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00:01 | This is, this is one aspect a little bit complicated, but it's |
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00:09 | of good brain exercise. So I'm gonna dwell on it too much. |
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00:13 | it's one of the steps in BS processing and, and also in a |
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00:17 | of other uh ocean bottom seismometers and . And there are a lot of |
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00:23 | areas that, that use this And the idea is that again, |
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00:32 | we're running the V S P, particular, we've got all these receivers |
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00:36 | the well, and typically they're on wire line and the wire line tool |
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00:42 | rotates a little bit as it's coming the well. So you can imagine |
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00:48 | uh there might be calipers but there not be. And so we don't |
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00:52 | know the orientation of the tool. know, we know the well |
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00:57 | And so we know that more or the top part is vertical. So |
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01:00 | know what the vertical channel is in GEO phone, but the horizontal |
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01:04 | I don't really know which way they're . So the way that we can |
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01:11 | do that is to imagine that I've say two positions, the horizontal channels |
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01:18 | sensing at one orientation here at a orientation here. And I, I |
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01:23 | really know the way the instruments So I have to figure that |
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01:29 | So um if we think of the coming down at some angle and it |
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01:38 | the tool and it just moves the and that tool movement gives us the |
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01:46 | . It's like if I had a a wave coming down, I hit |
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01:49 | GEO phone, it oscillates it up down. That outputs a little |
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01:54 | Likewise, if I, if the comes in sideways and hits the |
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01:58 | it oscillates it back and forth. the two sensors measure what is on |
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02:05 | sensor orientation, right? So I've a three component tool and the wave |
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02:12 | coming in at some angle. And these sensors do is say, |
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02:16 | when, when you move on my , I output if you move perpendicular |
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02:20 | axis axis, I don't do anything I'm on a spring and that's, |
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02:24 | the only emotion my spring can Likewise, the horizontal guys say if |
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02:29 | move me up and down, I feel anything that's not moving my spring |
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02:33 | all. So these three sensors basically output the amount of motion that's in |
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02:42 | orientation. So and this, this actually way easier than it seems, |
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02:54 | it's kind of like dancing salsa or when you know how to dance |
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02:59 | which you might, it's really easy you don't know how to dance |
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03:05 | it's really hard. So we're just at the X and Y channels |
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03:15 | So the horizontal one and horizontal So we've, I've got the vertical |
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03:19 | . I'm not looking at that right , I'm just looking at the horizontal |
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03:22 | . And if a wave comes down hits that, then the Y channel |
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03:28 | measures how much motion there is on channel, the X channel or just |
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03:35 | how much motion is on its So if I plot those together and |
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03:41 | give the output at every point which really just a vector that has an |
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03:49 | and A Y coordinate and that X Y coordinate is a measure of the |
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03:56 | . And if I plot this in , just how does the vector move |
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04:02 | you can see here, then it of moves back and forth like |
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04:08 | So that's just what the motion is in the horizontal plane. And in |
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04:15 | , this motion is actually coming about degrees to the GEO phone because it's |
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04:21 | more or less equal amounts on the and the Y channel. So once |
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04:28 | , if this is the full if I just output what's on the |
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04:32 | channel, then the X channel is gonna oscillate back and forth like |
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04:35 | If I just output what's on the channel, it'll oscillate back and forth |
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04:39 | this. That's exactly what we see here. So normally we think this |
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04:46 | and here is what is the But I can also take the record |
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04:51 | plot what the motion is. So we take the two components and plot |
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05:02 | together as a function of time, might remember way back from math, |
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05:08 | are just such parametric realizations or it's a ho gram. So this is |
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05:17 | a hologram. When I plot the of the vector has broken down into |
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05:23 | and Y, I just plot the of that vector and, and where |
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05:27 | moving. And then that in time called a ho gram. So also |
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05:50 | if you were um in the physics in the electronics or electrical engineering or |
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06:01 | , You might have two voltages coming a circuit and you might want to |
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06:09 | how do those voltages vary with each . So if I plotted a voltage |
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06:18 | one area against a voltage from another , and I plotted how they vary |
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06:22 | in physics, they call that a figure. And it always reminds me |
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06:31 | when I was an undergrad at we were doing electronics lab and we |
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06:36 | um big cellos and I, I that familiar with the telescopes and we |
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06:44 | talking about Lisa figures. So I to put the probe of the asco |
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06:48 | the wall outlet just to see what of wave form was coming out of |
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06:52 | electrical outlet on the wall Well, did Turns out that the amount of |
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06:59 | that's coming out of your wallet that really high. The silos copes are |
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07:03 | . So it takes the, the right to the ground. So I |
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07:07 | circuited and blew up about a $3,000 . So good, good work. |
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07:14 | , man. Yeah, that that was kind of embarrassing, but |
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07:22 | never done that again. So I and then, uh, actually we |
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07:27 | the telescope. It did it fried a little bit, but it was |
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07:30 | . We replaced some of the uh some little circuit breakers and stuff, |
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07:35 | it was uh it was pretty dramatic the time. Yeah. OK. |
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07:41 | that's Lisa you figures. So what have to do in the BS P |
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07:48 | because the tool is rotating up well, we want to get it |
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07:52 | make it look like I had one G phone pointing at the so at |
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07:58 | source. And so I can effectively project the data onto this maximum |
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08:08 | So again, the recordings are just X and Y. If I plot |
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08:13 | photograph, it looks like this. I can also say let's take the |
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08:19 | of that hologram and project the X and the Y motion onto this new |
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08:28 | . So effectively, if I had the data with an X primed axis |
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08:33 | and a Y primed axis here, would have almost all the data on |
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08:37 | X axis. So this new axis just projecting the data from X and |
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08:44 | onto this AX primed axis. That's a rotation. And so we get |
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08:50 | and when I rotate to X prime Y prime, then the data puts |
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08:55 | all the energy on the X prime and I can throw the Y prime |
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09:01 | . So I've reduced the data from channels to two channels. And now |
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09:07 | makes it look like it was all in one plane, the X Z |
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09:13 | , the X prime Z plane. so now all the data just looks |
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09:18 | . So here's the uh in this , here's the X channel and the |
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09:22 | channel, here's the first breaking energy down and it looks all kind of |
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09:29 | because the instrument is rotating and it's with the amount of data on the |
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09:34 | and Y s. So I just my ho gram find the direction of |
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09:39 | arrival and then rotate these two channels put most of the arrival on this |
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09:51 | channel or the X prime channel. you can see now there's almost nothing |
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09:55 | the X wave of the P wave the orthogonal channel or the Y prime |
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10:03 | . So now I can just now has other stuff on it, she |
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10:07 | on it. But uh as far the P wave goes, now, |
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10:10 | got a much more continuous X primed channel. And now we can |
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10:21 | continue on and fun with figures. got the vertical channel because this was |
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10:28 | a slightly offset V S P. I've got most energy on the vertical |
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10:36 | and I've got a little bit of on the oriented horizontal ti now incidentally |
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10:46 | that, if my waves are coming like this, most of the P |
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10:51 | energy is on the vertical channel, which energy is on the horizontal |
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11:06 | The energy on the horizontal, would , the P wave is on |
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11:10 | So this would be the S Yeah. So now I've got a |
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11:13 | S wave. So I've on on the vertical channel, I've got |
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11:19 | of the P wave. Mhm But got the horizontal channel there too. |
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11:27 | of course, in a vertically propagating , the S wave motion is largely |
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11:33 | . And so sure enough, I've a little P wave energy on the |
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11:38 | . But now I've got this big event, the downgoing shear wave on |
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11:43 | horizontal channel. So I could pick P wave velocity and the shear wave |
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11:54 | . Now, I don't know whether could see it, but this says |
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11:56 | p waves arriving at .2 seconds at ft. So what's the P wave |
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12:09 | Down to 1655 ft? Um It be so feet per second, it |
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12:18 | be hm 1655 divided by 0.2. 82, ft /s. Yeah. |
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12:34 | that's good. And then you can that later the shear wave is coming |
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12:40 | nice and coherently and what's its So I've got the shear wave coming |
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12:50 | here. Mhm. So that's gonna 6255 x 0.4. So about half |
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13:02 | that. So 41, Yeah. is that kind of standard? So |
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13:11 | a V P over V S of or shear wave velocity is half the |
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13:16 | wave velocity. Mhm Yeah, that's the game. So we, we |
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13:23 | that the shear wave velocity is somewhere half the P wave velocity because it's |
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13:27 | secondary arrival. So, so that makes that all makes sense good. |
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13:43 | . I just want to go through that's called ho gram analysis. That's |
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13:46 | early step of most of the DS processing is just to make the data |
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13:51 | consistent. And we go really from , a three channel without orientation on |
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13:58 | horizontals to a two channel where the channel is rotated to be consistent and |
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14:09 | at the source. OK. Uh covered most of this stuff last |
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14:26 | Um Good. OK. Um let's just begin to look at it |
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14:45 | a little exercise and I'll give you few minutes for this exercise. I |
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14:54 | I think I think I posted this I better check. Mhm If I |
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15:15 | , I will. Yeah, let uh let me just post this I |
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15:37 | that's the best way to do Um. Ok. Um, this |
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16:24 | just one to roll through fairly But I'll, um, these are |
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16:32 | older data but this is just to practice in one of the, |
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16:38 | using the V S P for a interpretation. So there are a few |
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16:47 | , um, products here and you'll able to rotate these stuff, but |
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16:59 | , here's looking sideways and to see I can rotate this. Oh, |
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17:14 | on my home computer. So um my home license with Adobe is |
