© Distribution of this video is restricted by its owner
00:13 | Yes, got it. Are we now? Okay, great. So |
|
|
00:25 | already chatting about what you're doing, you're from and everything. Um Now |
|
|
00:33 | the notes here. Did you did download the notes? I have to |
|
|
00:43 | Yeah. Yeah. Yeah, no getting into my GPS. Alright, |
|
|
00:50 | , so um seven lectures to exams exercise and I already explained to you |
|
|
00:57 | we may. I got a plan for this. It will be another |
|
|
01:02 | . Um Probably test but more It's about porn. It's about I'm |
|
|
01:19 | . Hello? Yes, I'm I'm right now. I'm I need to |
|
|
01:28 | you first thing monday morning, have insurance and I'll send that information first |
|
|
01:32 | monday morning. I know you don't it well then I'm gonna have to |
|
|
01:41 | because I mean, I'm not gonna home till like six o'clock. |
|
|
01:46 | So. Alright, so Right, seven or eight lectures, I'm hoping |
|
|
01:50 | get this thing worked out. I'm hard on it. I got a |
|
|
01:53 | of different two pronged attack. That's the problem because that's that's a good |
|
|
01:57 | to do. Um kind of like basic theory, data interpretation, |
|
|
02:05 | uh processing, you know, interpretation and then then 5 67. I |
|
|
02:13 | uh the good part because I'm teaching to interpret gravity and that's what my |
|
|
02:19 | is. I'm writing a book about and basically the idea is we're gonna |
|
|
02:25 | through different kinds of base where we're learn all kinds of bases, There |
|
|
02:29 | classifications and then we're gonna go to different kind of basic platform basis rift |
|
|
02:35 | , You know, four land bases our basis, passive margin basis and |
|
|
02:41 | bases that are kind of complicated and gonna lots of examples that show you |
|
|
02:47 | kind of anomalies are produced in those , whether from mythologies, structures, |
|
|
02:52 | like that. So that's the The thesis of um the grading is |
|
|
03:00 | for each exam And then 20% for exercise. So if we do switch |
|
|
03:05 | , I'll probably give you a paper read. And then you can summarize |
|
|
03:09 | of like connect what you learned here what's in the paper like Oh, |
|
|
03:13 | see that they that way. So can I can I can learn what |
|
|
03:19 | learn. All right, So, so here's the beginning and I had |
|
|
03:25 | get my notes out for this But yeah, so gravity magnetic methods |
|
|
03:33 | how come can I get rid of thing? Man? That's, that |
|
|
03:43 | bites, you know, put it there for right now. Okay. |
|
|
03:50 | so the history of pragmatic method. they go all the way back to |
|
|
03:55 | of load stones by uh the Greek fails, fails of militants. And |
|
|
04:04 | the Chinese also discovered both stone and fact jumping like 1200 years or so |
|
|
04:11 | years, 1200 years. They actually the root of military compass. Always |
|
|
04:19 | back to you know then And then the matter? You can't get rid |
|
|
04:25 | that thing. Okay, thank Alright. Um Right, so then |
|
|
04:37 | , the italian scientist Galileo. Uh dropped, he got the famous experiment |
|
|
04:42 | he dropped two different size mass, two masses off our pizza to demonstrate |
|
|
04:50 | they hit the ground at the same . Okay. Um and of course |
|
|
04:55 | Gilbert, do you know about? don't know. Okay, so he |
|
|
05:00 | was, he wrote a famous book called day magnet day magnetic magnet. |
|
|
05:07 | magnet and of course he famously proclaimed world as a magnet. So he |
|
|
05:13 | the north polar magnetic field back in . Start doing Oh I think so |
|
|
05:31 | Okay, so um the first folks use potential fields to prospect were the |
|
|
05:39 | and they in 1630 they used magnets data magnetism to prospect for iron ore |
|
|
05:46 | then uh jean, is that how say that 16 72? He's a |
|
|
05:52 | astronomer on and see, he mentioned , He mentioned that depends only at |
|
|
06:02 | at the near the equator of french well as in paris. And so |
|
|
06:07 | he worked out that the earth shape a little bit different because of |
|
|
06:10 | Okay. And of course the place very famous for laplace equation which we |
|
|
06:17 | know from geophysics and then um but developing the spherical harmonic polynomial. And |
|
|
06:31 | then uh with regard to isil the idea that the crust of the |
|
|
06:35 | was floating in the man kind of an ice cube floating in a glass |
|
|
06:39 | water. There were two ideas that being argued between john pratt and George |
|
|
06:47 | Carey. And um and that was course they were called the hypotheses. |
|
|
07:00 | Pratt argued that the cross is uniformly and just had a different density variation |
|
|
07:05 | area said no across various thickness and of hit the thicker crust roots into |
|
|
07:13 | mantle and they're both kind of right . Um Then James Clerk Maxwell, |
|
|
07:21 | Maxwell equations, you probably know that class, uh you know the four |
|
|
07:26 | that connect electro Magnetics describe electromagnetic And then the first actual airborne magnetic |
|
|
07:33 | measurements were made from a balloon by Thompson elder in 1910. So we're |
|
|
07:39 | up to the 20th century, I know how I'm bending, mens mens |
|
|
07:49 | mens mens mens should not say So he's a duck's geophysicist and geologist |
|
|
07:58 | he's attributed with developing instrumentation to measure , particularly at sea. And then |
|
|
08:08 | guy Google from 1932. This is very interesting one. So he was |
|
|
08:14 | Hungarian and he he was, he the first gas reservoirs in Transylvania |
|
|
08:24 | So it was the first use gravity explore for hydrocarbons and victor. He |
|
|
08:30 | a very famous person, he has long history of long resident worked at |
|
|
08:36 | . He's, he's born in Russia Ginsburg, but he worked at golf |
|
|
08:41 | during the World War two where he the that they used to find Germans |
|
|
08:46 | range. So he's uh yeah um then you know Sgs actually conducted the |
|
|
08:56 | parable air man servant. And that Hannah 1994 from the first airport 1940 |
|
|
09:04 | 10,009 miles over the north slope of . Okay so we'll look at satellite |
|
|
09:13 | we started deploying satellites to measure gravity data. Uh 97 9 with the |
|
|
09:18 | sat Nasa launched that. And so just measuring the Earth's magnetic field from |
|
|
09:25 | very high altitude elevation. And then Germans launched the champ 2000 and that |
|
|
09:32 | at about 455 kilometers um of the . And then Nasa and Germany launched |
|
|
09:40 | . And this one is still collecting . There's there's talks on every year |
|
|
09:45 | the age where and they do a of leader not a lot of |
|
|
09:49 | things like environmental relations. And then the E. S. A. |
|
|
09:55 | Space agency launched gold which is a is a great atmosphere. And those |
|
|
10:02 | of what you really want to read history of gravity Magnetics. You can |
|
|
10:05 | out S. E. G. . 75th anniversary articles um with division |
|
|
10:13 | you know I have those if you to. But those uh yeah so |
|
|
10:18 | kind of an introduction into the history gravity Magnetics. Um And any questions |
|
|
10:28 | that observation. Alright so. Alright let's start with potential. Right, |
|
|
10:39 | we're gonna go potential then force and we'll start looking at rock properties. |
|
|
10:47 | . Oh I think everyone really, think it's important to, I mean |
|
|
10:57 | don't think it's I don't think it's necessary to have to be able to |
|
|
11:03 | or write these formulas down from I mean this one, I think |
|
|
11:08 | probably knows that anyways due to this , but it is important to understand |
|
|
11:13 | the potential is they want to force . And so I think those are |
|
|
11:19 | because once you understand those ideas then can start thinking about kind of rocks |
|
|
11:26 | stuff that produce anomalies. So gravitational is just using uh this is the |
|
|
11:34 | constant and it's equal to this right . It changes over time. Um |
|
|
11:41 | the reactions of constant times mass over distance. And so it's actually |
|
|
11:47 | It's the work required to move something a distance, to move a massive |
|
|
11:52 | of the mass over a distance. the Joy is a quick potential surface |
|
|
12:00 | we measure that in meters economy measured meters of ups. Uh But for |
|
|
12:13 | it is sea level. Um Okay , gravitational forest, which is And |
|
|
12:22 | the unit it's uh quality is uh kind of mass per area, |
|
|
12:31 | For probably two masses over area square through that. So you probably remember |
|
|
12:40 | m per second from physics or 32 per second. But that's also 980 |
|
|
12:45 | or 980,000 Milligan and Milligan is the that you always see gravity expressed in |
|
|
12:53 | industry, gravity is always in the . And most data are collected. |
|
|
13:00 | resolution of gravity data is one Typically they're measuring contractors will tell you |
|
|
13:11 | we can measure you know practice of that's fine, you know, But |
|
|
13:16 | one and that is like one part million. So let's grab it. |
|
|
13:21 | be measured with very extreme actors. , so when any potential work of |
|
|
13:27 | is more complicated because the gravity field mono polar. Everything points down the |
|
|
13:31 | field. Di polar. So you you know the poor situation. So |
|
|
13:35 | have two parts of the magnetic field B and H. To make field |
|
|
13:43 | and the the potential B times this uh times delta scale of potential. |
|
|
13:59 | . Right. This is the magnetic potential over there. Um Okay. |
|
|
14:08 | the forest is equal to the sum the two components that Hb H. |
|
|
14:14 | and M. A writer. H . Is the field strength vector. |
|
|
14:18 | M. Is the magnetization like and some of those times the probability is |
|
|
14:24 | to the magnetic funeral. And but this part is important parts in boxes |
|
|
14:32 | we talk about 45 Tesla's might hear say gamma same thing. Um This |
|
|
14:43 | Tesla's or 0.45 Gauss. No one to everyone everyone use when we talk |
|
|
14:51 | . And again the resolution one. that's about 20 clocks in terms of |
|
|
14:58 | . Okay. The field actually ranges over 60,000 to less than £30 At |
|
|
15:05 | Poles. It's like over 60,000. can imagine those flux lines all |
|
|
15:10 | So it's more. And the magnetic is the weakest like 30,000. Just |
|
|
15:16 | you can imagine spreading out. That's it works. So that makes |
|
|
