WEBVTT Kind: captions Language: en-US 00:00:01.280 --> 00:00:02.856 Greetings. 00:00:02.880 --> 00:00:08.456 The USGS Earthquake Science Center has a new nodal seismometer facility. 00:00:08.480 --> 00:00:12.160 I’ll describe a little bit about what we have and what’s available 00:00:12.160 --> 00:00:15.622 if anyone wants to use it. 00:00:16.720 --> 00:00:20.240 Nodes, for anyone who’s not familiar with them, are a new generation of 00:00:20.240 --> 00:00:26.136 seismometers that were really originally developed for the oil industry. 00:00:26.160 --> 00:00:29.760 They’re small, portable, wireless, and they have an onboard GPS 00:00:29.760 --> 00:00:34.376 and solid state storage. They have an internal rechargeable battery. 00:00:34.400 --> 00:00:39.336 They can record ground motion, timing, and location all in the same package. 00:00:39.360 --> 00:00:45.736 They can record for days, weeks, or even months in some situations. 00:00:45.760 --> 00:00:51.940 They can record both below the ground surface or above the ground surface. 00:00:53.280 --> 00:00:58.160 The ESC nodal seismometers are more research-oriented seismometers than 00:00:58.160 --> 00:01:02.936 the oil industry type, which are a typical vertical component. 00:01:02.960 --> 00:01:07.280 The ESC seismometers are three- component. We have 500 of them. 00:01:07.280 --> 00:01:12.480 We have four 16-slot portable charging systems and comparable 00:01:12.480 --> 00:01:16.800 harvesting systems. We have multiple field deployment tools – 00:01:16.800 --> 00:01:20.160 which I’ll explain later, several laptop servers, 00:01:20.160 --> 00:01:24.144 gigabytes of portable storage, and auxiliary equipment. 00:01:25.440 --> 00:01:29.520 The ESC nodal seismometers, again, are three-component seismometers 00:01:29.520 --> 00:01:33.816 with the internal battery that lasts about 30 to 40 days per charge. 00:01:33.840 --> 00:01:37.360 Now, that battery is changeable, as you can see here on the right. 00:01:37.360 --> 00:01:42.800 The sensor, recorder, and GPS is the top part of the unit, and the 00:01:42.800 --> 00:01:47.736 bottom part is the battery with the spike on it for securing it to the ground. 00:01:47.760 --> 00:01:55.989 Now, because it has internal GPS timing and location, you can – 00:01:55.989 --> 00:02:02.184 it is recorded automatically, even if it’s buried up to a meter deep. 00:02:03.280 --> 00:02:13.416 Now, they also have quite a wide recording range for frequencies, 00:02:13.440 --> 00:02:17.040 from seconds up to about 1,000 hertz, and I’ll show 00:02:17.040 --> 00:02:21.416 some slides on that in the next couple slides. 00:02:21.440 --> 00:02:26.296 You can select a choice of gains from zero to 36 dB in 6-dB increments. 00:02:26.320 --> 00:02:34.856 You can change the sampling rate from 0.25 milliseconds to 4 milliseconds. 00:02:34.880 --> 00:02:37.840 It can be deployed in one to two minutes once you’re on site, 00:02:37.840 --> 00:02:45.016 so they’re really fast for deployment. And they’re IP67 water- and dust-proof. 00:02:45.040 --> 00:02:49.520 So, if you bury them in a marsh, still you can be assured 00:02:49.520 --> 00:02:51.615 you’re going to get good data. 00:02:52.720 --> 00:02:59.040 Now, as I mentioned, the frequency range is quite wide, and to examine that, 00:02:59.040 --> 00:03:05.576 we did a study with UC-Berkeley, which was led by Taka’aki Taira. 00:03:05.600 --> 00:03:09.920 And what we did was we put a node outside the UC-Berkeley vault, 00:03:09.920 --> 00:03:14.776 one inside the vault with two broadband seismometers. 00:03:14.800 --> 00:03:23.496 And here is the – here are the recordings from a magnitude 6.7 teleseismic event. 00:03:23.520 --> 00:03:29.256 And the data are filtered from about 20 seconds to about 2 hertz. 00:03:29.280 --> 00:03:32.640 And, as you can see, the data are very comparable, 00:03:32.640 --> 00:03:37.920 particularly the in-vault node and the STS-1. It looks very similar. 00:03:37.920 --> 00:03:45.840 But overall, all of the recordings look similar in that recording range. 00:03:45.840 --> 00:03:52.216 And this is for the body waves. If you look at the S waves, again, this – 00:03:52.240 --> 00:03:58.296 going down to about 33 seconds in frequency, you can see, again, 00:03:58.320 --> 00:04:04.936 we have very comparable recordings for both the nodes and the broadbands. 00:04:04.960 --> 00:04:09.040 So this shows us that we can get very good low-frequency data, 00:04:09.040 --> 00:04:11.920 which is generally what you want for earthquake recordings. 