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17:21 | but here is, here's some circus and it's on its side right now |
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17:31 | it's split at the well location. there's a well drilled in here and |
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17:40 | we've got our surface seismic. There go. Ok. And so we |
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17:55 | see that um the surface seismic is . It's going from 500 milliseconds 5000.5 |
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18:02 | down to 1.5 seconds. And as look down, we can see some |
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18:12 | highlights here. This is a little , a reflector. We've got quite |
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18:17 | strong reflector just above B and then got a very strong reflector at |
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18:27 | And so our job and not knowing about this area is to interpret these |
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18:33 | . Now, what we do have uh we picked the first brakes of |
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18:39 | V S P. So I've got the first brakes of the, the |
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18:44 | S P picked and I've got a wave velocity and a shear wave velocity |
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18:48 | of that. Then our trustee geologist given us uh an interpretation. So |
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18:56 | this Pasco limestone that's just under 900 . And then there's the lower bath |
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19:01 | is a sandstone and then there's the , which is a, a carbonate |
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19:06 | limestone, Beaver Hill Lake, And so that's um just a little |
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19:14 | of a really a Strat graphic column a function of death. Then we |
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19:24 | some logs and we looked at these little bit before We've got our gamma |
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19:28 | logs going from 600 m down to m. Were you able to pick |
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19:34 | up there? Ok. Good. you can see we talked about the |
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19:39 | ray before that it's fairly high gam the near surface. And then we |
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19:43 | to a clean area and then we a dirty area and then it's cleanish |
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19:47 | it gets kind of funky at the . P wave slowness is in microseconds |
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19:53 | meter here. So it's fairly slow the near surface. Then we get |
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19:59 | and then slower, fast, it , fast. So those are, |
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20:04 | only got two logs here, but in depth. And then our BS |
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20:10 | we've got P wave energy going down is the depth scale. And we |
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20:20 | see that there's a change in the it goes from slow to fast, |
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20:25 | gives us some reflections. So that's P wave RBS P, we can |
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20:35 | on just the vertical channel here, wave down energy coming back. And |
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20:44 | we got the V S P processed two way time. So here is |
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20:56 | 600 m down 1800 m. So see uh our reflections coming back. |
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21:10 | now this V S P is in way time which we could stack and |
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21:18 | we have stacked that into the, got a synthetic size of ground and |
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21:23 | um a corridor stack or a P vertically extracted trace V S P, |
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21:28 | trace. And then we had an V S P. So this is |
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21:32 | little bit of a section. And again, we can see nice events |
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21:36 | the offset V S P, the offset V S P and the synthetic |
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21:41 | grams. We see fairly nice ties and don't worry about this. This |
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21:45 | getting into the converted wave stop. we don't have to worry about |
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21:51 | And the job is to create an plot. So by the, by |
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21:58 | L plot, you, you're, probably gonna have to snip and cut |
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22:03 | paste a little bit here if you do that. So the job is |
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22:08 | get the these well logs 600 to m, just put that on this |
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22:26 | . So the well logs right down . Now we've got a mapping from |
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22:32 | well log to the V S P but these guys in beside the V |
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22:43 | P in time beside this guy and snip out some of the surface seismic |
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22:54 | is at the same times and correlate surface seismic to the V S |
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23:02 | So you really are just going to putting in four of these one, |
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23:12 | This guy 600 to 1800 m On top of this guy 618 cm and |
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23:22 | that beside this guy and then put beside the surface size. So that's |
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23:32 | the L plot. And then the is on the surface seismic. There |
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23:41 | three horizons identified A B and C the job is to correlate those across |
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23:51 | V S P. The synthetics. you're gonna see that the surface size |
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24:00 | it is gonna correlate to some of events. And then we take that |
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24:04 | and we find out what depth it from and we find out what depth |
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24:08 | came from. We look at the and find out what geology it came |
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24:14 | . So, um why don't you quickly assembling that? And let's, |
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24:23 | take a break and assemble it. you, do you see how to |
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24:27 | that, Stephanie? I think Right. Let's take just about, |
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24:33 | give you just about 20 or 25 to try to put that together. |
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24:37 | gonna jump in, we've got a meeting right now too. So I'm |
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24:40 | jump into our faculty meeting and then be back in just about 20 |
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24:44 | See how, see how you OK. OK. Beautiful. Um |
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24:49 | gonna stop right now. See if can take a little break, see |
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24:54 | you can assemble this and then we'll we'll chat about it. OK. |
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24:59 | you in about 20 minutes. So this is the, can you |
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25:08 | that now, Stephanie? So this the uh the assembling and you can |
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25:15 | it's an L plot just because it's the shape of an L and with |
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25:19 | with your uh with that little the exercise and I'll leave, I'll |
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25:26 | this with you too. This is answer. But I want you to |
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25:29 | it and You can see that the this axis, the the depths the |
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25:37 | goes from 600 m or so to m. So that's in depth. |
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25:45 | course, the logs are, are in depth going the other way. |
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25:49 | it's good to be able to um these in any orientation. Then these |
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26:00 | and depth are the same depth as V S P. We could imagine |
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26:03 | the, the borehole is here and This log now, in principle, |
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26:09 | , the energy that has been shot zero asset is coming down into the |
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26:18 | , but it's been muted here. we've just muted off that downgoing |
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26:26 | And then as we talked about it we've shifted the upcoming energy to two-way |
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26:32 | . So we, we understand that the fact that we had energy |
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26:36 | down into the earth, it's hitting these interfaces and sending signals back to |
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26:41 | surface. Now, from the sonic density logs, we can create a |
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26:47 | seism gram in time. And then just stacked all this V S P |
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26:53 | across and created a A V S extracted trace or just a stack |
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27:00 | Then we've got an offset image that's little piece of offset seismic. And |
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27:06 | I've taken a little chunk of surface I could put it in here. |
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27:16 | with, with your exercise, you've uh you've got these pieces, I'm |
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27:21 | gonna worry about the converted wave the P DS but the P wave |
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27:25 | , the surface se make the, synthetic this guy and then getting that |
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27:32 | depth. So let's uh let's take example. You can, you can |
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27:46 | how some of this is done. then you've got another piece of paper |
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27:51 | is, it's not of the same , but it's also given the uh |
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27:54 | name of the units as a function depth, that little Strat graphic |
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28:02 | Mhm I was kind of when you on, I had just finished um |
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28:07 | connecting the dots to that. So here's the answer here. But |
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28:13 | could squeeze that other um the Strat column with the velocities. You could |
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28:19 | that and put that here and that just give you the, the names |
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28:24 | these horizons and um rock tapes. for example, somewhere this is, |
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28:32 | can see this change right here. . Mhm. So maybe just describe |
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28:40 | me what's happening as we go from to here. Well, we go |
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28:48 | a, a high gamma to we're decreasing in gamma. And then |
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28:55 | we are kidding faster to er, getting slow to fast on our P |
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29:08 | . Yeah. So our interpretation here that we've got a, a pretty |
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29:14 | shallower section And then uh this is m. So that's 600, that's |
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29:22 | 1200 m deep there. So that's around 1000 m right there. so |
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29:31 | a 1000 m depth, we go this kind of clay rich dirty stuff |
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29:41 | has a high slowness or it's not fast and then we hit an |
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29:54 | And, and everything, everything So at about 1000 m, we |
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29:58 | from this cruddy stuff to this very , more regular stuff. And when |
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30:08 | see something that's clean and fast like , like really fast. And this |
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30:12 | um well, we have to divide up but that's was that 500. |
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30:17 | there's 300. So this is like microseconds per meter. So there's a |
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30:27 | exercise for you. What's the you said 100 microseconds per meter. |
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30:36 | It's about 100 and 80 microseconds per . Ok. So that would |
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30:57 | Mhm. Mhm. So about 5555 per second. Yeah, so that's |
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31:23 | . So once again is that assault yeah could be four because four the |
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31:32 | one was at 4000. So we salt's pretty uniform no matter what the |
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31:43 | , it's always very uh low density it's always very moderate velocity, it's |
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31:52 | around 4500 m per second plus or a little bit. Ok. So |
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31:57 | did we say the velocity was 50 555. So that's too fast |
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32:03 | Saul. How about sandstone? that's like around 20. No, |
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32:14 | was in the two. Yeah, 3000 m per second. Too fast |
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32:19 | sandstone. So, could it be ? Yeah. Yeah. So this |
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32:27 | is largely a carbonate section. If go back to your Strat graphic |
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32:31 | you'll see that this is largely So as you just calculated, which |
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32:35 | good, that's, that's pretty It's 5500 m per second, which |
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32:39 | pretty fast. And so mostly what that fast is some kind of |
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32:56 | you know, how, how far is it to your place and from |
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33:01 | to the woodlands to your place, mi. Yeah, give or |
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33:11 | So that's, that's around 65 1.6. So that's somewhere around 65 |
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33:22 | away and This rock is going 5.5 . So it takes Something like |
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33:35 | 12 seconds, 12 seconds. If were carbonate from me to you, |
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33:41 | would take seismic only 12 seconds to there. So you can really see |
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33:49 | fast that rock is. It's really competent. Very fast. |
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33:54 | That's, wow. Yeah. um, this is, this is |
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34:00 | of your, um, uh, guide to the answer. But now |
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34:04 | we look down here, so we about this that we've got this big |
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34:08 | happening from mushy near surface stuff to carbonate. There's no carbon here. |
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34:16 | it turns out is the top of Mississippian. So we're going from a |
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34:25 | section into a carbonate section. So is a big impedance contrast. So |
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34:33 | do I expect in the seismic A reflection? Yeah, big |
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34:39 | So I'm coming down here in my V S P is in |
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34:42 | I come around to see what happens the energy hits that depth. And |