15:22 | It's not computing. Great. So financial is always described as in |
|
|
15:31 | of work, the amount of work to move some particle from one position |
|
|
15:37 | the next position through a field. the idea. So potential is always |
|
|
15:43 | . You know? And If you to, I don't know if you |
|
|
15:47 | about Rick. You want to read this stuff. I think somebody's at |
|
|
15:52 | library but 95. My friend in fact I have some slices and |
|
|
15:58 | wrote a book called theory and dramatic . And so in any case uh |
|
|
16:09 | a pretty good guy. Alright so I mentioned the GOP before the |
|
|
16:16 | I. As I said, it's equal potential service. So what you're |
|
|
16:20 | at here is the relative sea the height of the sea, relative |
|
|
16:26 | the W. G. S Spirit. You know what steroids and |
|
|
16:30 | are. Okay. Yeah. So to WTS. Which is a a |
|
|
16:39 | surface it is a it is derived polynomial has zonal sectoral, all this |
|
|
16:47 | components in and its attempt to best the shape of the so the is |
|
|
16:55 | and it is relative to the it's above it over here. So |
|
|
17:02 | what this means. Is there's some masses out here that's producing that that |
|
|
17:07 | masses here. There's a big mass here that's that's producing these big |
|
|
17:13 | So that's what that means. So is a is a measured surface in |
|
|
17:19 | . So that's important to think Okay, this is a really busy |
|
|
17:26 | . This is from book 2013 and is comparing topography which is this jiggly |
|
|
17:34 | up here, right with the Oid which is this long dash flying |
|
|
17:41 | . Right. So uh so the level, the sea levels down here |
|
|
17:47 | the ellipse oid, which is this uh Why here let's see. And |
|
|
17:58 | all these are just right angles, angles to the to the or oid |
|
|
18:06 | . And this goes to the center the earth dot. So gravity preventers |
|
|
18:13 | the vertical gravity relative to the so other words it's gonna be deflected from |
|
|
18:21 | actual uh angle through the earth. ? So that deflection when people do |
|
|
18:32 | said you measured. Right. So can we can do the oceans with |
|
|
18:38 | data because we have satellites out there measure that when places they measure the |
|
|
18:45 | , they just stack that data out we can measure the marine areas. |
|
|
18:52 | land, land is like it doesn't like why? So we can't measure |
|
|
18:58 | with satellites. These we have to to go in with a meter that |
|
|
19:03 | the gravity but also measures this So there there are joyed measurements which |
|
|
19:11 | gravity measures. They're also have the angle measures. So there are far |
|
|
19:17 | adults. It's free dating download from National Geodetic Survey. The NGS they |
|
|
19:26 | . Okay, so right, normal is defined preferentially avoids here. So |
|
|
19:32 | gravity is to the spirit it looks here. So that's that's the |
|
|
19:37 | Um Yeah. Okay. Alright. that's that's that kind of explains the |
|
|
19:44 | of those those things. Okay, now here's my little case history. |
|
|
19:50 | is um this is Chavez and and they did was these are g Oid |
|
|
19:59 | anomalies over Yellowstone. Right? So the topography. So you know, |
|
|
20:05 | or minus 4,404,000 m on this color . So everything here of course is |
|
|
20:11 | starts over here. Um use the it goes from 2 to 20 |
|
|
20:18 | So it's comparatively tiny. It's a small difference. Only 2020 m 20 |
|
|
20:25 | is like you know nothing in So even though these colors are |
|
|
20:31 | This is just a tiny tiny novel terms of amplifying and then this is |
|
|
20:36 | crust the crust here. This is the service tomorrow. This is going |
|
|
20:42 | on this 30 year 55. So on the order of I would say |
|
|
20:48 | 20 to maybe 60 km that's pretty . And then they did they had |
|
|
20:55 | they tested to s way demographic So this is this is kind of |
|
|
21:03 | I'm gonna do things. I'm gonna you, I'm gonna explain something, |
|
|
21:06 | gonna show some application and all I have all these papers you want |
|
|
21:11 | else? Um So they have this , N. W. U. |
|
|
21:17 | . One one dash S very catchy . And so this is s way |
|
|
21:23 | at depth 50 kilometers, 100 Uh just basically looking at depth slices |
|
|
21:30 | the crust. And this is the always in percent, you probably have |
|
|
21:36 | any commodity bakers before. So when do the pictures they make like this |
|
|
21:42 | always used some percentages of and and do the color scale backwards from what |
|
|
21:55 | do, gravity Magnetics. We always always color magnetic maximum read and minimum |
|
|
22:02 | . But they decided that guys always it the other way around. They |
|
|
22:07 | philosophies, they always blue and slow they call it red. And I |
|
|
22:11 | they do it that way because it right, slow slow and be you |
|
|
22:17 | hot hot would make things slower. ? So that's why they do it |
|
|
22:21 | in any case you can see this this is the the trace of the |
|
|
22:28 | track. But the north America's very you see it going all the way |
|
|
22:34 | . So the inversion of all results both tests indicate that madam densities derived |
|
|
22:40 | can be integrated with tomography to include improve the mantle imaging. And that |
|
|
22:47 | a necessary thing. Mantle imaging It's really important. I mean, |
|
|
22:54 | anomalies are like, okay, so are you looking at? So that's |
|
|
22:58 | degrees right? The resolution of toma to market, I think it's like |
|
|
23:02 | degree like 100 clock in and then It's like 50 club plus mine. |
|
|
23:13 | , so yeah, in any so that's a good thing to |
|
|
23:16 | All right. So, we can for fun, we can look at |
|
|
23:21 | potential uh graduate potential of MArs which , which is of course fun. |
|
|
23:27 | let me see what I have some here. So, right, the |
|
|
23:32 | Southern highlands, this this area here from goth topography. So this this |
|
|
23:42 | topography. MS kurt This is the that they manager from. Okay, |
|
|
23:51 | an airy conversation model. And so predict that a large portion of the |
|
|
23:55 | should be composed of ancient enriched representative sample of primordial crust. And |
|
|
24:03 | think I got my notes pretty Um Right. Published estimates of Meyers |
|
|
24:12 | crustal things have ranged from 1 to clones. And uh in any |
|
|
24:20 | So, So they're saying that this power, this high power, this |
|
|
24:26 | uh root power route of the power this this is harmonic degree 0-30 and |
|
|
24:33 | that this high power um with low degrees is most likely a result of |
|
|
24:41 | load and global flexion associate with this order site. And then this five |
|
|
24:50 | um whenever I go to the, you been to the EU? You |
|
|
24:55 | really go this next year is gonna , this year is gonna be |
|
|
24:59 | It's the best common states. I it's amazing. You should go, |
|
|
25:05 | you can submit a paper, you submit a poster. In any |
|
|
25:11 | It's uh there'll be 20,000 research students and the Eu covers all covers |
|
|
25:22 | oceans, magnetosphere planetary like seeking those those guys don't know anything and they |
|
|
25:30 | big fights and I got no dog the fight. So I like the |
|
|
25:35 | just wanted the one in Chicago. always in December going to the one |
|
|
25:38 | Chicago last month for the first time 2019 there were 17,000 which is pretty |
|
|
25:47 | considering Chicago. So you should think money. It's about if there's 11 |
|
|
25:54 | I would choose that would be the I would for you have a new |
|
|
26:01 | everyday work anyways. Right? So , I like I like the planetary |
|
|
26:05 | because I don't have a dog. , now it's like a magnetic |
|
|
26:12 | Okay. Um so just remember the hat that I talked about before, |
|
|
26:16 | some data from it and this is . So it's very, very tiny |
|
|
26:25 | very very small enough. And the that kind of sticks up at least |
|
|
26:33 | me is that this just looks like data are, I mean it looks |
|
|
26:38 | it's just one dominant waving percolating through . Um, In any case. |
|
|
26:46 | this, the Mag said that's a km altitude and then they convert that |
|
|
26:53 | potential. How do you convert the potentially integrate? So the, the |
|
|
27:00 | when you take the driven potential, get the field and interval, the |
|
|
27:04 | brings it back to potential. so here's the potential and I guess |
|
|
27:09 | is in New Tesla per me Plus or -2.7. So that again |
|
|
27:18 | small and it looks, it looks like this. But uh, it |
|
|
27:24 | like, you know, things are of subdued a little bit like things |
|
|
27:29 | short and a little bit. I wavelengths are kind of like uh |
|
|
27:35 | Alright. And then what they did they downward continued that continuation. We're |
|
|
27:41 | talk about that more Probably tomorrow. think what continuation is is the financial |
|
|
27:48 | he says if you know the field one elevation and you know it every |
|
|
27:54 | . As long as there are no or since between those two elevations. |
|
|
27:59 | , so I think I would continue to 10 km. So it went |
|
|
28:03 | 3 410. So that will But as long as they're still above |
|
|
28:11 | you're probably not going to many So it's probably okay. And again |
|
|
28:16 | can see that now always going are up. They're getting smaller and smaller |
|
|
28:21 | you're getting closer to the source you . So you go from these just |
|
|
28:26 | attention to this area. Here you from those to these and you can |
|
|
28:32 | that the amount is getting smaller smaller you're getting closer to the source. |
|
|
28:36 | that's how it's worked. And then this they did a they did an |
|
|
28:42 | . We're gonna talk about that as . But basically there's two kinds of |
|
|
28:48 | forward modeling. When you take a and you calculate what its responses and |
|
|
28:53 | in responding where you take data and try to figure out what the models |
|
|
28:59 | can invert for rock properties in this magnetic susceptibility. So actually invert this |
|
|
29:06 | is the distribution of the magnetization of rocks. These are s I can't |
|
|
29:13 | that conversion easily. Um Yeah in case my sense is these are not |
|
|
29:22 | but But that if you look at bottom one and and if I can |
|
|
29:31 | at all these bats they're all just alike, aren't they? Um Yeah |
|
|
29:38 | that's an example of potential of magnetic and then of course you got to |
|
|