00:04:11.920 --> 00:04:15.760 But the nodes also go very high on the frequency scale, 00:04:15.760 --> 00:04:18.800 up to about 1,000 hertz, which the broadbands do not do. 00:04:18.800 --> 00:04:23.896 Broadbands typically top out at about 25 to 50 hertz. 00:04:23.920 --> 00:04:28.645 So it makes the nodes a very flexible instrument. 00:04:30.080 --> 00:04:33.920 Now, that makes them ideal for aftershock recordings, 00:04:33.920 --> 00:04:38.400 short-term earthquake monitoring, noise studies, reflection and refraction 00:04:38.400 --> 00:04:40.640 site characterization, guided wave recordings – 00:04:40.640 --> 00:04:44.581 a whole series of the type of recordings that you might want to do. 00:04:45.360 --> 00:04:52.480 And they are very simple to deploy. Basically, you need two things. 00:04:52.480 --> 00:04:55.416 You need a node, and you need a simple magnet. 00:04:55.440 --> 00:05:00.320 And that will start it – will record it. However, if you’re deploying 00:05:00.320 --> 00:05:03.520 a lot of instruments, it’s good to have something called a field 00:05:03.520 --> 00:05:08.743 deployment tool. And that’s the thing that looks like a calculator here. 00:05:09.840 --> 00:05:14.936 It will – if you don’t have that field deployment tool, a compass 00:05:14.960 --> 00:05:19.416 is probably another thing that you need when you go out. 00:05:19.440 --> 00:05:23.760 Now, they’re very simple to turn on, and I’ll show just an example of this. 00:05:23.760 --> 00:05:28.400 With that magnet – you put that magnet in a strategic location. 00:05:28.400 --> 00:05:33.016 It’s turning on. You’re done. It’s going to record. 00:05:33.040 --> 00:05:37.200 Now, if you’re deploying a lot of these things, as I mentioned, 00:05:37.200 --> 00:05:40.616 you probably want to use this field deployment tool. 00:05:40.640 --> 00:05:45.896 It uses RFID technology to identify the node. 00:05:45.920 --> 00:05:51.200 It records wirelessly the lat, the lon, the serial numbers of the battery 00:05:51.200 --> 00:05:55.280 and of the node, the line number, etc. – most of the information you need 00:05:55.280 --> 00:05:58.776 in order to process the data in order to keep track. 00:05:58.800 --> 00:06:04.080 So you don’t need pencil and paper to decipher what instrument went where. 00:06:05.920 --> 00:06:09.040 So, it’s as simple as pushing a button, 00:06:09.040 --> 00:06:15.866 like you show here, and all that data are recorded from the instrument itself. 00:06:17.520 --> 00:06:21.040 Once you have that information when you deploy, when you come back to 00:06:21.040 --> 00:06:26.160 pick up, it’s also a very simple process. You can be 1,000 miles away and 00:06:26.160 --> 00:06:32.400 simply put in that you want to go to that site, and it will tell you the 00:06:32.400 --> 00:06:35.336 directions you need to go in order to get there. 00:06:35.360 --> 00:06:40.400 So locating the instrument is very difficult after it’s been out for 00:06:40.400 --> 00:06:44.560 a month or two or three, and there’s been rain or wind, 00:06:44.560 --> 00:06:48.560 and it’s very hard to locate the instrument. This FDT will help you 00:06:48.560 --> 00:06:55.574 do that very easily. We also have chargers and harvesters. 00:06:56.640 --> 00:07:02.080 They look like a small rolling suitcase. They’re portable. 00:07:02.080 --> 00:07:07.760 They can plug into any 110 outlet. The chargers will charge batteries 00:07:07.760 --> 00:07:12.216 in about four to six hours for a completely drained battery. 00:07:12.240 --> 00:07:21.760 And the harvesters will download 16 nodes at 20 megabytes 00:07:21.760 --> 00:07:26.056 per second per node. So they’re very efficient and very fast. 00:07:26.080 --> 00:07:32.400 So, because we have four harvesters and four chargers, that means that 00:07:32.400 --> 00:07:36.720 there can actually be four separate site investigations going on in different 00:07:36.720 --> 00:07:42.225 locations by different PIs at the same time with a subset of the nodes. 00:07:43.040 --> 00:07:45.920 This is what they look like – the harvester is on the left – 00:07:45.920 --> 00:07:50.616 when you open it up. The charger is on the right. 00:07:50.640 --> 00:07:56.480 So having these inside of a hotel room, you can do quick downloading and 00:07:56.480 --> 00:08:01.395 recharging, get your instruments back out in the field very quickly. 