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34:46 | happens reflection mega reflection. So I'm at the V S P, the |
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34:53 | S P says you've got energy going to the surface big time. And |
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34:57 | synthetic seism gram says there's something Now, do you, would you |
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35:03 | the synthetic seo gram to tell us same thing? Yes. Yeah, |
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35:09 | here's the sonic log. And when look at the change in the sonic |
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35:14 | , there's a big time change So that's gonna give me a big |
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35:17 | reflection in the synthetic seism gram. the synthetic sees it, our seismic |
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35:24 | it and then we go to the seismic stuff and we see it. |
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35:35 | , this is going from uh low to a high velocity. And you |
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35:42 | see that this signature corresponds to a trough peak. Hm It this was |
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35:57 | is not S E G normal So going deeper, we've got an |
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36:05 | increase or decrease. So going across interface going deeper does impedance increase or |
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36:18 | . It was that's a negative, would decrease 50 50 chance, |
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36:29 | Um No, because is that it it would be increasing. Why is |
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36:35 | increasing? Because it's getting faster? , we're going from a low velocity |
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36:42 | high velocity generally the density is going follow. So the delta V the |
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36:48 | in velocity is positive here going So there's gonna be a positive reflection |
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37:00 | . Now getting into a few more the details, they have plotted all |
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37:06 | this vass Anchorage, but that's the that slummer used to plot all this |
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37:14 | . So a positive impedance contrast here plotted as a negative spike. Getting |
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37:27 | some of the details, this gets to acquisition. There was a reason |
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37:30 | could say, well, why, did you bone heads do that? |
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37:33 | doesn't make good interpretive sense. But the seismic world originally, it |
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37:39 | And the original was because when we a GEO phone on the surface to |
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37:45 | out how it was wired. People a tap test, you tap the |
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37:52 | phone on the top and it gave positive output. So that was just |
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38:00 | make sure that was a check in field that checked to make sure that |
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38:04 | was wired properly and then nobody plugged their data on or anything was |
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38:09 | So the tap test was the gold tap in the top of the GEO |
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38:13 | . It should give you a positive on the instruments. So that being |
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38:18 | right? Mhm OK. So if have a an explosion explosion, first |
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38:27 | down and I'm going down and the coefficient is to say in this |
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38:36 | um negative, then first motion would down. In this case though the |
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38:45 | changes to the positive, we just that the velocity is increasing. So |
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38:49 | means that the first motion is the uh the reflection coefficient is positive |
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38:54 | V is positive. So the reflection is positive. So it sends the |
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38:58 | back up as a compression. So sending the energy back up. When |
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39:04 | hits the GEO phone, it pushes GEO phone up. So what should |
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39:08 | GEO phone read? It should be negative. That's right. So the |
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39:17 | reflection coefficient from a positive impedance contrast the field would read? Mhm So |
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39:29 | is all plotted in field polarity. . If that makes sense, this |
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39:37 | now getting into a little bit more the details, um we, we've |
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39:40 | to worry about uh the polarity and shape and the, and the beauty |
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39:45 | the V S P is that now know unambiguously the polarity of this |
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39:54 | So again, with the surface I don't really know whether this is |
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39:59 | impedance increase, decrease, whether there three layers there. I don't know |
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40:03 | going on. But with the V P I can see there's a clean |
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40:08 | right there it comes down, there's signature of that interface and it's a |
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40:13 | trough peak because I have a band instrument, I don't have a spike |
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40:18 | into the earth. I have this shape that I'm measuring. So this |
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40:26 | agrees. So I completely understand that of these data are plotted in field |
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40:34 | good. So if we go down farther, so this was an impedance |
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40:46 | . If I go down here into layer, which is the salt, |
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40:49 | a little layer of salt there. I go from the carbonate into the |
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40:54 | , is that an impedance increase or that be a decrease, it's a |
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41:00 | . So now the decrease corresponds to kind of impedance. So my recorded |
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41:07 | in the surface is a decrease. that correspond to in geology? A |
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41:14 | density, a higher deft well, this case, just a higher |
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41:20 | So OK. Well, I'm I misstated that we're going from a |
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41:25 | impedance, it's getting slower to a impedance is an impedance decrease. |
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41:34 | And there's nothing um sophisticated about An impedance decrease manifests as a peak |
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41:42 | the field. OK. So we that an impedance increase was a |
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41:49 | So a impedance's decrease has to be out as a peak. And you |
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41:56 | see, well, is that a fantasy lie? Well, no, |
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41:59 | it is, we've got an impedance going into the salt from the |
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42:03 | And I see a nice big positive coming off that impedance decrease the top |
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42:10 | the salt because it's relatively a lower and it's a much lower density. |
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42:17 | that much lower density times the lower gives me a much lower impedance coming |
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42:23 | of a high velocity, higher density . So now we understand a little |
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42:33 | more, not just about the timing the events and the type of events |
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42:37 | can actually say about whether the it's impedance increase or decrease corresponding to the |
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42:44 | of the seismic data. So let's another one. We've got this layer |
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43:05 | . You can see we got carbonate . Then something funny is going on |
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43:10 | here. It's dirty. Mhm It's . So could that be another salt |
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43:27 | ? No, no, you're exactly . Why not? Hm I |
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43:34 | according to the mythology law, we've a shale but the um velocity is |
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43:41 | the, it just doesn't make Well, the, yeah, the |
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43:46 | is not so much the velocity, the, it's the gamma rate. |
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43:51 | , gamma, the the velocity of is relatively low. So this, |
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43:56 | seen the velocity down here that So velocity alone this could be |
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44:05 | But the gamma ray says no, is, this is quite dirty. |
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44:10 | so I don't really know what it . All I know is that it's |
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44:15 | and it's dirtier. So it's probably straight from these two lines. |
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44:32 | So, but let's look at this , that's, so that's our interpretation |
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44:35 | I'm going from carbonate here. Mhm what I'm interpreting to be a slower |
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44:44 | Shelley garbagey and it might, might probably not pure shale, but |
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44:51 | it's dirty. So this shay sandy which is characterized by a slower |
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45:02 | So once again, I'm going from velocity to slow velocity. So that's |
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45:06 | impedance decrease. And if I've got decrease, what kind of reflection is |
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45:14 | la it's gonna manifest as a So if I come down here, |
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45:19 | come right down, down, down, down, boom. There |
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45:22 | is. Now, do you believe we're seeing that on the surface seismic |
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45:30 | I go over here, there's this event. Is that event real? |
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45:35 | it a multiple? Is it What's going on? Um Would that |
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45:50 | um a multiple or is it just offset? Because I can kind of |
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45:56 | like that, that the lighter one under like that big dark one. |
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46:02 | . Um, so maybe, what, what did we say |
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46:07 | What's a dark, uh, big correspond to? Oh, that's gonna |
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46:12 | the, um, that's that other that's the trough, the load |
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46:16 | load of high velocity and pence Yeah, that's that one for coming |
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46:25 | here in depth. It's there. . It's bang on the top of |
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46:33 | low velocity layer. Mhm. So is very definitive. I believe |
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46:41 | And what is it? I go and I look at my logs. |
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46:45 | It's the top of that sand which a a low impedance. Now, |
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46:54 | bottom of the sand is going from to high impedes. So how should |
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46:57 | manifest on our seismic? A little ? That should be the the peak |
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47:05 | were just talking about. We went high to low as a peak. |
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47:10 | low, I'm sorry, low to is the. So I come over |
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47:15 | and I look at my seismic, got a peak trough and so how |
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47:18 | I going to interpret that peak trough as a in and secrets? Is |
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47:31 | what you're asking? Well, I that as this layer. OK. |
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47:37 | . Yeah. No. OK. wasn't really sure what you are. |
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47:40 | . And so the the layer has peak and in my field polarity here |
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47:45 | peak corresponds to a negative reflection coefficient is an impedance decrease. So I |
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47:51 | the impedance decrease here. And then going into a trough which in seismic |
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48:00 | to an impedance increase in the log . And so I come down there |
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48:05 | this line and I see when I out of this sand and I, |
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48:08 | hit the bottom, I hit the of the carbonate. That's the impedance |
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48:13 | which in field polarity is a So I see the top and the |
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48:18 | of that sand lay. OK. what this is this is doing arm |
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48:34 | and weightlifting exercises and not. So go out and play sports. So |
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48:43 | we're looking, we're going from the Time Domain here, that signature to |
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48:52 | borehole log domain and that signature. what we're doing is we're just going |
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48:57 | and forth here, but it's exercising brain because I'm going from seismic wiggles |
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49:02 | time to rock properties in depth. that's what this plan is intended to |
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49:11 | because we've got these seismic wiggles in . I don't know what that means |
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49:14 | all. But when I correlated it the, the V S P extracted |
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49:20 | , the synthetic and I look at it evolves and then I go back |
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49:24 | that depth. I can see exactly it means. That peak means that |
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49:39 | decrease. So that's when you assemble , that's what you want to look |
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49:46 | and look at the character as we into depth, we can see the |
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49:50 | character. So we've done a we've looked at a lot of |
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49:53 | So we're beginning to understand what this means. That's the log, the |
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49:58 | jet folding in depth. But as geophysicist, generally, we're looking at |
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50:02 | sections. And so we've got to transforming in our mind from the seismic |
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50:09 | to the log and then from the to the seismic section. And that |
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50:13 | the, that's really the job of interpreter is to be going back and |
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50:17 | like this all the time. You , the geologist is gonna spend his |
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50:22 | her time doing this. Most seismic are gonna do this. The |