29:43 | back to mars and then here's a by journey and Stefanik. Um See |
|
|
29:49 | is security. Alright, so let's there the satellite that measures 400 meet |
|
|
30:02 | altitude. And what they did was took 14 die poles. Okay. |
|
|
30:07 | here's the field And then here's the of potential. So this is an |
|
|
30:12 | to get here. And they represented by these 14 disciples trying to model |
|
|
30:18 | field and they're suggesting that this exercise they're interpreting that different stages of |
|
|
30:30 | Yeah. Results suggest states and organizations episodes of the mechanism. So I |
|
|
30:41 | in my notes here that maybe you to take a little break point. |
|
|
30:45 | got a late start. I don't which one keep going. Alright, |
|
|
30:50 | . Good. It's easy with one . There's no disagree. Okay, |
|
|
31:01 | here's I'm sorry. Here's my summary potential. This is after this |
|
|
31:05 | But anyways so remember grabbing our units exploration, millions tests and you might |
|
|
31:15 | old people like me say gammas. exactly the same. Now again, |
|
|
31:27 | is always about work. Okay. the greater potential our field for |
|
|
31:34 | And of course the integral goes back I said and again, once |
|
|
31:39 | five times joy is a measured act potential subjects typically immediately. All |
|
|
31:47 | so that we can graduate from from to force fields. And so there |
|
|
31:55 | the gravity may I feel they are to the fields they are conservative, |
|
|
32:01 | means that they have continuous to emit , they're harmonic because they satisfy the |
|
|
32:06 | equations. In other words, the order differential equation with respect to position |
|
|
32:10 | equal to zero. Del square times field del square is zero. They |
|
|
32:21 | the rotational. In other words, no funny business going on in the |
|
|
32:26 | . They don't like do funny no vorticity. And they're so in |
|
|
32:33 | ? And then that flex through the of zero. So what you got |
|
|
32:36 | going in is the same as what got going out. Um They can |
|
|
32:41 | and contract, but but the field concerned. Okay, so it's a |
|
|
32:46 | confusing to me. And then of they are, they are flux. |
|
|
32:51 | fields, you know, the properties right there measured their measured over now |
|
|
33:00 | . Uh for points and regions that outside appear, they just follow the |
|
|
33:08 | white voice lines reduces, but for inside 245 mrs constant times. I'm |
|
|
33:22 | gonna test your first uh This is F. Y. Okay, so |
|
|
33:28 | law, that's actually Newton's universal law gravitation attraction. And that says the |
|
|
33:34 | between two masses is equal to their or their distance apart times gravitational |
|
|
33:40 | And that's that's something everybody knows. But I mean this is a theoretical |
|
|
33:48 | because the masses are point masses. a non physical. And the distance |
|
|
33:53 | fisherman's. That's also so this constant over time because our ability to measure |
|
|
34:02 | better. So you know Newton's universal of gravitation was thought to be true |
|
|
34:10 | universal to this guy named Albert Einstein demonstrated that this is gravity actually spends |
|
|
34:18 | . So just just to show that still a theory. Still theoretical. |
|
|
34:25 | so this guy got um Friedrich Gauss think um Glosses law basically is is |
|
|
34:35 | this idea that you get this from theory as well that you have this |
|
|
34:40 | can encapsulate some disturbance, some little and a sphere. And you can |
|
|
34:46 | over that sphere. Remember we're talking grades there, right? The same |
|
|
34:50 | of idea. So total massive push the normal component of the graduate |
|
|
34:54 | integrate over a closed mind in the . Yeah so it's a surface integral |
|
|
34:59 | gravitational flux. And uh inside you to use you have to use poison |
|
|
35:06 | that's why I mentioned question so um here's a little example of gravity. |
|
|
35:17 | applying God's law for gravity and it's be, he's using Michael gravity basically |
|
|
35:25 | high resolution measured data over small And um my program is modeled for |
|
|
35:35 | a lot to examine carboniferous limestone, , lime stones and this is in |
|
|
35:43 | catchment area. This public water in southern U. K. Right on |
|
|
35:48 | on the coast. And then we down to Bahamas and they did the |
|
|
35:53 | thing. I mean study by the reefs. And this was for a |
|
|
35:57 | terminal of pork terminal construction to sort make sure there's no voids. You |
|
|
36:03 | what car stitches, right cartridges. like for its like limestone, but |
|
|
36:09 | water will reach out cavities in them then become hazards and big sinkholes ahead |
|
|
36:13 | there or something that's called constituting. yeah. Um, okay, so |
|
|
36:24 | the UK example right here is great and along the coast down here. |
|
|
36:30 | interesting here and along that coast, little tiny here down here, this |
|
|
36:34 | tiny area right here and that area right here. So it's a |
|
|
36:40 | tiny, tiny, uh, but it's okay, it's still gonna |
|
|
36:43 | fun. So look, it goes 70 80 69. So that's 100 |
|
|
36:49 | . So it's like 100 and 20 . It goes from 88 42, |
|
|
36:58 | , 80. So it's 120 it a tiny tiny area. And the |
|
|
37:02 | dots are all the little stations and is Milan that goes from 0.6 minus |
|
|
37:11 | plus 0.38. Okay, so and that adds up to, that |
|
|
37:18 | up to 0.1. So it adds to the whole range is 1/10 of |
|
|
37:26 | . You can do services, but you have to do a lot |
|
|
37:29 | special operations. But this data once you get this, it's actually |
|
|
37:32 | beautiful data and you can see the right here. So these are gonna |
|
|
37:38 | , but you might target those are deficiencies. So that's gonna be where |
|
|
37:42 | might think that there is uh you , a karst feature in it. |
|
|
37:49 | , okay. Um and here's the a little three D rendering of their |
|
|
37:55 | where got to these things. So they're doing is I think they're assuming |
|
|
38:00 | constant density of the invert infrastructure. they have the density counts and then |
|
|
38:06 | that then they have adapted to define these features and that's kind of busy |
|
|
38:11 | I think there's another figure that Oh no, that doesn't. |
|
|
38:15 | so anyways, right, so they hatch into the deepest ones down |
|
|
38:22 | and then they have big areas patch 55, 5 m, five |
|
|
38:35 | Yeah, my own cabinet things in . So what did they say? |
|
|
38:39 | me just okay, This result providing depth incident between two and 5 meters |
|
|
38:52 | our south training features. So best these, I think. Yeah. |
|
|
38:59 | using, Alright, so all right let's jump down to the Bahamas. |
|
|
39:06 | this grand bahama island and it's kind like beneath this thing and this is |
|
|
39:10 | container factory this down here and the ports and they wanna, I guess |
|
|
39:16 | want to out build it's taking here they want to make sure they can |
|
|
39:20 | which is microgravity. Now this let's get some scaling this 79 |
|
|
39:26 | 78 degrees west. That is on word of 100 kilometers, 111 kilometers |
|
|
39:32 | degree. It's always it's always a , so whenever you see in that |
|
|
39:40 | no scale, it's just some Okay so oops. Ah alright so |
|
|
39:51 | this now, this is a little bigger. So this goes from zero |
|
|
39:53 | about 3 50 So it's about 350 350 m. So it's a lot |
|
|
40:02 | . The other ones just like and goes from, okay, they call |
|
|
40:09 | just it's still the lows are still flip they flip the switch, it |
|
|
40:15 | from minus point oh six plus So again the dynamic range is about |
|
|
40:20 | say like point 1/10 of a. And then you see you have this |
|
|
40:25 | eyes in what they called, not one, not only to this cross |
|
|
40:30 | A to B. And then going de sc going, I always I |
|
|
40:35 | know what they're doing it this But anyways C. D. |
|
|
40:38 | Um they intersect this one and this goes here so you can see what |
|
|
40:43 | those results look like. And here have it. So the 20 |
|
|
40:52 | And and and and even hopefully we the exercise. Well the observed it |
|
|
40:58 | always dots. Those represent the actual measures and calculated from modern. Always |
|
|
41:07 | solid one. It's calculated from So here's the result, here's their |
|
|
41:15 | data in the dots versus the calculate is A to B. So here |
|
|
41:20 | have some shallow features and then you this steep feature here. This big |
|
|
41:25 | down here at 10 m depth, m step and see the deep. |
|
|
41:32 | this is actually going south the door they intersect here an anomaly one. |
|
|
41:37 | these these models should tie there uh integrated. All right. Um Is |
|
|
41:45 | anything else I think to himself interesting or was that was? And then |
|
|
41:53 | feature here. This is just they what's called oil or depth estimation and |
|
|
41:58 | going to learn about that. Um , alright. For Magnetics. So |
|
|
42:08 | it is of course more comfort. this this is the formula for so |
|
|
42:14 | uh our regional integral of del field normal to the field. So that's |
|
|
42:28 | a like a. O. Is do a here's what happened and what |
|
|
42:37 | find one of them wasn't good enough up. It's not asking me it's |
|
|
42:49 | now. Yes, I stopped. stopped. Right. Yeah, |
|
|
42:54 | Yeah. Um Okay. Right. yeah, so it's it's very simple |
|
|
43:02 | to like we were talking about in beginning before class. You know, |
|
|
43:06 | this is all, can you pull the it's the same sort of |
|
|
43:11 | Okay, the magnetosphere. So the magnetic field interacts with solar winds to |
|
|
43:22 | the magnetosphere. So the Earth is slow circle down here is here down |
|
|
43:28 | . But then you have, you the plasma sphere, this geometry of |
|
|
43:31 | solar winds are blowing this way. the main atmosphere is important. It's |
|
|
43:37 | so you understand how have you seen figures like this before? Yeah, |
|
|
43:45 | simple ones. But this one is really nice one. And because it |
|
|
43:50 | the different components plasma sphere, the ring currents, plasma sheet, magnetic |
|
|
43:55 | , plasma, mantle tail, current then what they call the inter |
|
|
44:00 | And then the magneto pause. you know, lots of stuff to |
|
|
44:06 | about. But in any case just get your sense of what the magnetic |
|
|
44:10 | magnetosphere around the Earth looks like. then um I'm sure you've heard of |
