just I just think it's an topic. There's so much like I |
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171:30 | wanna say back and forth on it is so many different things to read |
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171:33 | it. I like it. So would suggest reading this paper if you |
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171:38 | . I have it if you I can send it to you, |
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171:43 | that team. I'll make another. I will send any paper to you |
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171:52 | you want that you said that I you. I have them all. |
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171:58 | , okay moving on. Um This the mag sat scale or not only |
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172:05 | . This is a very old This goes this is 1982 but it's |
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172:10 | out for the kind of like But you can see that the inclination |
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172:14 | 45 And then plus or -45 and do the magnetic equator. And these |
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172:22 | those same anomalies that I kept showing the big view. But these look |
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172:27 | much better. There's just there's a bit more of a, you |
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172:31 | a little bit more variability in wavelength stuff. So I like this one |
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172:35 | lot better. But if you do power spectrum of this field, what |
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172:42 | get is you get and if you know, if you plot the |
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172:46 | of that power versus harmonic degree um you get an interesting plot, you |
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172:55 | this very long wavelength linear feature here then it flattens out. So this |
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173:02 | slope of the short of the, the higher degrees. That's all these |
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173:07 | . But there is there is a wavelength, the point that you just |
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173:11 | see in this and that's the core . So people think of the car |
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173:15 | . So we'll look at power spectrums and we talk about anomaly source |
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173:22 | But this is kind of a preview that because we can use the same |
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173:29 | in local areas and kind of dissected spectrum into different death regions of the |
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173:38 | that are being produced in the So that's a tool for interpretation that |
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173:44 | get to. But this is kind a preview of it. So data |
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173:50 | variations, variations in the intensity Earth at the precise is this my summary |
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173:57 | ? No, it's not. precise processes that give that give rise |
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174:04 | second operations are not well understood, we know that. Oh right. |
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174:09 | is second rate. So this is this is like 100 years or 20 |
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174:14 | . I mean the Earth, the of the Earth actually dressed as the |
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174:22 | like uh to the west, to east. Um we'll find out, |
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174:27 | I know that just so we understand secular variation. So here's an |
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174:31 | this is from garland. This is textbook 1979 secular change Earth from. |
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174:38 | this is 1922.5 versus 1942. So a 20 year difference. And so |
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174:46 | see uh let's look at this. in 22 you have this high, |
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174:50 | it's drifting to the west. So have this high right here in the |
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174:56 | atlantic. So there's africa and south . It's just not the coast again |
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175:01 | 20 years later it's migrated across the and it's just sitting out here north |
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175:08 | brazil. Okay, let me see I can find another one. |
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175:12 | so this one here over the over right, is now drifted and over |
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175:20 | over um just north of Africa. You can find another one. |
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175:27 | and this one here, that's right . That one is drifted as |
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175:33 | So the field is drifting to the . Um And that's called the secular |
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175:42 | . Which is which is this is reason why you need to retain the |
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175:46 | . G. R. S. old because because the field is you |
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175:50 | they re they re update the G. F. Of course your |
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175:53 | methods get better plus the field is . So you have to continually |
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175:59 | Right? So the you know the formula this lasagna for polynomial, it's |
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176:06 | is rooted. Let me go You can find that formula. That |
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176:12 | . Where is it at? But my formula that's trained magnetic. Didn't |
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176:29 | have it? I'm sorry. One time. Please bear with me I |
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176:34 | to find this. I thought for I had to endure for you. |
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176:44 | I haven't. I'm gonna make a . I. G. R. |
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176:49 | . Formula. That's that kills It's very similar though. It's very |
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176:56 | to um Two the last word correction you can imagine. Alright. Um |
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177:07 | here's uh here's the summary of the field change. There's external and internal |
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177:14 | that affected. So um uh Beginning the very smallest there's pulsations down |
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177:26 | There's things called-based journals here. Um are external recurrence of storms. Semiannual |
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177:35 | . I see that's the 11 year . And then here you have the |
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177:40 | change which we just talked about and over here is reversals on the order |