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50:27 | the geophysical interpreter is running back and between these two. Mhm Good. |
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50:38 | you've got a bit more of a of, of that. OK. |
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50:56 | , here's another example. So we see that again, we've got logs |
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51:03 | depth here. This is shallow and this case, uh we've got an |
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51:08 | P log and a gamma ray log we can see that our gamma ray |
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51:14 | goes from 0 to 1 50 and S P log goes from zero to |
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51:20 | like minus 50. So if we look at the gamma ray, there's |
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51:31 | of character on here. It's generally up as we go deeper, but |
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51:36 | all pretty chilly, classy garbagey. . The S P shows that we've |
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51:43 | a few areas of big permeability, we can go down into the we've |
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51:51 | here, the product, the impedance . And so the impedance log goes |
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51:56 | low impedance, low density, low to high impedance, high density |
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52:03 | Then we've got our processed BS P then circus seismic and then synthetic and |
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52:11 | an offset. And so we just the same thing. We have to |
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52:15 | to interpret this kind of poor surface , but we can correlate that event |
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52:24 | figure out exactly what geology it corresponds . So that, that's the job |
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52:29 | this plot. It correlates geology and with seismic in time. OK. |
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52:47 | then there's more of the same OK. Well, that's uh that's |
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53:04 | of the V S P stuff um just as one little other example as |
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53:10 | case we can look at. Um was again to hammer home a few |
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53:20 | of these ideas. We imagined that got to say our V S P |
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53:28 | the well in the middle. And we've got a lot of different shots |
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53:32 | we can make a V S P of all those shots. And this |
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53:36 | , this was one of the cases we were involved with. So we |
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53:38 | a well in the middle, then had two offset shots uh in various |
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53:45 | around this guy was shot because the was drilled and it missed the target |
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53:51 | they couldn't get in to shoot a 3d size because it was too expensive |
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53:54 | they had a rig on site. they quickly put a GEO phone in |
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53:59 | well did a bunch of shot points then created the offset V SPS. |
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54:04 | here is the idea. Uh we a well log are zero offset V |
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54:10 | P and then they walk away the V SPS. And now we're gonna |
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54:15 | at the events and interpret them. these horizons And then correlate this is |
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54:25 | of a bad picture, but this an old one and then pick that |
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54:29 | and create a structure on the top that um map. Now, in |
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54:38 | case, we picked an event that interpreted as the base of the |
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54:42 | And we're looking for a high in below it. So in other |
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54:51 | we pick the base of the salt we're looking for a reef sticking up |
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54:55 | the salt. So it was a , the salt got deposited on top |
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55:00 | the reef. But I'm looking for structure on the reef. And sure |
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55:06 | , if you see just in this here there is a high on the |
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55:10 | of the salt and that's the reef looking for. And so with |
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55:15 | they took the well and then deviated well to hit the top of the |
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55:19 | and get the hydrocarbons in the So that's uh the kind of thing |
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55:26 | can do with multiple offset V Hm. And that can be done |
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55:32 | fast. So that's, that's Ok. Well, great. Uh |
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55:43 | , let's continue on for just a of minutes then take a little |
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55:50 | Um We're gonna, we're gonna move uh another geometry. That's another borehole |
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56:20 | . So we've talked about, logs down the, well, we've |
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56:25 | put a seismic shot. We've got seismic log with velocity and reflectivity and |
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56:31 | we walked away the seismic source that us an opportunity to create a |
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56:35 | So we've created a picture. Then done a little bit of interpretation of |
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56:39 | we use that new picture. And we're gonna put shots and receivers in |
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56:44 | well. So now I, now I have two wells and I'm |
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56:48 | gonna have just receivers in the I'm gonna have shots in a |
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56:52 | So that's called the crosswell geometry. before we get to that, here's |
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56:59 | little uh and before you see the , you might see the answer. |
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57:06 | this is just uh I think it to be called Chinese squares or something |
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57:12 | that. I'm sure that's illegal But the um yeah, but the |
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57:19 | idea was that they Are four unknown in this pattern. So there's one |
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57:29 | in each of those squares. So here, number here, number |
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57:33 | number here. And then the sum these two numbers is five. The |
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57:37 | of these two numbers is nine da da. So if you haven't done |
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57:42 | already can you quickly guess. What's number here, here, here, |
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57:47 | . What are the numbers that go here to give these sums? It |
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57:54 | should, when I pull up my , the numbers are right here. |
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57:57 | , no, it took the fun . Yeah, that's ok. |
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58:02 | that, that's because it's so much to guess, you know, I |
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58:05 | we every day. I don't know you do that at all. |
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58:08 | I play word. OK. I, I do we every day |
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58:11 | but it's, it's, it's really . These little puzzles are really |
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58:16 | But um, so there you But we could create some different |
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58:21 | Uh But as you can see, you've got, you've got all |
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58:25 | Yeah, because the PDF smashed them together. Mhm To tell you the |
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58:30 | when I was first working on way, way, way back. |
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58:35 | It had just come out and I trying to figure out everything about tomography |
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58:41 | I was actually giving a talk with lot of people and explaining a little |
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58:47 | about tomography. And I had an like this and I did the case |
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58:52 | I had everybody else do the case everybody gave different answers and I had |
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58:59 | just calculated one of the answers. so when everybody gave me the |
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59:02 | I thought, uh-oh, they're uh-oh there are all these different answers that |
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59:10 | you can see work. So when get into inverse theory, this is |
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59:15 | of a classic problem. And the problem is non uniqueness. So there |
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59:21 | an answer but it's not a unique . So in other words, this |
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59:26 | a, in a sense, this or these measurements are not enough, |
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59:31 | not adequate to give a unique So that's an interesting detail. So |
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59:39 | I'm gonna process this data, say gave this data to a computer to |
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59:45 | , it's probably gonna blow up because going to have multiple answers, then |
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59:52 | not gonna be able to figure that . So you can see that all |
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59:55 | these, all these guys work. if I give it one more observation |
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60:00 | I give it one more equation, can see now which of these does |
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60:07 | have to be A different one Yeah. So all of these were |
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60:17 | with just four equations and four but they weren't the right observations of |
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60:23 | right equations to make it unique. if I add another equation in |
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60:27 | then that selects a unique answer. it exists and it's unique. Um |
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60:37 | where we're going with this is because is effectively the case for the crosswell |
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60:46 | . So we're gonna use this a . But before we get there, |
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60:51 | one other place that we did was work in Belize and we were trying |
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60:59 | do imaging of pyramids. And so took seismic down there and I'm just |
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61:08 | show you where it was in So here's the kind of structure we |
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61:19 | seismic receivers and sources around the structure then we're trying to nondestructive, we |
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61:25 | if there's anything inside this structure. that's, that's the idea. In |
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61:31 | , here's the pyramid that we were on. Here's one of the archaeologists |
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61:35 | were setting up and so we put ring or a belt of geophones around |
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61:41 | pyramid and then we tap and we trying to make a picture of what |
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61:46 | inside of it. So let's go now, that's where we're going. |
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61:51 | here's the math. So you can that if we're taking a shot and |
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62:02 | receiver, this is a slice through pyramid or it could be a slice |
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62:07 | anything that the time to go from shot to the receiver is the sum |
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62:16 | all the transit times through each picture picture element or little square. So |
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62:23 | what we get here. So the transit time from a shot to receiver |
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62:27 | just the sum of all the interval times for each one of those little |
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62:31 | or pixels. Then you can see the travel time through each pixel is |
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62:40 | the distance over the velocity of that . That's the sum of the transit |
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62:46 | , which is just the sum of distance times the slowest. Does that |
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62:55 | sense? All good? So that's we get. And now we could |
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63:05 | that this is just for one shot receiver, but I've got many shots |
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63:09 | receivers. So say for all the shots and receivers, I've got J |
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63:13 | are all around. So each one those is now an equation of a |
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63:18 | travel time from each receiver. So I have a matrix and a couple |
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63:28 | actors. So the vector here T strictly the total travel time from one |
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63:37 | to receiver multiplied by all of its . The second line is just the |
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63:46 | receiver. And so this T is vector of times P is a vector |
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63:53 | slowness and A is the geometry. to make this simple, we're just |
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64:11 | say T is the vector of all different travel times P is the slowness |
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64:16 | all the different um pixels arranged into vector. And A is just the |
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64:23 | the distance through each one of those . So we're expressing it this |
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64:27 | which is easy. And then we how to solve this equation. We |
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64:31 | by a transpose and then I take inverse of a transpose A which is |
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64:39 | that gives me this equation. And is how I solve that matrix |
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64:53 | This is tomography. So what we do is just go in do our |
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65:16 | which takes days trying to avoid scorpions malaria and lances and all kinds of |
|
|
65:25 | . Looking forward to getting out to beach. And uh we do that |
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65:29 | we come back, we pick all first breaks. We know the |
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65:35 | Mhm I just assume straight rays for pixel. So I know this, |
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65:40 | arrange it like that, do the . And that gives me the velocities |
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65:46 | slowness. So that's exactly what we . And here's the resulting picture. |
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66:02 | these are low velocities in blue and high velocities in the red. And |
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66:08 | is just one slice through that ancient . So we thought that maybe we |
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66:14 | start to see some of the internal . And ultimately, we did a |
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66:18 | of these slices and we reconstructed the . And what we're looking for is |