|
|
44:15 | Northern lights, right? Aurora So that's where you've seen. |
|
|
44:23 | So yeah, so that's basically um when the solar winds interact with the |
|
|
44:31 | at the polls, because the you know, the the fuel lines |
|
|
44:35 | converging, getting vertical uh electrons are in the other atmosphere when they lose |
|
|
44:43 | energy debate in the So yeah, are that's just and uh whatever. |
|
|
44:51 | and the fact of the magnetosphere. , so getting back to the Earth |
|
|
44:56 | a giant magnet under as well, would say the geographic north pole, |
|
|
45:05 | ? Is that where the magnetic north the magnetic north pole is, you |
|
|
45:10 | sort of at a different angle that is called declination. And then of |
|
|
45:16 | the field comes out of one pole rapture and goes to the other |
|
|
45:21 | So what that means is that the earth cornfield? What I'm talking about |
|
|
45:27 | , it is inclined at different angles on where you are at on the |
|
|
45:33 | . So this is called declination at magnetic equator field is you know, |
|
|
45:40 | uh flat as we say, say flat, zero inclination is horizontal. |
|
|
45:47 | then of course at the poles that magnetic pole, rather the field is |
|
|
45:51 | . Okay. And as I it's it's well over 60,000. Less |
|
|
45:56 | 30,000 when you go from pool. , so here's a contour map of |
|
|
46:04 | magnetic field intensity. Right? So is 20, you can see this |
|
|
46:08 | 25,000 going up. These are 5000 . So that's 30 35 40 45 |
|
|
46:18 | 55,000. And this goes up here to I think that's 85,000. There's |
|
|
46:25 | southern pole. The maps only go or minus 70 degrees the north |
|
|
46:32 | So sweet. Is that it? guess that's it. That's the north |
|
|
46:36 | , is it? And we have . Yeah disclosure there now I think |
|
|
46:41 | pulls them somewhere else. Yeah. . Alright. So we can look |
|
|
46:47 | the inclination. So this is the core here, this yellow line and |
|
|
46:54 | goes up to let's see these these by 20. So there's 2040 60 |
|
|
47:01 | . Yeah, it doesn't go it doesn't go up to 80. |
|
|
47:08 | these are by Tuesday, is that ? Yeah. 2 to 4. |
|
|
47:15 | 86 degrees inclination. But this is magnetic sample. That's 80. That's |
|
|
47:23 | the 2468. Yeah. So that's the inclination. You can see that |
|
|
47:31 | magnetic. So here's the here's the equator. So they're roughly satisfied. |
|
|
47:38 | not really. This is well. . And that's fine. Let's look |
|
|
47:45 | duck. So this means this is angle. So this is so this |
|
|
47:51 | is my and this is zero degrees . Those lines all run straight into |
|
|
47:58 | pole. Right? Here is the pole. So all these declarations like |
|
|
48:03 | here is gonna you know. And I think yeah reds are positive |
|
|
48:08 | lose their negative. So bed for methods we have to adjust the |
|
|
48:17 | All right. Right. Right. . Exactly. Right. Yeah. |
|
|
48:25 | Okay. Let's just dig into because some important concepts to understand it. |
|
|
48:31 | then so at either pole, north soft pole the magnetic field produced. |
|
|
48:37 | mean, it's only if the magnetization only from the inducing field and the |
|
|
48:45 | will produce the symmetric hot. No what annual you transact through the |
|
|
48:52 | Doesn't matter. It will produce a economy. The same source body. |
|
|
48:59 | mean it will be magnetized this way at the magnetic equated depends on what |
|
|
49:07 | . So from south to north it produce this magnetic mode. Right? |
|
|
49:14 | then so yeah, the inducing field write the same thing. So you |
|
|
49:21 | this risk is horizontal. Right? . So that means in between the |
|
|
49:30 | and polls in the northern atmosphere you a what we call an anomaly taker |
|
|
49:40 | the source will be so this is So this will be right in that |
|
|
49:45 | halfway between the low. So in northern hemisphere the high of the |
|
|
49:51 | there is always south of the source is a direction and in the southern |
|
|
49:59 | high is north of the certified. . So what does that look like |
|
|
50:07 | three dimensions. So here we have same source, the square Q. |
|
|
50:14 | and north pole. It produces a heil just like can you see that |
|
|
50:20 | these kind of tours? See that at the magnetic equator it produces, |
|
|
50:28 | is why this. Now you're getting sense for a while I say south |
|
|
50:31 | north south to north. And and it's always sort of but the same |
|
|
50:37 | for produced this symmetric lo So now you go from here just down to |
|
|
50:49 | inclination, you can see that this starts to migrate southward. You start |
|
|
50:54 | develop low at the northern part of . You go down another 30° and |
|
|
51:00 | highest migrated down here. Now the was here. And then you go |
|
|
51:04 | a pretty good deal up to See how that how that works. |
|
|
51:08 | know from here to here to here here actually I said little is abc |
|
|
51:17 | but you would go as you you know as your as your source |
|
|
51:23 | softly in the northern hemisphere. What the south pole? So. |
|
|
51:29 | Two things at the same time saying pole equator obviously the equator. But |
|
|
51:34 | see that's the same monopoly and all all I did from because it's so |
|
|
51:41 | you're at the south pole again it's poll. So there's the same the |
|
|
51:46 | . But then as you move north latitude 60°. You see that this this |
|
|
51:52 | now the high sense to moderate uh the North. Right? And as |
|
|
51:58 | you and as you go closer to equator of the high line further and |
|
|
52:04 | finally the highest place quite well as . So it's the same thing |
|
|
52:11 | But that's that help you visualize how last night again we talked at |
|
|
52:18 | S. H. Meeting and there a profile, a magnetic profile and |
|
|
52:25 | was a model and I said it to me like it's hemisphere. Absolutely |
|
|
52:35 | . And I knew that because the between the profile of. Okay, |
|
|
52:46 | this is this is a historical reference God. So gas. Um. |
|
|
52:56 | . Yeah. Yeah. So uh earliest recorded magnetic intensity is useful for |
|
|
53:01 | present politics stuff. This is from this is 9 18 44. This |
|
|
53:08 | an old paper, the first the um Measurements of 1790s. Okay. |
|
|
53:18 | God's developed method in 1832. So Lewis is doing, he said I |
|
|
53:24 | to test it. So he's gonna to these cities around the world and |
|
|
53:28 | the magnetic field and compare this. go go's presented his law. His |
|
|
53:34 | in 1831. Loomis tested it Um direct measurements in 1844. Just pay |
|
|
53:43 | we now for the few elements Okay so what I'm calling dr nation |
|
|
53:49 | called variant when I call inclination they what I call field trip. They |
|
|
53:54 | intense. So there's some terminology. What is not to say the appearance |
|
|
54:01 | a general theory of terrestrial magnetism from name. So celebrated back in the |
|
|
54:07 | uh furnishing the three elements inspiration. have computed from the three elements of |
|
|
54:16 | Station, the four tablespoons. So just show you one. So here's |
|
|
54:19 | of the tables from that paper. again, so here's declamation, inclination |
|
|
54:27 | field strength. And you have different Montreal Syracuse, Albany, Albany spring |
|
|
54:35 | Hartford whatever most of them. The here's here's Loomis I think from yeah |
|
|
54:47 | measurement is from uh cause presented oh he presented a law. So he's |
|
|
54:57 | his idea. And so this is difference in a degree. So to |
|
|
55:04 | . Anyways. So that's that's some scientific historical stuff. And This is |
|
|
55:13 | Loomis conclusion he says from the sealed way they talked to deal with uh |
|
|
55:19 | is not manifested in respect to magnetic . We may expect that in a |
|
|
55:23 | years the errors of God's theory for part of global. Pretty well known |
|
|
55:28 | it is to be hoped to The illustrious author, resume the discussion |
|
|
55:34 | give this theory the greatest. So is a very famous man is big |
|
|
55:37 | of in Brunswick Germany. And then an 18th session compass. Just for |
|
|
55:44 | . I just stopped at it. Okay so the summary of of magnetic |
|
|
55:52 | fields, gravity. The r vector , they obey the classes uh equation |
|
|
55:58 | poisons equations. Um Law are the for calculating potential fields and the Earth's |
|
|
56:06 | field. So the same source will a different not only shape depending on |
|
|
56:13 | it is on the earth and So that's really because of the |
|
|
56:18 | declination feels straight. Okay, so you wanna take a little break |
|
|
56:24 | Good. Good, good. So 17. Am I going too |
|
|
56:38 | All right. I mean I just I mean so that's the theoretical stuff |
|
|
56:44 | I'd like to just now we're gonna about density and magnetization. Okay, |
|
|
56:49 | we start with that easiest for um both density is controlled and controlled by |
|
|
56:57 | minister of the grain density porosity and course space fluid. And you can |
|
|
57:01 | this by weighing a sample and air adversity of water. And the difference |
|
|
57:07 | gonna be what it's um it's measured by relating ferocity to the matrix |
|
|
57:15 | Robi That's that's gambling. But there also roby measurements like um it's estimated |
|
|
57:23 | by assuming that increases like passion will you some examples of that. Um |
|
|
57:29 | the units we use graphic here gcc often literature, you might see kilogram |
|
|
57:39 | usually industry, everybody talks. So rocks in generally range from 1.92 |
|
|
57:52 | basically Crystal and Ross in the The upper crust brand. Um |
|
|
58:01 | in general. These are just rules thumb. Lower across 2.9-3. And |
|
|
58:08 | the upper mantle uh will be right , 3.2, maybe a little bit |
|
|
58:17 | if it's like close to a spreading . Okay, so We're gonna track |
|
|
58:26 | of three rock types Sansom granite and various sources, there's just, you |
|
|
58:36 | , there's just tons of literature out that have these tabulated uh rock samples |
|
|
58:44 | their destinies and their mechanization center. ? So here's a fraction of all |
|
|
58:51 | from Carmichael. Carmichael is, you , CRC manuals goes up. CRC |
|
|
58:58 | all kinds of mathematical table. They rockets, right? So Carmichael. |
|
|
59:04 | is mathematical CRC handbook rock properties. , So here's Here's the comparison of |
|
|
59:13 | bulk densities actually frequencies. So a of granite. Right? The density |