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177:44 | thousands of years. So um so this includes secular magnetic experiences of |
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177:53 | reversals. And over here it's micro storms and seasonal changes. So there's |
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177:59 | lot of things that affect the magnetic , but you really only do one |
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178:04 | . Now the magnetic poles move they sort of wobble, you |
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178:13 | and uh reliable Palin genetic data are . Now Poll Rwanda is this idea |
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178:24 | so what you do is if you a stereo net and you plot positions |
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178:30 | south american africa, the rotation that make can be described. The rotation |
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178:38 | any plate on the Earth can be in terms of a rotation pole, |
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178:45 | ? That that you know to the the to the diameter of the earth |
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178:51 | some angle. So you can describe rotation atmosphere with a pole location and |
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178:56 | on the angle. So these dots where that hole intersects the surface down |
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179:05 | . So there'll be another one on other side, right? And then |
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179:10 | the plates move around. So these the relative pulls between the rotation angle |
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179:17 | north America. South America over time described by these poll locations and some |
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179:24 | and then over time you can reference to each other. In this case |
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179:30 | a parent polar. So it's africa south America reference to each other. |
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179:36 | , now there's true polar wander where reference them two. The hot |
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179:43 | fixed reference frame. So I don't if people the idea of fixed hot |
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179:50 | is is really being challenged a lot days. But so you would do |
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179:57 | relative and apparent polar wander reconstruction between and south America and you do these |
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180:06 | on the sea floor spreading anomalies as as um paleo magnetic data which which |
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180:15 | which is detects remnant magnetization as I . And um this is just to |
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180:23 | random and paleo Magnetics but and then can plot that um that polar motion |
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180:32 | to each other. But then you take that and rotate that whole system |
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180:36 | poles through the through polar under path the in the spot reference rate. |
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180:43 | then what you can do is you do that with all the clothes, |
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180:46 | the ocean basins and do that with all. Why am I telling you |
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180:50 | ? So yeah, this is the bit I just want to talk about |
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180:55 | we're talking about polls and the polls around and then of course not only |
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181:00 | they move around but you also um plates move around and so these are |
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181:08 | the sort of tools that people use try to keep keep track of that |
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181:14 | sort of summarize with dated corrections, is temporal tied instrument trip, special |
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181:23 | elevation free air train at boss for platforms and missed. I leveling or |
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181:31 | loops and temple from magnetic journal if want secular which is which is actually |
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181:38 | the Nigeria and then special the main and in this tie level. Um |
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181:46 | it. Any questions was that? So this is really the summary of |
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181:53 | magnetic field changes and the only correction the I. G. R. |
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181:57 | . And then this last bit on wonder. Um I just wanted to |
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182:03 | this idea to. You might have of it already but I think it's |
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182:06 | because it is a magnetic field issue paleo Magnetics has to do with remnants |
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182:12 | we talked about and uh it is that that has done particularly with reconstructions |
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182:23 | and things like that. So any any questions for any of this |
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182:29 | Not right now. I kind of to just like look through it and |
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182:35 | cool. You can always ask me week or whatever. Oh well that |
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182:46 | a lot. What do you What do you got you guys want |
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182:49 | take a lunch break down and reconvene do the next lecture. Yeah that'll |
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182:57 | . What what what what do you I'm up for anything if you want |
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183:02 | start early to finish early? That's with me. I don't care. |
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183:07 | you want to do like 30 minutes minutes 1215. Um Okay if you |
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183:19 | . What about you? Is that with you man. Are you gonna |
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183:22 | at lunch? Uh both of work me to start a year old. |
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183:31 | you are you're taking lunch, Yeah. But I can take lunch |
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183:39 | when you have the uh So you I'm talking I guess. Right? |
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183:46 | . Yeah. Yeah. Fair Okay. I just wanted I didn't |
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183:51 | didn't know if you wanted to read book over your while you were eating |
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183:54 | something, so okay then. So it is you calling the shots? |
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184:01 | see you in half an hour. |
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