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66:29 | that's an indicator of cavities or tombs burials or riches. Mhm. That's |
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66:37 | we're looking for. Again, these were all built uh over the years |
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66:43 | then they were built upon and then over and then drilled and then built |
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66:48 | da da da da. So there's lot of structure inside here, but |
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66:52 | were trying to get the uh internal in a nondestructive noninvasive way because with |
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67:01 | these structures, you don't want to them and you don't want to cut |
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67:08 | them. Now, looters did because through Central American coast, there was |
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67:11 | of drugs going through and still are then, and then lots of arms |
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67:17 | then lots of looting of these So people would go into the |
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67:20 | they would search all over talk to locals and then find a pyramid and |
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67:25 | uh cut it and try to loot . And so that, that happened |
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67:28 | lot. You can see that big like this, this is cleaned |
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67:32 | But where we were, people would these structures and then cut into them |
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67:37 | see if there's any goodies inside and often was. But anyway, that's |
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67:43 | , we were just doing the archaeology the uh the imaging. So that's |
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67:46 | basic idea. Um Now we could out that was taking a horizontal |
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67:52 | but we can do the same idea vertical slices. And if I've got |
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68:08 | well here and then another while here receivers, I can just get the |
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68:16 | times to each one of these receivers the shot, divide up the earth |
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68:23 | take these sums that travel time is sum of all the slowness is through |
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|
68:28 | and then do the inverse problem with guy and create an image between the |
|
|
68:38 | . So, and that's, that's we're gonna do. But let's take |
|
|
68:41 | quick break, Stephanie, then we'll back, we'll talk some more about |
|
|
68:46 | . OK. All right. Toxin. OK. Great. Welcome |
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69:09 | . OK. We're just gonna kind spot check in here, Stephanie to |
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69:14 | to get some of the basic concepts in and then wrap up. So |
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|
69:22 | , the basic idea with Crosswell is got to have some kind of source |
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69:27 | the, well, now, so got to create this kind of disturbance |
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69:31 | the, well, and then we've to have a receiver in the other |
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69:35 | , to, to record that So once again, some kind of |
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69:41 | deform or something in, in well, and then some kind of |
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69:45 | that's vibration or pressure sensitive in the . Well, and so uh here's |
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69:51 | of the sources that we've done just the, in the shallow case down |
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69:55 | the mark. So one is uh sparkler, what's called a spark |
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70:04 | and this uh for this guy, is just a big stack of batteries |
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70:12 | then it has a spark plug on end. So the way it works |
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70:27 | that we're gonna have uh batteries on surface and then we're gonna charge up |
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70:32 | set of capacitors and batteries down So we're gonna charge this all |
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70:36 | put a big voltage across here and release it across just a little metal |
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70:45 | here. So you've seen spark plugs a car or from a lawnmower or |
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70:50 | like that. And so it's just release across the little um gap between |
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70:58 | two pieces of metal. So what does is that this is in the |
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71:02 | in the water and it basically uh , it's very, very hot, |
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71:10 | a huge electric current going across, heats up the water, basically |
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71:14 | it just produces steam and a And so quick discharge, electrical discharge |
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71:22 | the water heats it up. And so it just creates a, |
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71:27 | pressure pulse in the borehole. And our shaker. Uh, another, |
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71:34 | technique that's mechanical. This is another that we have is this is uh |
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71:40 | little cylinder. The cylinder has a inside it and then a plunger and |
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71:43 | weight on the end. And this into the borehole, we inflate the |
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71:50 | here so that it presses against the of the borehole and then you just |
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71:55 | it up and drop it. it just creates boom, a sheer |
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72:01 | the borehole wall. And that is disturbance of vibration that propagates across between |
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72:10 | wells. So this is just an of one of the ones that um |
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72:13 | we shot at Lamar. So we our two wells. I think you've |
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72:21 | those guys uh Lamar and then we've the uh the sources on one |
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72:30 | And then the receivers now as a , we can put download geophones again |
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72:35 | sometimes we use a hydrophone cable, hydrophone cable just has uh pressure sensors |
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72:44 | it. We just lower it into hole. It has all these pressure |
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72:47 | and then we're gonna detect the energy goes from one more hole to the |
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72:58 | . Did we do Croswell at Lamar , with you at all? |
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73:06 | because I was the semester that COVID . So we couldn't do anything. |
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73:11 | But I did do a well exercise Doctor Wiley. Uh, we did |
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73:18 | water or like hydrology, geophysics or with him. We did something but |
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73:26 | was my first song out there to . Yeah. Um, so |
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73:33 | you've been there once? Just the ones with, uh, Bob |
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73:37 | with ones with Doctor Wiley? And I did another one for, |
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73:40 | when I took, uh, applications GPS and we did a couple different |
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73:46 | out there with Bob Wang. Doctor Wang. I was like, |
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73:50 | was his name? I can't It was so long ago. Um |
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73:53 | yeah, we went out there with too, but that was it. |
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73:56 | , ok. Oh, good. , you know the area and then |
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73:59 | we've also drilled two wells there or wells and that's where we do a |
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74:02 | of little tests and instruction. So was the idea and just to look |
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74:08 | some of the data, here's the of data that we receive. So |
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74:13 | we're again looking in depth and this the Scorpion. So this was the |
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74:24 | , the spark or source in Well, and then We had the |
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74:31 | array in the fluid in the Well, and the hydrophone was going |
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74:37 | 22 m to 118 m. So , and you can see that uh |
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74:45 | know, the shot, the shot something like 30 m down in one |
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74:51 | , and that um propagates across So , the uh the, the shot |
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75:00 | in one well, at about 30 and then we've got the hydrophone string |
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75:03 | the other. Well, that's down and 18 m. And so we |
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75:07 | and then that data is recorded on hydrophone string. And then we were |
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75:16 | part of this exercise, we were testing different sources. The other, |
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75:21 | , the weight dropping source, the one with the bladder is called a |
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75:25 | source. And so we were testing spark versus the Ballard. You can |
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75:29 | the sedate is pretty clean and you actually start to see some reflections coming |
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75:33 | up to the surface now. So Ballard gave some very nice, some |
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75:40 | nice data. So once again, our geometry, we've got uh a |
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75:47 | , say one shot here, the is going down here and you can |
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75:52 | see the energy propagating across and arriving all different times. So in this |
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76:07 | , the uh thesaurus was at 38 . So the thesaurus was just right |
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76:14 | about there. So in around here we can see the energy all coming |
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76:24 | . Now, there's other, there's energy forms because what happens is the |
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76:28 | goes across, it hits the fluid , this hydrophone string is in a |
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76:32 | filled borehole. And so we get low velocity wave going down the, |
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76:37 | fluid which isn't too instructive to We're looking for, we're looking for |
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76:42 | going on between the wells, not going on in the fluid here. |
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76:47 | we're gonna suppress that in processing and pick all this stuff now as a |
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76:54 | project with a student right now, , we're looking at uh DA |
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77:01 | which is a fiber optic data. the fiber optic sensor in a horizontal |
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77:07 | with shots on the surface. So got the wells drilled horizontally, there's |
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77:13 | all in the horizontal well inside the , then we've got surface shots. |
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77:18 | I think you can imagine that's again crosswell geometry just now on its |
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77:23 | So shots receivers and so we can that whole thing is also crosswell and |
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77:32 | what we're starting to do right now uh another one of the grad |
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77:38 | That's his part, his phd. . So um that's the basic idea |
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77:52 | um with the crosswell geometry. Uh you can see how it, how |
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78:05 | works is we've got all of our and for every shot we can pick |
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78:14 | times of the receivers. And so you can see that much of this |
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78:20 | has been interrogated or traversed by different . So we're gonna do our standard |
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78:29 | here that we imagine we're gonna divide area up into squares or pixels and |
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78:36 | sum all the interval travel times to the total travel time. For every |
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78:40 | of these guys put it in a matrix equation and do the inversion and |
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78:46 | out with the velocities that are And so that's the idea we could |
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78:53 | different pixel sizes. We run lots different tests and then ultimately come out |
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78:58 | these velocities. So this is the of the slowness that fit all of |
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79:06 | travel times. Now, you can that sometimes there are no rays. |
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79:11 | the the area of confidence is right the middle here. So I'm confident |
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79:16 | these velocities, but this gives us background. So you can see that |
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79:21 | again, the sediments at Lamarque are around 2200 m per second, that |
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79:28 | number that we know and love. that's the P wave velocity of all |
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79:32 | sediments around here. So that's just the first arrivals in this particular geometry |
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79:47 | the tomography kind of concept good. . So that's uh that's the cross |
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80:04 | which we can put, we can it flat to look at pyramids, |
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80:08 | can put it on its side to at dams in the near surface. |
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80:12 | can turn it the other way and at surface to a horizontal well. |
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80:17 | it's a very, very powerful concept how to process data and make a |
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80:25 | good. So there's a bunch of stuff here. But I wanted to |
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80:30 | um just a little bit more um taking this into the micro seismic world |
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80:41 | this is uh also a big application a down hall source and uh surface |
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80:47 | receivers in the well. And so a, here's a kind of example |
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80:56 | and to bounce around not just oil gas because who knows where you're gonna |
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80:59 | up working. But this was in , the geotechnical world. And you |
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81:06 | see this nice mountain here and a valley. It turned out that uh |
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81:12 | can see a little bit of rock here and there was a peak here |
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81:18 | that 100 years ago failed and caused huge rock slide and buried an area |
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81:27 | the middle of a valley. So was uh actually the most fatal landslide |
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81:36 | North American history. And it buried a little village, a town in |