|
|
59:21 | sandstone density. This is dash It's pretty variable assaults. They're more |
|
|
59:28 | , but they can be sent down . So, but these are the |
|
|
59:32 | things. So sand stones are typically the range range here density some |
|
|
59:37 | It's in here. And what's also ? Just as a sort of |
|
|
59:43 | Okay, we can look specifically at . This is from Carmichael again. |
|
|
59:47 | . So the main density from their 2.2 Plus 9.2 Standard Deviation. And |
|
|
59:57 | is a history graham showing that the of densities pretty well behaved Granted. |
|
|
60:05 | mean, that is 2.66 And That's very well. So, I |
|
|
60:13 | , I've always used like 2.7. the boot a correction and which is |
|
|
60:22 | of the gravity crisis we'll learn But 2.67. Identity of parts. |
|
|
60:28 | yeah. So this is the that's very well behaved data set. How |
|
|
60:33 | samples did they had? What do say? Uh So 3334. |
|
|
60:44 | 334 I guess. Yeah. So a lot of savage And the |
|
|
60:50 | So they're saying the mean is That's um medium rather is to question |
|
|
60:57 | mean is 2.74. I've got the ones. Go back, go |
|
|
61:00 | go back, go back. that's the same. That's the |
|
|
61:05 | This is a little different. So means 2.74 standard .47. So, |
|
|
61:12 | it can be low density. What it lower densities? You can have |
|
|
61:17 | erupted the salt their best killer. have bubbles in them and stuff. |
|
|
61:24 | that will lower the density. That's that's what all this nonsense is. |
|
|
61:27 | like I've modeled seamounts in the south . They have like densities like please |
|
|
61:36 | on the ocean floor, but they this kind of dense okay ball ranges |
|
|
61:44 | bulk density for rocks with insufficient All right. So, in other |
|
|
61:47 | , no, no more history. here's the range and hydrate 2.8 to |
|
|
61:53 | . I'm just gonna circle on a of these. And hydra, that's |
|
|
61:57 | precipitation. Right? So, when you know, in where you |
|
|
62:01 | like in reasons like salt is you can also end up precipitating an |
|
|
62:08 | , which is modus We're salt Right? So 2.1 or 2.2. |
|
|
62:14 | used 2.16 in the industry typically. No. Does it sound but it |
|
|
62:20 | also precipitate, you know, and 2.8-2019 for chips. So the chips |
|
|
62:26 | in here. There's no chip Okay. And then of course, |
|
|
62:34 | can look at some uh carmen's don't limestone, 1.5, That's really very |
|
|
62:42 | again, that's because this maybe this , you know, limestone that, |
|
|
62:49 | know, that is not very This might be like limestone with corals |
|
|
62:57 | stuff like that. And I think close to some kind of change. |
|
|
63:03 | 2.7. Okay, let's look at . Under cemetery shale. 2.062. |
|
|
63:13 | that's again, that's really very, just depends on it's compacted and |
|
|
63:18 | alright, let's look at some. So these these are metamorphic rocks. |
|
|
63:25 | 2.59 to 2.84. That's like lower 2.673 point one prototype. That's like |
|
|
63:35 | rocks 3.1 point 274. So I highlighted the ones that are, that |
|
|
63:45 | really kind of more common for me catch my eye. Okay, now |
|
|
63:52 | stances from Sharma, another source Sharma . There's a, there's a newer |
|
|
63:59 | , I think it's 81 or But sandstone here 2.152 point 42.73 point |
|
|
64:08 | granted. 3.2 point 5 to So just kind of tracking our |
|
|
64:13 | Call me index rocks. Just for edification here, we're looking to get |
|
|
64:20 | And 211. Okay, California this is a handler Bob sheriff, |
|
|
64:28 | of them um sand stones, So the average 2.35. And then |
|
|
64:40 | okay, they have wet and dry granted from Salford uh 2.5 With the |
|
|
64:50 | and an average of 2.64 assaults? 2.99 average. That's really high. |
|
|
64:57 | really really high. That's a 76 . Okay, 1988. Another |
|
|
65:06 | So here he has a bunch of stones from different parts of the |
|
|
65:10 | different parts of the United States. there's some great Britain Switzerland but mostly |
|
|
65:16 | U. S. And To see is a high value 2.17 down |
|
|
65:24 | So sedimentary rocks can be more very you can imagine because they can be |
|
|
65:30 | levels of compaction. Different companies with units. What am I looking at |
|
|
65:37 | ? So this again, this is going like chalk and marble. So |
|
|
65:42 | are different formations in Edinburgh is very formation out in West Permian basin. |
|
|
65:51 | it's co evil with what we call the NOX the NOX like in |
|
|
65:57 | Um Yeah, but so these are carbonates, um marble is a metamorphic |
|
|
66:05 | but I guess Metamorphosis Card, it be anyways, densities, saturated, |
|
|
66:13 | density 2.75. So these are 2.26 the lowest one I see here up |
|
|
66:20 | 2.8. That's really, that's really . But that's the total lights, |
|
|
66:27 | the lights are gonna be more Okay. Glenn roles in texas. |
|
|
66:35 | , So just more examples. You use these as a resource I |
|
|
66:40 | So I don't have a shale placed a slate. So slate is a |
|
|
66:46 | . So where's the slave show? are all everybody you all just |
|
|
66:52 | Um 2.4, is the lowest one see here. 2.66. And then |
|
|
67:02 | sand, clay, gravel. And this is very loose, shallow |
|
|
67:05 | They're all very light, but at , just under two. So, |
|
|
67:12 | you would imagine, because they're in surface, they're not compacted at |
|
|
67:18 | Okay, granted they say mean density , which is really consistent. The |
|
|
67:26 | is 2.5.8. So that looks consistent the other work. All right. |
|
|
67:33 | what is all this stuff? What I doing going? So, I |
|
|
67:36 | this little summary Carmichael C. S telford at all. T |
|
|
67:44 | Right, so sandstone means two x - 2.42. And for each of |
|
|
67:53 | , overall the sandstone has two point does that fall on our graph? |
|
|
68:00 | about here. That's pretty good. all those different sources, Granted from |
|
|
68:07 | those ones. Average 2.67. well, granted. uh it's probably |
|
|
68:15 | averages 20 little bit bullish. Carmichael , You said 2.66. And then |
|
|
68:24 | was salt 2.96. So it looks looks about right as well. So |
|
|
68:33 | this this is kind of some good to kind of keep in your head |
|
|
68:38 | you're thinking about these rocks because these numbers that are pulled from man, |
|
|
68:45 | good. Good to know. And um Ok, so, Alright, |
|
|
68:49 | , hi, this is again average of surface and of course based on |
|
|
68:54 | referred was from mobile oil. So of samples, 617 2.32 for |
|
|
69:03 | 2.42 for shale. 2.54 for 2.61 for specifically, that means |
|
|
69:12 | And they only have 101 105 cent metamorphic, which is pretty one. |
|
|
69:20 | And then But so basically, so so I think this is consistent with |
|
|
69:29 | summary from before. This is this from behind and they're just doing the |
|
|
69:35 | stuff. But they're kind of I'm showing because it's kind of a neat |
|
|
69:38 | to plot this data out. So going from 13 plus grass or cubic |
|
|
69:45 | and you have different kinds of So up here are these are all |
|
|
69:49 | are precipitated these salts. Um sandstone gap grows cyanide um miles. |
|
|
69:59 | I'm just my circle dollars, Right? So everything the three standards |
|
|
70:05 | been tracing through all this seemed to and uh right along. And I |
|
|
70:10 | that if you look into this stuff compare these ranges with the other |
|
|
70:14 | you would find it. This this is probably pretty good. Okay, |
|
|
70:20 | that's Hanson, that's just physically measured . You can also measure density in |
|
|
70:26 | , well, right. Um, is both density for every cubic centimeter |
|
|
70:32 | goes 2-3. And so this is and you see everything is just under |
|
|
70:38 | . Right? So things go from about 2.5 to around 2.5, maybe |
|
|
70:46 | , something like that. So that's density as a function of top. |
|
|
70:55 | so if you were to quite honorably data, what we do is we |
|
|
70:59 | of come up with a depth you know, layering structure because you |
|
|
71:05 | do things I mean is based on , there's no that density function to |
|
|
71:13 | into the layer. So you would block this out. I mean, |
|
|
71:18 | is one density to hear another another interval. Where is this |
|
|
71:24 | So and so forth. Kind of a lot. So another example you |
|
|
71:32 | convert from velocity, right? From laws. There's uh, there's some |
|
|
71:38 | by uh, Jerry Gardner used to at this university. He did a |
|
|
71:43 | paper 97 for gardener and gardener and know about that. Okay, |
|
|
71:51 | so jerry, I took two Right? So here's our you do |
|
|
71:57 | same thing. You can block that into into velocity region and then you |
|
|
72:03 | go to Gardner, I think I buried the next slide cross my |
|
|
72:09 | Yeah, so here's the table. has to figure out if Gardner jerry's |
|
|
72:13 | and you see for different mythologies, has a, the philosopher just has |
|
|
72:20 | velocity percent on this side and the gets me on this side, these |
|
|
72:27 | logs. But so you could, know, measures that you have the |
|
|
72:34 | here, density and he has limestone, dolomite and hydrated. But |
|
|
72:40 | also has this, it's uh 123 velocity to the corner of And people |
|
|
72:53 | that relationship still today. Now this published a paper uh, whatever 15 |
|
|
73:05 | ago. Uh, and he could , here's Gardner's equation. So we |
|
|
73:13 | talked about, but then we also in another one. This is a |
|
|
73:17 | famous one, the Nathan drake which is after Ludwig, the name |
|
|
73:23 | . And that's just one that goes here and christian ceremony published the paper |
|
|
73:28 | just do compliments. Yes, their . Um, Godfrey, right, |
|
|
73:36 | freak some based on oceanic rocks. that's this profile here. What |
|
|
73:50 | Here we go now. Okay, . Um, right density from |
|
|
74:02 | so uh, this, this is same increments. I just showed you |
|
|
74:10 | , in the table. I have , uh, I didn't give you |
|
|
74:16 | spreadsheet, but this is stalled, for all these. I mean it's |
|
|
74:20 | in BP and actually um, the is that this snake drakkar we solved |
|
|
74:30 | analytically. So there's a formula and this is that's uh, feet |
|
|
74:39 | second. The other one was meters second, right? Yeah. |
|
|
74:44 | Now on sanitary basis because rock mostly . They as as they get buried |
|
|
74:52 | get more and more dense compassion. ? So there's a whole bunch of |
|
|