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81:45 | crow's nest pass as this is And uh this is called the Frank |
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81:52 | . So there was some worry that of these other peaks might um also |
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81:58 | at some point. And so we asked to investigate this and put some |
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82:04 | on and monitor the peak. So we actually ended up, it was |
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82:13 | um uh a quick, quick So we bid on the contract and |
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82:18 | we turned out we had to put this equipment on the mountain in |
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82:22 | in the winter. And so uh quickly did that. I remember the |
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82:29 | helicopter ride in the winter that we in to get all this equipment. |
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82:34 | We're bouncing around and they let us on the top of the mountain |
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82:40 | And I really started praying to every or goddess that I knew. I |
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82:47 | this, this is really a bad . But here we are. So |
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82:53 | uh we installed uh the equipment on mountain and here's an example. So |
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83:01 | this case, we had six stations we started monitoring cracks inside the |
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83:12 | So now we're listening to the These are micro seismic events inside the |
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83:19 | . And so once again, our is pick the P wave arrival |
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83:23 | the shear wave arrival times and locate source and find out the velocities. |
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83:32 | there are only a few stations in case. And that's um again, |
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83:36 | big inverse problem like we've been talking from the travel times, estimate the |
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83:43 | and the velocity. So some of signal processing is we don't want to |
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83:48 | around and pick this all ourselves. we have to figure out how can |
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83:51 | automatically pick events. And incidentally, just saw an advertisement for micro seismic |
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84:02 | . Did you see that? Oh, sorry, I was on |
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84:11 | . I didn't even know. Um , I haven't. They're looking, |
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84:15 | looking to hire people and your profile probably be very hirable with them. |
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84:22 | . Micro seismic ink and they do stuff that I'm just about to show |
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84:26 | . That's exactly what they do. they've hired a for a few of |
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84:31 | former students there already. So Uh think Jose Basil is there right now |
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84:48 | uh I think Elena might be there . I think they've hired several of |
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84:54 | students. Hm. Ok. So kind of work that they do is |
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85:01 | this, they monitor hydraulic fracturing and enhanced geothermal systems. They've just started |
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85:10 | whole new uh subsidiary company called, think it's called Micro Thermal Inc, |
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85:17 | is doing geothermal work with uh down fracturing and hydraulic fracturing, et |
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85:22 | So what they do is they do from geophones that are on the surface |
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85:27 | in the borehole and they're monitoring fracturing or, or seismicity underground. So |
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85:35 | what you do. They've got all sensors and they, they first of |
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85:41 | have to detect events. So say got some seismic, we're continuously recording |
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85:54 | a surface station or in a down station and then there's a, a |
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86:00 | fracture or a micro seismic event or mini earthquake or something. And that |
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86:05 | a vibration and that vibration transits to sensor, our geo phone and boom |
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86:13 | it is. So I would like be able to automatically detect that. |
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86:26 | it looks pretty easy when uh I see it, you could go in |
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86:29 | you could say, OK, there's onset I can, I can determine |
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86:34 | . But now you've got to stay all night 24 hours and you're only |
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86:37 | to staying up 20 hours, OK. You're accustomed to staying up |
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86:43 | hours, you get two hours but you want to go to sleep |
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86:46 | those two hours. Um So we to do this all automatically, but |
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86:54 | would tell you that this used to be picked by hand. So when |
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87:00 | was, when I was a there were whole companies that just took |
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87:05 | like this, they just had dreams people that just picked these events all |
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87:08 | long. And as grad students, was our job. And even up |
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87:12 | about 15 years ago, people still to do all this stuff by |
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87:16 | And grad studentss probably still do for earthquakes. But uh there's so many |
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87:22 | these events they gotta to be And so you can see how we |
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87:26 | begin to do this. There's a of character here, we can |
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87:31 | first of all, the simplest thing can do is say, you know |
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87:34 | the amplitude changes a lot. So defining the event by an amplitude |
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87:38 | And this is the the simplest way do it. There's something called a |
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87:43 | term average that's just gonna take the as it runs along here of a |
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87:50 | number of samples. And then there's long term average, it's gonna take |
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87:56 | average of a whole broader window of . So if I run the short |
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88:05 | average across this signal, Then I the little line in red here, |
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88:11 | can see that this all averages out almost zero because it's kind of like |
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88:16 | noise. So we're getting zero there then all of a sudden the short |
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88:21 | average when it hits this, it up like crazy. Now, the |
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88:29 | term average is just another averaging. so it's coming along and as it |
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88:34 | to get in here, it's starting feel that the aptitude is increasing, |
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88:38 | it's got such a long window that doesn't feel it too much and then |
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88:43 | it gets bigger and bigger and then down. So one simple way to |
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88:52 | a detection would be to just take ratio of these two guys and once |
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88:59 | ratio exceeds a certain value, I'm declare that's a trigger, that's an |
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89:08 | . Mhm Now, in fact, could have just set a noise level |
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89:15 | and then gone in right in this said whenever it gets above a certain |
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89:19 | level, just pick it and people that. So that would be one |
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89:22 | , but it's often it runs into . So you can see what happens |
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89:26 | . We take our short term our long term average, take the |
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89:31 | and when that exceeds some trigger say two, we're going to say |
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89:37 | that is the event and then we're gonna calibrate a little bit because I |
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89:47 | there's a bit of a delay but the event is somewhere around |
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89:51 | And so that's how we can first of all, just calibrate |
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89:56 | give it its threshold and then from on, just let it go in |
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90:00 | do all of its picking and just me the time. So that is |
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90:06 | event picking. And then once I've all those picks, I can start |
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90:10 | process them. So here's what micro ink is gonna do or some company |
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90:19 | it, there's a hydraulic fracture that breakages, that break causes a vibration |
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90:25 | we monitor that and get the arrivals all these different levels. So the |
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90:37 | , one of the problem with this that actually we don't really know the |
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90:43 | or the location of this micro seismic . But I've got a monitoring |
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90:50 | So I could have measured the So I might have I measure the |
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90:54 | here. I've got that and now the velocities, I've got to determine |
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90:59 | location. So this is the hyper location problem. And so let's just |
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91:10 | one. Here's a simple case. was actually real data. So we |
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91:23 | a, we had receivers in the and then there was an event someplace |
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91:35 | I don't know where it was, from just one receiver in the, |
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91:42 | , I'm gonna try to determine where event was. So that the, |
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91:48 | technique is that we find an we've got an automatic pick. So |
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91:54 | get an arrival of the P wave some time P this event went off |
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92:02 | some unknown times, say, and it traveled some distance with a known |
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92:11 | . So the P wave time, you can see here is T P |
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92:14 | equal to T plus D over B P. And you can see the |
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92:30 | S if there's a shear wave it happened at the same time, |
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92:35 | it just took longer to get there it traveled more or less the same |
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92:38 | , but it was traveling to the wave velocity. So if I can |
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92:42 | the P wave arrival and the shear arrival, then I can determine how |
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92:50 | away it was. And the way we're gonna do that is to subtract |
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93:07 | two guys. What does subtracting them ? It gets rid of the T |
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93:10 | term, the origin time term because don't know what that was. And |
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93:15 | I'd like to get rid of And the way I can get rid |
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93:17 | it is to pick the P wave the shear wave time and subtract |
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93:22 | And that difference gets rid of the time. So you can see the |
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93:42 | equation here, I pick a P time. I pick the shear wave |
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93:49 | . I know the velocities because I've say a V S P measurement or |
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93:54 | characterized the subsurface. So I know P and I know V S and |
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93:59 | all I need to do is calculate distance. So what that's going to |
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94:14 | is give me um a distance from receiver to the source. Now, |
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94:28 | I had a whole pile of I could do various things. But |
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94:31 | , for example, I've just got receiver, but it's a three component |
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94:37 | . Then we talked about photographs at angles and so I can use how |
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94:42 | energy is on each channel to figure the direction too. So I get |
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94:52 | distance from the difference in arrival times I'm gonna get the direction from how |
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94:57 | is on each channel. So you imagine here if I've got a vertical |
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95:02 | and a horizontal GEO, this energy gonna arrive. And how is it |
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95:09 | to express on the vertical and the geo how it's gonna express like what |
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95:23 | you mean like positive or negative Yeah, so we'll get, we'll |
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95:27 | some energy on the vertical and some on the horizontal and it's going to |
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95:33 | up and down like this. So should, for this case here, |
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95:38 | should see energy on the vertical and should see energy on the horizontal. |
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95:43 | it's gonna look, if I plotted together, it would look like a |
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95:48 | . But separately, I'm just gonna energy on the vertical and I'm gonna |
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95:51 | energy on the horizontal. If that was more or less equal, then |
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95:56 | would tell me the arrival angle is I saw equal energy on the vertical |
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96:05 | equal the same amount of energy on horizontal. What arrival angle would that |
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96:11 | me Uh is that 45°? Yeah, be about 45°. Yeah, but if |
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96:24 | , whatever the ratio is, I just take the inverse tan of that |
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96:31 | ratio. And that's gonna give me angle just like you pointed out. |
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96:38 | let's just do this little calculation. actually was from a uh this is |
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96:48 | data from a site. And we that the P wave velocity on average |
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96:57 | this site is about 2000 m per . The shear wave velocity is around |
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97:02 | m per second. So I've got velocities and what I know, |
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97:25 | that I had my three component geophones and then I recorded this data. |
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97:49 | I want to figure out I've got recording here. How far away was |
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97:56 | rupture or that micro seismic event? we want to use our little equation |
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98:02 | was T S minus T P is distance times the reciprocal of these |
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98:21 | So here's the vertical element, Horizontal and Horizontal two geophones. And we're |
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98:34 | to interpret that there's the first arrival is the P wave arrival and we |
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98:40 | see how it it expresses on the channel and the X and Y |
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98:50 | So first of all, what time , what time is this arrival |
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99:00 | Hm. A little so P wave a little less than three. |
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99:05 | So like maybe like two point 7 . Yeah. So let's take it |
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99:17 | .2 seven. Ok. And then s wave is more than three, |
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99:31 | .26. Somewhere around there. So the S wave is Maybe like |
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99:40 | . Yeah. So somewhere around Ok. So just plug that into |
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99:51 | little equation. One over 701 over . Mhm. I got negative. |
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100:24 | , I did not get pulled Wow. Miles. So two About |
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100:49 | , 97.8 uh meters. OK. oh 835 Oh I guess 20.26. |
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101:23 | , .26. So that should be . Yeah, which is OK. |
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101:37 | we're just, we're just doing this . So it's somewhere around 90 |
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101:46 | And so that that tells us how away it is. It doesn't say |
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101:55 | it is, it just says how away it is, but we can |
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101:59 | a little bit better than that by idea of we had three components here |
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102:05 | I have an arrival angle that's got , for example, big time on |
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102:15 | of the components. So first of , if say I've got vertical and |
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102:23 | horizontal is north X and then Y east. So if I've got Z |
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102:39 | vertical and say X is east and is north? Why is north? |
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102:57 | a yeast more or less? What do you think this is coming from |
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103:07 | you can write it down. I've Z why is north? So just |
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103:39 | make sure, let's see. Um I'm seeing where it's ok. Um |
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104:20 | not sure how I would figure it . I mean, I know it's |
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104:30 | I know that um hm would it ? Mhm. No, I'm not |
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105:11 | . Well, um you can see there's very little arrival this on this |
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105:20 | horizontal channel. Ok? So if no arrival on the North channel, |
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105:26 | no energy in that channel really? the energy be coming from that |
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|
105:36 | Yeah. No, there's nothing on North channel. So it's not coming |
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105:41 | the north. If it were, have, I'd have energy there. |
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105:46 | there's there actually is a little, bit but not very much. |
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105:52 | So we can see on the East now this guy there's a fair amount |
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105:58 | energy. So it's coming from the then on the vertical channel, there's |
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106:07 | fair amount of energy. So it's upward. Mhm So when it, |
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106:22 | know that there's a half of the is on the vertical, half is |
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106:28 | the east. So It's coming up of as 45° on the vertical and |
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106:38 | channels. I don't even see that X Y at first because our chat |
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106:46 | was like kind of covering it because was like, how am I supposed |
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106:49 | know? But it makes sense Oh, good. Oh, that's |
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106:55 | bad about that. Yeah. that, that's key, that's key |
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107:00 | . Yeah, I was like, am I supposed to know? |
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107:05 | I've noticed that sometimes the, various things are being covered up by |
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107:11 | or something. So, but it is so that now we |
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107:18 | we can even check this out a bit because that was the P wave |
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107:25 | was oscillating on these channels. But had the shear wave coming up |
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107:30 | which we assume is coming up sort in the same direction it was from |
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107:34 | same source. So if I have shear wave coming up like this, |
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107:54 | remember its particles are oscillating Ortho So I should still see primarily. |
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108:02 | it's a lot bigger. Mhm So a little bit on the north channel |
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108:13 | little bit. So we know that source is not directly east, it's |
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108:20 | little bit east northeast because there's a bit of energy there. And then |
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108:29 | I look at this, I've picked Z, here's X. So the |
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108:37 | wave is coming up, we can some of it on Z, we |
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108:39 | see some of it on X, shear waves coming up. I could |
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108:45 | some of it on Z and some it on X. Now, if |
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108:48 | look just in plan view, as said, most of the energy is |
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108:52 | X, but there's a little bit Y or North groups. So we |
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109:12 | check. And that ultimately is what seeing so that here's the energy we |
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109:21 | its distance, we got its direction we can do all that just from |
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109:24 | single G phone. Now, in practice, you're gonna use a |
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109:32 | array of geophones to nail this a better or you're gonna put some on |
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109:36 | surface like micro seismic does. But is an idea of sort of an |
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109:40 | in situ shot and an in situ in the crosswell geometry. And if |
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109:47 | trying to detect events, then this how we can do it. So |
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109:53 | is called a hypo center location. means beneath like a hypodermic needle beneath |
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109:58 | needle. So this is a hypo , the epicenter is on the |
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110:05 | the hypo center is at depth. so this is how we can do |
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110:09 | micro seismic analysis. And so what going to do is you've got a |
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110:25 | fractured area, you've got sensors in , well, it breaks it |
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110:33 | we pick all of those arrivals and we estimate where the break was and |
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110:41 | big it was. And this is people do with micro seismic analysis. |
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110:47 | so they're trying to find out where the rock break and then how big |
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110:51 | it, how big of a fracture it cause? How big of a |
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110:55 | was it? And this is the of micro seismic analysis that's used to |
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110:59 | hydraulic fracturing for oil or as micro thermal is now doing or micro thermal |
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111:09 | geothermal production. So that's um uh application. Good. Oops. |
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112:52 | Sorry, I was dealing with screens and I think I lost you. |
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112:59 | still here. Ok. Oh, , good. OK. So that's |
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113:07 | that's a run through of crosswell. just a quick, there's lots of |
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113:11 | stuff there, but that's just a overview of some of the cross view |
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113:17 | concepts. Uh Let's just take one case and put this all together. |
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113:35 | is all all posted. Stephanie, uh there's a bunch here, but |
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113:38 | just go through one case. I you probably remember this time. Uh |
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113:45 | years ago, I was taking pictures my uh my view uh here and |
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113:51 | could really see, you could really the water Here was, here's Highway |
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113:59 | 88 here, completely flooded. Then buildings outside my building were under about |
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114:08 | ft of water. Um But let's on will just pick one of these |
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114:17 | cases. Uh I want to quickly, quickly talk about Geats and |
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114:51 | OK. Let's uh let's take this that ultimately, a lot of the |
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115:04 | um what our job is is to how much uh fluid or, or |
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115:14 | in place or gas in place or resource or something, how much is |
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115:21 | place. And again, our job to calculate basically an oil column and |
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115:28 | that oil column times an area and gives us the volume of resource in |
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115:33 | . So this is in, in reservoir world. So what we've been |
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115:48 | with our log analysis is we've been the thickness of the area of interest |
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115:55 | the iso pa. So we've been log ins interest. We've determined sand |
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116:02 | say from the gamma ray log. been looking at the porosity logs and |
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116:07 | with resistivity, we've been calculating the of hydrocarbon fill. So if we |
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116:14 | all that together, that gives us oil column or just the thickness of |
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116:26 | resource, and then if we multiply times the area, that's just the |
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116:31 | of fluid there. And so that's original oil in place or original gas |
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116:37 | place or we could convert that probably original heat in place or our original |
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116:43 | water in place. So this is whole idea. And so we imagine |
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116:49 | seismic is gonna have to be interpreted give us the area. All of |
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116:54 | log analysis is gonna give us the column multiply it together. And then |
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117:00 | turn that over to the production engineers the accountants and they're gonna tell you |
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117:05 | you get any more of this or a bonus this year. So that's |
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117:09 | idea. So we can put that more of a sophisticated equation that the |
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117:13 | oil in place is conversion factors, area times thickness times porosity times hydrocarbon |
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117:24 | . Um Then when we take the out of the ground, typically the |
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117:30 | is gonna come out of it. the oil is going to shrink or |
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117:37 | , It will expand because it's under pressure, but it's gonna shrink because |
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117:41 | gas will come out of it. so that's a little factor. Might |
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117:44 | .9 and it's not too big, it might be some little factor. |
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117:50 | . So what I wanna do is wanna put together our log analysis and |
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117:55 | seismic and try to estimate the original in place and we'll do that with |
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118:02 | study. So in this case, going to interpret our seismic and then |
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118:07 | well logs try to put it all and get a volume. So we've |
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118:14 | a 3d seismic in the area and we're taking that volume of echoes reflectivity |
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118:21 | I'm Cutting across it, I'm looking the volume at one time and in |
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118:31 | , there's sand channels in this area we're looking at the top of the |
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118:36 | channels at that echo time. So you looking deeper in the volume cutting |
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118:43 | and I've got the amplitude of the reflections at that time. And I'm |
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118:49 | these bright amplitudes as my sand Now as it turned out, these |
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119:03 | drilled and oil was discovered. But very top and what, what the |
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119:11 | is here is just the amplitude of reflection. So this is a big |
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119:14 | reflection. So as we've talked, we go down the section, what |
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119:21 | cause the biggest amplitudes that we could what kind of rock change or can |
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119:30 | the biggest reflections like from you like from like a low density to |
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119:37 | high density or something? Yeah. . Yeah. Because like we smell |
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119:43 | the salt and then when I went that shale to limestone, like those |
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119:49 | pretty big differences. Yeah. So could be a big mythology change. |
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119:57 | . But what else can cause big competing contrasts? Um Hydrocarbons. |
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120:12 | exactly. Especially gas. If the are gas saturated, that's gonna really |
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120:17 | the density and lower the velocity. so that's another big contrast. And |