74:57 | that study this. And you could the compassion with the death density profile |
|
|
75:08 | presidency based on some exponential decay Right? And this is it. |
|
|
75:12 | in this case 2.7. Right? um Z goes to infinity. This |
|
|
75:21 | 2.7. Okay. Now if zero it's c If Z is zero then |
|
|
75:34 | . So here it is. See sets the desk for zero |
|
|
75:37 | So if if you use minus 0.55 . Then you're gonna end up. |
|
|
75:46 | then the zero debt is gonna be . I I use this function. |
|
|
75:53 | used it to model onshore offshore Like I didn't model the whole top |
|
|
75:59 | land. So the land part. you can't even even 2.15 is a |
|
|
76:05 | too low for land, it's a too high for water body motion. |
|
|
76:10 | bottoms. But you can't use to different density because then you have a |
|
|
76:15 | at the coastline and that would look . So so I use this |
|
|
76:19 | So I use 2.15. Used to C. Sets the minimum and then |
|
|
76:27 | . Is of course in in depth kilometers and K. Is the shape |
|
|
76:31 | this. So um this one uses minus 0.2. But if I use |
|
|
76:39 | .4 U. Shaped this will go this. Everybody's .1 shape of. |
|
|
76:46 | what you do is if you have bunch of wells you populate, make |
|
|
76:51 | scattered clouds as wells. And then just use this function you diddle with |
|
|
76:57 | gentleman to see and the first So you figure out this range and |
|
|
77:03 | you play around with K. So get the best fit kind of curved |
|
|
77:07 | then you can apply that to other areas when you're modeling. Yeah. |
|
|
77:15 | . Now here's an important thing to salt salt is like the fluid is |
|
|
77:23 | . So that and and its density the industry we used 2.1 cents. |
|
|
77:28 | everyone recognized it could be a little be, you know could be but |
|
|
77:33 | a dirty soft. There might be sort of mixture of some sentences. |
|
|
77:38 | . Um What that means is that shallow sediments are gonna be lower density |
|
|
77:46 | the song. And but but mostly sediments are gonna be much higher |
|
|
77:55 | So that's what we call a crossover . The stash alone and it's typically |
|
|
78:01 | 1200 m below the poverty or about ft. That's a good number to |
|
|
78:06 | on. You never think about But it's so what do you |
|
|
78:11 | This is an old paper? Anything but it really illustrates this very |
|
|
78:16 | Now they're doing this as a function d right? But it still it |
|
|
78:21 | worked. You can just think of in terms of salt is beneath the |
|
|
78:27 | depth and as as the height of salt crosses it's above the cross over |
|
|
78:32 | depth you start to see this. this part here the nominees broad part |
|
|
78:38 | being produced by this thick deep low contracts. But the upper part is |
|
|
78:44 | produced this bit here being produced by shallow party. So you have this |
|
|
78:51 | anomaly that shows you that's that's a anomaly for salt. Sometimes here's the |
|
|
79:01 | . Sometimes it all could be done but you could have right, it's |
|
|
79:07 | high intensity it's precipitates another middle. that could also be produced by so |
|
|
79:15 | could be two things, it could the salt is telling you about the |
|
|
79:18 | it could be this cap right on of that song. Okay, okay |
|
|
79:26 | I have here a little model and I'm gonna have I'm gonna show you |
|
|
79:31 | example of a two dimensional cross sectional from the literature and I like this |
|
|
79:36 | because I don't know if you've seen seen this favorable versus up it's pervasive |
|
|
79:44 | was great things man and everybody likes time I complain about this, people |
|
|
79:50 | well he's a nice or or or they know him you know I know |
|
|
79:56 | a really nice. So this is they always say that? So that's |
|
|
80:00 | of right? But okay, so okay, so he has this idea |
|
|
80:05 | he says that the breakup now this the breakup of this is this is |
|
|
80:10 | this is before Panji. So he that he can map spreading segments and |
|
|
80:22 | from, so there are now beneath Appalachian and I think that's just |
|
|
80:30 | I mean that's like saying you can the bridge and transforms, right? |
|
|
80:37 | just defies logic. So um and and plus there's a there's a it's |
|
|
80:47 | rift. So it's a special powder they're just dead end. They don't |
|
|
80:52 | . Um So, so this is risk which which required some sort of |
|
|
81:00 | thought or some sort of even oblique . He's got he's got extensive going |
|
|
81:05 | way to represent that's not physical Right? So I think, and |
|
|
81:12 | say, okay, so here's of course there's the Mississippi investment. |
|
|
81:18 | are all rest bases that form with . Okay, so these are these |
|
|
81:26 | protozoa and Cambrian teachers. Well, I think that and this is just |
|
|
81:40 | brief extension together because because I just that's just that anyways like I |
|
|
81:54 | but yeah, anyway, so it's . So here here's this feature laying |
|
|
82:01 | top of the graph, his same . Um here's the now this was |
|
|
82:07 | in pennsylvania with the collision of south and africa. Right? So this |
|
|
82:14 | this, this popped up at the time central basin platform. You've heard |
|
|
82:18 | before, it's in the middle of Permian basin. Um you've heard of |
|
|
82:23 | ancestral rockies. So those those you look at but the ancestral rockies which |
|
|
82:33 | oriented and which is which is where Oklahoma used to be. But then |
|
|
82:44 | inverted. He's all for intensity with of America and there's right, but |
|
|
82:55 | these pictures were Denver but the Mississippi see is high, high, that's |
|
|
83:02 | the rift, this is right, not here, that's the rift and |
|
|
83:06 | the wrong trough comes up, comes through here. Yeah. Anyways, |
|
|
83:15 | the graph and then here's the view so there's right, there's they model |
|
|
83:24 | slab, Right? But he's here then the collision of Africa and South |
|
|
83:33 | Gun one. Now um the slabs it this way because there's no |
|
|
83:41 | that's why we think the the other because and here's a little mom, |
|
|
83:49 | think this plan's a little flawed. this is 25 km and they have |
|
|
83:56 | have basin sediments going down 25 there is no base that people in |
|
|
84:01 | world that is not physically, 25 on this planet, it's just not |
|
|
84:07 | . Okay, the deepest basins on planet are 16-18 there's no there's no |
|
|
84:17 | face. I mean there are some are as deep as nine, maybe |
|
|
84:21 | , but most time based seven So okay, so that was 25 |
|
|
84:28 | . And then they have a whole of different things. But see I |
|
|
84:31 | made a model of that and I , well you know what actually if |
|
|
84:35 | just use some reasonable dents, you have to have all this complexity. |
|
|
84:40 | can just model this way. I think you can model slabs, |
|
|
84:43 | argue they're not easy to model, that Dennis had some really elevated |
|
|
84:50 | But yeah, so I think they their their model goes like this. |
|
|
84:56 | I think really this is kind of to my my attitude about modeling and |
|
|
85:03 | using the same density control that he in this paper. So my idea |
|
|
85:10 | is you only have. Alright, um All right, let's talk about |
|
|
85:25 | mechanization around. So rock magnetization is more complex dense rock samples remnant and |
|
|
85:31 | . So they can be induced. can be magnetized by the inducing field |
|
|
85:35 | also they might carry some remnants from previous mechanization. Feel about that. |
|
|
85:39 | heard about that. Okay, Alright, so rock school Um typically |
|
|
85:45 | less than 580 500. Once they're to the point where they capture the |
|
|
85:53 | uh magnets, if they can do . If they had minerals that can |
|
|
85:57 | magnetized, they will capture the inducing orientation. Right? Well then if |
|
|
86:04 | rock moves around plate tectonics, Blah Blah slipped around or anything. It |
|
|
86:11 | it will begin to be magnetized by new industry but it will retain it |
|
|
86:18 | retain some of the original organization that's remnants. Okay. And there can |
|
|
86:24 | primary readiness. There can be secondary to get the picture right because rocks |
|
|
86:29 | a long time. Um Alright, it can be highly variable even at |
|
|
86:35 | scale there can be reversed magnetism, remnants. Like sea floor spreading |
|
|
86:41 | You heard about those? Those are those those are reversed magnetize the ones |
|
|
86:45 | are pointing the wrong direction. So the opposite. Don't be wrong but |
|
|
86:50 | the opposite direction. Okay, so Maxwell again, there are two kinds |
|
|
86:54 | magnetic fields of the field and the that we talked about. Um They're |
|
|
87:01 | to one around. Again, the abilities will be probability. So, |
|
|
87:07 | there are the common magnetic metals. two groups according to charlotte. There's |
|
|
87:12 | iron titanium oxygen group, F E E two, S. E O |
|
|
87:18 | 203. That's a turner system. is an iron software. Okay. |
|
|
87:27 | That's kind of why I'm not gonna that. Alright, so the types |
|
|
87:31 | 19 was dying. And that's where . The little diet polls are actually |
|
|
87:38 | up in opposition of the industry, is dying magnetic. It's weakly |
|
|
87:44 | So but but the little things, little that can oppose the inducing |
|
|
87:48 | Okay, this para magnetic which is small field is induced under the inducing |
|
|
87:56 | but it's tiny and it's really insignificant us. We don't care about the |
|
|
88:01 | we want. The one we care the most I say worry about is |
|
|
88:05 | alike and that's a product of spontaneous is very formal for pedestrian. So |
|
|
88:11 | you have a rock with arbitrary domains but once you hit the feeling |
|
|
88:17 | magnetized and induces your direction. Okay here again is our strongly magnetized our |
|
|
88:26 | magnetic source. So run in So as I said is a current |
|
|
88:33 | of the rock independent of the applied so that once ahead once it gets |
|
|
88:38 | primary mechanism is gonna hold on So then after you rotate it then |
|
|
88:44 | I said you have some you have combination. And basically the magnet measured |
|
|
88:49 | is equal to the industry field is vector of Plus the remedy. Very |
|
|
88:57 | , very easy to understand. Um actually like 14 but I'm just gonna |
|
|
89:05 | 70. So run and mechanization, ? So what whenever you mention accusation |
|
|
89:14 | all all it's called the batch of right? These are all but there's |
|
|
89:21 | is thermal rent. So this is in rock school below the period temperature |
|
|
89:27 | a. Okay. There's a So that means grains that were previously |
|
|
89:36 | but they're forming there there they are a component in a sedimentary rock. |
|
|
89:44 | will align in the field direction, ? There's crystallization or chemical remnants so |
|
|
89:52 | acquired at the time of new creation growth of crystallization of magnetic grains that |
|
|
90:01 | will retain the remnants and as long they're below the curie point. And |
|
|
90:06 | you have a remnant magnetization tabling, pizzo remnant. So that's under mechanical |
|
|
90:12 | . So if the rocks are they can be magnetized on that one |
|
|
90:17 | reverse. So that that acquired And I can't think of an example |
|
|
90:23 | this is in other words, there's , random mechanization that is acquired under |
|
|
90:31 | tension. So lightning strikes. So you can be then there's |
|
|
90:38 | This is a long term explosion to a nice. So there's lots |
|
|
90:46 | different kinds of remnants. They exist . Okay, let's let's go back |
|
|
90:52 | our favorite three little rocks here, granted. And best salt. And |
|
|
90:58 | can see the magnetization. So let's susceptibility. This is in micro |
|
|
91:05 | These are humans island. There's in literature, there's people with all different |
|
|
91:09 | of uh units, but it's also sedimentary rise. They are effectively not |
|
|
91:19 | or metamorphic rocks. See how tiny are. They're all down here. |
|
|
91:25 | think the nominal value people use for rocks is 70 In an animal. |
|
|
91:32 | you solve this -10. But igneous . All right now this is 600 |
|
|
91:40 | typically use about 2000 grants and for microts this this is 6 47. |
|
|
91:50 | pretty low 25. That's, that's low for uh Okay, so this |
|
|
91:58 | from dobbin and savage. Let's Do I have some more? Of |
|
|
92:01 | I do. But back to So they had Sansone 230 samples um |
|
|
92:09 | of the four avenue micro. So is this is 10 to the minus |
|
|
92:21 | . No, this is this is is tantamount. That's um Michael |
|
|
92:24 | D. S. Right, So 0 to 1665. That's a really |
|
|
92:29 | value. Oh and then um but of you should see are pretty |
|
|
92:35 | I don't know anything about that number 1,000 4000. I believe that. |
|
|
92:40 | was wretched. And then they have samples here, like Minnesota, Oklahoma |
|
|
92:46 | so forth. They had whatever they . Sure. For samples. |
|
|
92:56 | 100 to 800 beds. I Okay, the salt. So 2100 |
|
|
93:04 | that 100 27 samples 900. That's low, 84 80 400. Now |
|
|
93:11 | talking like that 6000. That's Some of these in Australia. |
|
|
93:20 | That's extraordinary. Um 20 900. what what what are you learning here |
|
|
93:27 | this stuff that susceptibilities are all over place. There's no there's no |
|
|
93:34 | Wait. Right, so what we're at here, we're looking at |
|
|
93:37 | this is the salt continue. Yeah. Okay. Um Now this |
|
|
93:46 | sharp granite. 22 40,000. I don't believe that because I had |
|
|
93:54 | model stuff like salt 502 £120. extorting sand stones 35 to 19. |
|
|
94:04 | would never give it that high but I like 35 35 to 70 |
|
|
94:11 | . Let's see if I have some . Of course I do. |
|
|
94:13 | This is back to tell food. stones 016 60 that remember 0 to |
|
|
94:22 | to 14,500. So, in since the sedimentary rocks are very |
|
|
94:30 | sand stones are pretty high in major . Assault gag rules. They're very |
|
|
94:37 | Megan. That makes sense. The oceanic rocks are full of iron |
|
|
94:43 | manganese and you know, granted are , there's a high degree of |
|
|
94:50 | And and uh so they're not gonna left. Okay, so we're going |
|
|
94:59 | to dover and savage sandstone 16.8 25 - 2700. The south. |
|
|
95:12 | bad. Um This is a this kind of it's a nice exercise because |
|
|
95:18 | see how different everyone has. So, all right. Again, |
|
|
95:24 | Major. Right, So this is again, basic intrusive. Uh |
|
|
95:32 | Oh, actually this is right, is the range. That's the number |
|
|
95:35 | samples in those ranges. Okay, very few and more. Most of |
|
|
95:39 | in this range. And then basically grants. That's enough. Look at |
|
|
95:46 | . That's horrible. Um sedimentary. , most of. Alright. Um |
|
|
95:58 | this is he has decent charts in book assault acceptability. Uh Right. |
|
|
96:07 | This is so the conversion from I. One S. I. |
|
|
96:13 | way S. I. Is I know what university you have to look |
|
|
96:20 | S. I. Conversion or. , I gotta look that up because |
|
|
96:31 | that's weird. Alright. So but a relative thing. Right? So |
|
|
96:39 | is in this range grants are in range. Perhaps there's no sandstone. |
|
|
96:45 | this chart doesn't have no red circle . Way. Really tiny. |
|
|
96:56 | Yeah. Alright. This little This is from a from a thesis |
|
|
97:06 | a student here and the student modeled gulf of Mexico. You have these |
|
|
97:13 | anomalies. And the students said well can line up these features with |
|
|
97:18 | This is magnetic ated. So the goes from 1 to 43 2 or |
|
|
97:23 | 22. They said this must be ancient bridge is supposed to be a |
|
|
97:28 | that formed when the basin opened So these are enormous amounts hundreds of |
|
|
97:39 | . When I saw this, I her I said those analogies cannot be |
|
|
97:44 | by starship because they're too big. must be produced by composition ship. |
|
|
97:52 | don't like that. They published us . But if I model this with |
|
|
97:57 | constant magnetic 7,000,003,000, which is kind high for granted This structure has relief |
|
|
98:05 | going from almost zero 2, That's not physical. There are no |
|
|
98:16 | not. So the thing is is big and when we get into |
|
|
98:24 | I have a I have one slide I say to memorize and that will |
|
|
98:30 | relationship wavelengths and amplitudes and how you think about this. But that will |
|
|
98:35 | that will be anyways. Uh If tomorrow, maybe it'll be next |
|
|
98:40 | But anyways this is a pitfall and related to rock properties. When you're |
|
|
98:48 | and big, it's going from minus 32. That's that's five. I |
|
|
98:55 | it's 303 100. Uh Anyway, a pitfall. All right. Now |
|
|
99:03 | a thing we call it a ratio that's the ratio of remnant mechanization to |
|
|
99:10 | mechanization. So the bigger the values the stronger the remnants. Pretty |
|
|
99:15 | Um So this is carmichael. This collin burger ratios for here's basalt. |
|
|
99:25 | kinds of assaults ratios ranged from 15 over 100 82 57. So, |
|
|
99:33 | burger ratio. Um uh Whatever. to write that would be 2-1, |
|
|
99:43 | it? That would be That would two times. That would be one |
|
|
99:48 | remnants. Two parts who two one part induced. That's a |
|
|
99:54 | So anything over I would say anything a half is important. Right? |
|
|
100:04 | over a half the support that we to. That would be a third |
|
|
100:07 | the remnants. So Grant Sedimentary rocks than .1 because they don't quite often |
|
|
100:16 | don't have, you know century. . If if there all the church |
|
|
100:22 | bases on around around this around the . You know those they're all in |
|
|
100:27 | pretty much cost to an inducing Okay. Um graph of metamorphic and |
|
|
100:36 | rocks. So here's Heinz again one these remnant dominance and induction dominant granted |
|
|
100:47 | saying their introduction. I don't believe uh Simon, I believe this, |
|
|
100:52 | I think why is that? I . Yeah. Okay okay uh |
|
|
101:05 | So here's magnificent ability. Okay so are different, well is like a |
|
|
101:17 | print effect. So these are these done. These are all mantle |
|
|
101:23 | Okay, intensity. And then the . Oh yeah of automatic rocks and |
|
|
101:31 | rocks and metamorphic. So automatics are mental rocks. Okay so um the |
|
|
101:42 | example is um of Connie's murder So this is a study. They |
|
|
101:49 | some R. O. V. . So they had a they had |
|
|
101:53 | deep a deep source of instrument I . It just motored around the ocean |
|
|
102:00 | here and they took some samples and calculated races of 1 100 - |
|
|
102:09 | That's really hot. And this is , this is in the Okinawa trough |
|
|
102:15 | . So Japan is there Taiwan china . So let me I think I |
|
|
102:23 | some notes on this. Yeah. the equivalent source inversion vision model statistical |
|
|
102:34 | . What's the result here? So they inverted these data for |
|
|
102:44 | So you just have a layer and just they have the total fields. |
|
|
102:49 | have the data to calculate the magnetic from the field. So here here's |
|
|
102:57 | inversion solution. This is in uh in susceptibility in F m. I |
|
|
103:06 | the conversion from that 1256. So m 1256. Now it does. |
|
|
103:14 | this ranges from -1202 plus Uh 1500. My procedures. So not |
|
|
103:29 | highly. Um Then this one is annihilator and that that's just a function |
|
|
103:37 | makes this all positive. So this their final magnetism organization. They want |
|
|
103:42 | have all positive values for whatever. don't think it's really important. But |
|
|
103:48 | , so this is the shape of magnetization of the rocks. And they |
|
|
103:54 | the I guess that they used to they used to call just supposed to |
|
|
103:58 | a confederation. Rocks indicate high colonics . So the summary for density and |
|
|
104:11 | for density rock samples from rock logs, conversion from philosophy and estimated |
|
|
104:17 | compassion lots of different ways. Megan basically rock samples and I think they |
|
|
104:23 | susceptibilities tool that they can put down . Okay, for density sedimentary rock |
|
|
104:29 | range from 1.9 and 2.7 salt 2.6 higher. And of course you have |
|
|
104:36 | cross over that 1200 m crystalline That means that is 2.7 you know |
|
|
104:44 | in the upper upper continental crust, upper crust. And so for magnetic |
|
|
104:55 | . Some of the rocks are essentially magnetic, effectively not magnetic one. |
|
|
105:00 | to christmas rocks, hundreds, 200 units. Amazing assault gathers thousands of |
|
|
105:15 | run the magazine several types and contributions very specific. So that's the summary |
|
|
105:25 | density and magnetization. That's a good to know. And and you |
|
|
105:31 | I don't know, I've gone so . How long is this supposed to |
|
|
105:34 | to? What should I do more ? Well, it is a lot |