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120:23 | it turns out here, it's actually . So we've got a mythology change |
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120:29 | shale to sand and then the top the sand is gas saturated. So |
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120:36 | gives us these boomer reflections. Those reflections were drilled now as it |
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120:53 | out uh you drilled through them and was oil but the reflection is actually |
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121:00 | on the top. Ok. So that was in time and I |
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121:10 | to convert it to depth. we could just stretch it like we |
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121:18 | before. But this is an aerial . So I've got, I've got |
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121:23 | number of wells in here and from well logs, I know the depth |
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121:30 | that reflector say. So I know depth of a reflector from the well |
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121:40 | . And I know the time of reflector from the seismic, I picked |
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121:45 | seismic and then I can do that multiple horizons. So I can |
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121:50 | say one event here, pick another here and take the time difference. |
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121:55 | that's called an isochron, that's a thickness. But then I know from |
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122:01 | well logs, I've got the interpretation the that top and the base. |
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122:06 | I know the actual depth thickness So from multiple well logs, I |
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122:13 | that all the depth thicknesses and then my seismic having picked two surfaces that |
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122:19 | to those, I've got the time or the isochron. So I can |
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122:28 | the Isochron thickness. That's just the between two layers and the actual depth |
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122:35 | two layers. So I want to this Isochron map to in time to |
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122:44 | iso pack or an actual thickness map depth. So what we're gonna do |
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122:54 | use some just statistical ideas to, do that. So here's the one |
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122:58 | idea for Friday afternoon. The idea that I've got all of these wells |
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123:13 | for each, well, I've got thickness. Now, you can imagine |
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123:23 | the wells are really close together, difference in thickness is gonna be what |
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123:34 | if the wells are really close Yeah, then the thickness isn't gonna |
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123:42 | very big. Yeah, for It should be pretty much the |
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123:47 | And in fact, as I put wells exactly together, the difference is |
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123:51 | to go to zero and then as take the whales farther and farther |
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123:58 | well, anything could happen. But what I can do is I |
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124:08 | look at how much does that difference as I go farther and farther |
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124:15 | So, the whole concept here is a function of distance. How much |
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124:25 | do I get? Mhm. So , I can look at The |
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124:42 | the one thickness and then I could at all the other distances away and |
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124:49 | how different those are and construct what's a Vario gram, which is just |
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124:57 | difference in that thickness. So here's plot of a vari gum as I |
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125:03 | farther away from one, well, variation gets bigger. Mhm Stand to |
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125:12 | . But it turns out that when scale that variation, it usually levels |
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125:18 | . So once I've got a certain away that the that the variation is |
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125:22 | a certain number, so that's, kind of a limit. So what |
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125:30 | wanna do is take this Isochron which is a measure of the time |
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125:43 | from the seismic between say this Mississippian a Manville at the tops. And |
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125:47 | got a time thickness and I've also a thickness from the log. So |
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125:55 | I'm gonna take each log and compare to each other log and see how |
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126:01 | changes as a function of distance. how I construct the vari gram and |
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126:06 | I want to convert this whole map a thickness using those vari graphs. |
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126:19 | the question is suppose I just have data and I've got these sects that |
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126:24 | going 100 and 50 m, 100 60 m, 100 and 80 |
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126:27 | And I look at the variation as function of distance. Then I can |
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126:32 | you I can give you a number any point here. That's based really |
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126:39 | all these other points. And the in GEO statistics is that from looking |
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126:49 | these pairs and seeing how the variation as distance, that gives me a |
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126:56 | . So if I want to output point here, I'll use all these |
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127:01 | and add each of these values weighted how far away they are. So |
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127:06 | are the two concepts in GEO statistics I want to output. I want |
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127:12 | get a, a point here, I only have all these other |
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127:18 | So how do I use all these points to predict what's here? And |
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127:23 | way you do it is it'll take these known points compute how they vary |
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127:27 | distance. And then for this point , I will wait the distance from |
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127:32 | point to all the other ones, their values and get a value that's |
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127:36 | weighted sum. Oh that's a But that's the GEOS statistical approach and |
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127:44 | works pretty well. So I'll do , not just with the well logs |
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127:52 | are in depth, I'll do that with the time thickness from the |
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127:57 | which is in time. But I've a relationship between time and thickness. |
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128:04 | so I'll convert everything and geo statistically each one of these points using that |
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128:11 | . So this is called core. now I've converted, using all the |
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128:16 | information and all the seismic information. converted this whole map now to depth |
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128:23 | thickness. And I'm looking for thick in the reservoir. Then I can |
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128:40 | leave one of those points out. the whole analysis. Look at my |
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128:45 | compare to the actual point and get error and begin to understand how wrong |
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128:50 | am. This is called a validation . So with this thickness, It's |
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129:03 | somewhere around 170 m thick, but can leave one of these real well |
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129:08 | out do the all the analysis compare real to the predicted output. And |
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129:13 | I can say that in general For map, I'm within plus or -10 |
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129:20 | . And so that gives me a . OK. So we go through |
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129:30 | whole analysis and we take all the from seismic, all the a all |
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129:39 | I've got from the log and I predict the thickness with confidence. I |
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129:46 | predict how much sand there is with . And I can also do the |
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129:50 | same thing with porosity and even So we put all that together. |
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129:56 | then ultimately jumping ahead, I can the oil column conjure that up from |
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130:08 | and then predict how much oil is place. So that's, that's a |
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130:17 | . And it would um that's a course in itself. But that's the |
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130:21 | idea of using logs with seismic and it all together. Now, the |
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130:29 | we want to do this is that got a few logs and I've got |
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130:33 | size back and I would like to exactly how much oil is it in |
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130:39 | and I can do that. And people are going to, the engineers |
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130:43 | gonna pump it for a year or and they're gonna history match and do |
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130:46 | their simulations and they're gonna get a , but their number came two years |
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130:51 | our number. And so we came with a number that said, you |
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130:56 | , you've got eight million barrels of in place there after a couple of |
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131:01 | of production, they came out with similar number. So, uh I |
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131:14 | say that jumping there, I gave talk some time ago about 10 years |
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131:19 | we'd done the work, a guy up and he said, you know |
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131:21 | , I just wanted to check and how with 10 more years production, |
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131:25 | this all turned out. So he and he looked at this whole area |
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131:29 | he got the government statistics on how had been produced. So ultimately, |
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131:37 | had predicted that you would be able say that this particular pool there |
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131:43 | I think what we predict, we that there was 90% chance that there |
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131:51 | 4.5 million barrels of oil. And after 10 years of production, they |
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131:55 | actually there was 5.5 million barrels of . So that was pretty good. |
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132:03 | Again, uh with a little bit time, AP 90 is what the |
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132:08 | industry uses for reserves. And that's probability that your answer Is 90% |
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132:20 | So we said that it's 90 there's 90% chance that there's more than 4.5 |
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132:26 | barrels of oil there. And then the end after 10 years of |
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132:30 | they said, well, we've found there's actually 5.5 million barrels of |
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132:35 | which is good because that would be our p 50. But when you |
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132:41 | it to the bank, they don't to say, I don't want 50 |
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132:43 | odds. I want a 90% So that was good. So Stephanie |
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132:50 | wrapping up with our work. Um looked at some core, we looked |
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132:58 | well, logs, we did petro , we did some of the basic |
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133:02 | for saturation. We did V S ties and then we looked at the |
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133:08 | geometry really fast. And then how do we can roll all this |
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133:13 | together to get uh, a reservoir . So, um, that's |
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133:22 | that's a quick run through and I your brain might be partially full, |
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133:30 | saturated. Good. So, I we'll, um, I'll leave it |
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133:43 | . Um, just got the one , one little exercise that we talked |
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133:48 | earlier, so, maybe finish that and then, uh, I'll |
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133:54 | uh, Utah and you the, test probably Tuesday night, I |
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133:59 | And then Tuesday or Wednesday and then got three or four hours to go |
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134:04 | it. It won't be that It'll be something like an hour long |
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134:11 | . Do you want me to have back to you by Tuesday or send |
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134:15 | to you Wednesday night? Um, , how's your schedule looking for |
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134:21 | Do you have a couple hours Wednesday ? Yeah, I mean, I |
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134:26 | home from work around what time I get home about five and then everybody |
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134:33 | home at about six so they can the baby while I kind of just |
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134:37 | myself in office. So that should fine. Well, why don't |
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134:41 | I'll send it to you Wednesday morning something and then just set it in |
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134:46 | Wednesday night when you finish it. . Ok. That'll work. That's |
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134:52 | . All right, good. we'll do that then. Um, |
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134:55 | then, uh, I, I know, does I, are, |
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134:58 | you online when you do it or it just, or just, |
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135:03 | by yourself? Or how, how been doing that? Oh, I've |
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135:07 | been doing it by myself. So I'll get it to you Wednesday |
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135:13 | and then you could take three or hours however long you want it only |
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135:16 | an hour long, but you can some more time and then just fire |
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135:19 | back to us Wednesday night. I can do that. Ok, |
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135:25 | . We'll, we'll talk to uh, in the interim and |
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135:29 | uh, wrap things up for late night. Ok, that'll work. |
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135:35 | , beautiful. Have a good You too. Thank you so |
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135:37 | I appreciate everything. You bet. to you later. See you |
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