|
|
105:53 | because you know, I don't have I don't have people interrupting me and |
|
|
105:56 | not okay, actually have a question you out of curiosity because I remember |
|
|
106:04 | when I took a class with doctors he was talking about whether or not |
|
|
106:11 | maybe entering like a polar reversal. like what are you, what are |
|
|
106:16 | thoughts on that? That's the timescale reversal. So what's done? I |
|
|
106:34 | , you know, the long normal that. So between 121 roughly? |
|
|
106:43 | for 80 million years ago, there no reverse. They call it the |
|
|
106:50 | things and during and then between Like 21 60 that is that Jurassic |
|
|
107:08 | There is what's called, there's there's cretaceous negative class. I just told |
|
|
107:13 | about those from 81 to 1. there's also something called the Jurassic that |
|
|
107:18 | something but that wasn't because there were funeral versus that's because there were just |
|
|
107:25 | few reversals were very fast and the strength is very weak for that. |
|
|
107:35 | , you know, it is you know, who knows? But |
|
|
107:40 | mean, it's just speculation. I not something that I think a |
|
|
107:46 | So maybe just some, some literature that. I have a friend, |
|
|
107:52 | of my colleagues he worries about, he's looked into this, he's |
|
|
107:59 | he likes to talk about, but not something like not good. So |
|
|
108:08 | all right. So, um, , any more questions, why don't |
|
|
108:13 | flip through the slides and you see we can stop and talk about it |
|
|
108:17 | that way I won't feel like I'm . So no questions on, |
|
|
108:21 | so wait a second. So, . So it's next saturday interpretation rolls |
|
|
108:31 | film, there's a single slide out that will right, right. Say |
|
|
108:38 | because whenever, once you memorize that for the rest of your life, |
|
|
108:43 | you know that information, you'll be to look at any grab and say |
|
|
108:49 | , tell us about. So, . So this is where I |
|
|
108:56 | this is the stuff that I teach dr is these these three lectures |
|
|
109:02 | I split it up in the but, but yeah, um, |
|
|
109:08 | , I have a question about it . So is it a four |
|
|
109:13 | So I don't think so. I I'll just write, you just write |
|
|
109:18 | exam to you just taking it at . So um I just said it |
|
|
109:24 | you and you just you know to that that even you know and I |
|
|
109:30 | the same thing here and then if we get that and I hope that |
|
|
109:36 | organized stuff. But if this I don't know this week, I'll |
|
|
109:42 | you know. But if this happens I can then I will, you |
|
|
109:48 | , we'll do the exercise together. will do the you'll see the |
|
|
109:53 | Okay? So then you just have go to work through and through the |
|
|
109:55 | . And I want I mean the I work because I'm not so much |
|
|
110:01 | want you to answer. But what more concerned is that you understand if |
|
|
110:05 | get a feel for the kind of and magnetic contrast produce different anomalies. |
|
|
110:12 | what I think you did the right? Did you like it? |
|
|
110:17 | know very well. And I think just it's just designed to fit with |
|
|
110:25 | data. Right? See that's one . Did you get a good grade |
|
|
110:30 | it? Yeah. You got you the model. Perfect. Okay. |
|
|
110:37 | right. I mean, but some don't some people like they tend to |
|
|
110:44 | take this personally. But, my , my opinion, people that have |
|
|
110:48 | a geologic background do better in my then people would just straight up |
|
|
110:55 | you'll be fine. You gotta get here. You have you have a |
|
|
110:59 | challenge. But a lot of they have an undergraduate geophysics and they've |
|
|
111:04 | no job. Some universities do it way and there they struggle because my |
|
|
111:12 | really you have to understand something about . One more question about. So |
|
|
111:20 | have final exam because according to the dr so we have a final exam |
|
|
111:30 | February 14. So do we still that one? I thought it |
|
|
111:38 | What's 10? The 10th? It's 10th. It's Wednesday the 10th. |
|
|
111:44 | tenses friday so. Oh right right . Um Yeah Final 6-15 on the |
|
|
112:07 | . Yeah. Yeah. Oh I'll it, I'll fix the schedule. |
|
|
112:14 | god. Um Yeah, I don't that's frank, that's frank. |
|
|
112:37 | cause our last class was supposed to Friday and then I take the final |
|
|
112:42 | , I mean I could just take final um Yeah, I don't know |
|
|
113:00 | to do, but So there has be something happening on the on the |
|
|
113:07 | . Okay, so we can actually the schedule then? Yeah, Except |
|
|
113:15 | . Yeah, I know this is , but the ones in the |
|
|
113:19 | Yeah. So I could. All , Okay. Alright. Anything else |
|
|
113:24 | this thing? What else did Alright, so alright, so I |
|
|
113:33 | through this history blah blah yada yada . And then uh this is a |
|
|
113:39 | is a little, I mean I need to rework this slide because I |
|
|
113:44 | potential enforce potential enforce and um I that's okay But what's important is uh |
|
|
113:54 | know, is really these boxes on slide. I think I think maybe |
|
|
113:59 | need to do that slide over and of course this is this is from |
|
|
114:04 | rick's book and uh I think that's . Can we go over these slides |
|
|
114:11 | um starting here. Okay. yeah, yeah. Here we |
|
|
114:29 | Let's start here. I think it's to start because you're talking about the |
|
|
114:34 | is a magnet, right? So have to north's different from magnetic, |
|
|
114:38 | know that from your field, And the field at the polls. |
|
|
114:44 | polls is burning and the field of magnetic equator is horizontal everywhere else It |
|
|
114:53 | . So it produces a symmetric high , symmetric low here. Then it's |
|
|
114:58 | combine those two shapes everywhere in Yeah, that's where you have the |
|
|
115:04 | between here and here. Right. then the field strength inclination declination. |
|
|
115:15 | right. So at the pole again high. Either pull north or south |
|
|
115:22 | think equator south to north or north south because it's symmetric. But is |
|
|
115:27 | going south and north oriented in a south direction. It's going to produce |
|
|
115:32 | symmetric low at the magnetic equator. in the northern hemisphere, This is |
|
|
115:42 | because you have an anomaly high low . And the source is directly beneath |
|
|
115:49 | . The maximum gradient. Right? you know, it's in the northern |
|
|
115:55 | because the high is south of the loads in the north. Right? |
|
|
116:07 | think about it this way that high you go south in the northern answer |
|
|
116:13 | you go south, this low has migrate to be over the that's what's |
|
|
116:21 | . This shape is changing such that actually like a face face. And |
|
|
116:29 | in the southern hemisphere in the high north of the source. You can |
|
|
116:34 | tell what happens for your in once understand it. So in the three |
|
|
116:40 | . This is just showing that in D. So if you take a |
|
|
116:43 | would be like symmetric high the cube the is the source and it produces |
|
|
116:49 | symmetric high pole northern hemisphere and the is always the same such a |
|
|
116:59 | But then as you go south from north, the high everything starts moving |
|
|
117:04 | with the direction, so now you're degrees inclination C. So this high |
|
|
117:10 | shifted down to here and there's a developing on this northern flag, |
|
|
117:15 | You go further, that high starts lose, right? See this is |
|
|
117:20 | amplitude and this high is losing it that amplitude has been Consume this |
|
|
117:27 | right? You know, first off 30°. Now you're losing a lot more |
|
|
117:33 | to the high but your on the and then if you keep going |
|
|
117:38 | you end up with just a see how that it's like it's like |
|
|
117:44 | law was consuming farming and getting bigger bigger. And then of course Southern |
|
|
117:51 | the same thing. Just the other instead of as you go, sounds |
|
|
117:55 | you go north, col 60° The saluting amplitude, lowest gaining |
|
|
118:03 | 30°, the lowest gaining and losing And the high, the lowest getting |
|
|
118:10 | to end up back here. That sense. Visualize that. So this |
|
|
118:19 | is just interesting. The stuff on . Did I pass anything that was |
|
|
118:23 | ? No, no, no, like this little study. But uh |
|
|
118:32 | else did they go over? Uh ? I think this stuff is pretty |
|
|
118:38 | . It's just I just wanted to you that there are a lot of |
|
|
118:42 | values. Um you know, you , people measure these rocks and a |
|
|
118:49 | of different uh samples values to I went too fast. I gotta |
|
|
118:59 | slower. It's not understandable question about . So why don't you just use |
|
|
119:08 | low pass filter too? You mean block out these things? Because you |
|
|
119:21 | to first you have to have sharp , right? Because you want to |
|
|
119:25 | it. But if I blow it would be. And anyways, |
|
|
119:35 | mean, I don't really work with don't in this kind of stuff, |
|
|
119:40 | definitely someone will send you a file LS file and then we'll have robi |
|
|
119:45 | in it and then you can plot . Typically what I do is I |
|
|
119:49 | do a scatter plot of those and just block them out like this. |
|
|
119:54 | just live on so I don't I don't have an example of |
|
|
120:03 | No I don't I've used sonic check shots and velocity conversions. And |
|
|
120:11 | used uh three I'll send you the spreadsheet and I've. Yeah but yeah |
|
|
120:28 | used this one's not just I use one most of the time and then |
|
|
120:33 | I use this a lot. This of relationship that's just informational. That's |
|
|
120:39 | just whining. Um It's an interesting . I mean it's too calm. |
|
|
120:44 | think your models to come. I you can make anything up if you |
|
|
120:47 | . Right? But I mean they have data to support small. You |
|
|
120:51 | have it. It's just weird. then we talk about modernization and then |
|
|
120:57 | types of that promise again a lot different sources. Um Then I think |
|
|
121:13 | showed you this pitfall and Collins were . Uh And then the school |
|
|
121:21 | It's kind of hard to understand. Yeah and sovereign I guess. |
|
|
121:32 | I have to work on. I know if I gotta add material. |
|
|
121:36 | need to add material or just go explain it or something. What's the |
|
|
121:48 | left so far. Just like a and |
|