00:08:02.720 --> 00:08:10.536 The nodes are available to ESC scientists and collaborators to use. 00:08:10.560 --> 00:08:13.440 Whereby, they can use just a few nodes, or they can use 00:08:13.440 --> 00:08:19.576 all the nodes at the same time. And, again, we have about 500 of them. 00:08:19.600 --> 00:08:25.840 The availability can be seen at this website shown here on the right bottom. 00:08:28.960 --> 00:08:33.736 Now, one of the problems with portable seismometers in the past 00:08:33.760 --> 00:08:37.176 has been that they’re notoriously unreliable. 00:08:37.200 --> 00:08:44.696 Sometimes we have as much as 20% failure rate on the old seismometers. 00:08:44.720 --> 00:08:51.120 But these nodes are incredibly durable, as you can see from this – 00:08:51.120 --> 00:08:53.970 this is a video by SmartSolo. 00:08:54.581 --> 00:08:59.495 [banging sounds] 00:08:59.520 --> 00:09:04.800 Now, this is the tumble test. So, when they are thrown in 00:09:04.800 --> 00:09:11.096 and tumbled around, 200 rotations, you’ll see, when they come out, 00:09:11.120 --> 00:09:15.816 if they’re blinking green, that means they’re recording as they should be. 00:09:15.840 --> 00:09:20.216 They’re also – this drop test, where you see the same thing. 00:09:20.240 --> 00:09:25.630 If it blinks green, you’ve still got a good, functioning instrument. 00:09:28.489 --> 00:09:34.720 [silence] 00:09:34.720 --> 00:09:37.816 And, in this case, it blinks green. 00:09:37.840 --> 00:09:41.816 There are also optional external batteries. 00:09:41.840 --> 00:09:45.760 Like I said, the typical node will record for about a month to – 00:09:45.760 --> 00:09:51.256 about 30 days to 40 days in the field, just on the internal battery. 00:09:51.280 --> 00:09:55.120 But if you want to record for, say, three or four months, you can buy 00:09:55.120 --> 00:09:58.400 these external batteries that are attached – they can buried 00:09:58.400 --> 00:10:02.856 with the node, or they can be set on the ground surface. 00:10:02.880 --> 00:10:06.742 very convenient for a little bit longer-term recording. 00:10:07.600 --> 00:10:11.280 I’m going to show an example of a passive and an active study 00:10:11.280 --> 00:10:14.936 that we’ve done using the nodes. Here is from Ridgecrest, 00:10:14.960 --> 00:10:20.376 where deployed 461 nodes occupying 575 sites. 00:10:20.400 --> 00:10:26.616 We got them out the day after the major earthquake – the 7.1, 00:10:26.640 --> 00:10:29.576 and they recorded for about two months. 00:10:29.600 --> 00:10:35.120 We have 12 linear fault-crossing arrays and 2 two-dimensional arrays – 00:10:35.120 --> 00:10:39.440 one across the Garlock, one across the major seismicity, which you can 00:10:39.440 --> 00:10:43.496 see here. Here’s the major seismicity shown in white. 00:10:43.520 --> 00:10:49.976 We recorded about 14 terabytes of data during that time, and again, 00:10:50.000 --> 00:10:53.760 we recorded – at least the network reported 00:10:53.760 --> 00:11:00.856 30,000 earthquakes shown here. And we were able to record that. 00:11:00.880 --> 00:11:05.256 Here is an example of a single station and a linear array. 00:11:05.280 --> 00:11:11.736 And for the three components of those from the Ridgecrest nodal data. 00:11:11.760 --> 00:11:21.840 We also conducted some studies whereby we conducted 00:11:21.840 --> 00:11:23.976 guided wave studies. 00:11:24.000 --> 00:11:29.656 On the right shown here is our linear array across the fault trace. 00:11:29.680 --> 00:11:35.016 These yellow dots show where geologists mapped the faults. 00:11:35.040 --> 00:11:37.976 And the red lines show those as well. 00:11:38.000 --> 00:11:43.440 And, when we project those locations onto a plot of PGV versus 00:11:43.440 --> 00:11:45.520 the station locations, we see we get these 00:11:45.520 --> 00:11:50.776 prominent peaks where the two faults were met. 00:11:50.800 --> 00:11:56.160 We also get a small peak in between, suggesting that there’s another fault 00:11:56.160 --> 00:12:01.656 in the shallow subsurface that didn’t make it to the surface. 00:12:01.680 --> 00:12:05.440 So we found, from many studies, that this is a very convenient way 00:12:05.440 --> 00:12:09.840 to precisely map exactly where the faults are located. 00:12:11.680 --> 00:12:16.696 Another study that was done using the nodal data was by White et al. 00:12:16.720 --> 00:12:22.240 And here, using the nodal data – remember I said the network 00:12:22.240 --> 00:12:27.280 located 30,000 earthquakes. Well, we were able to re-locate 00:12:27.280 --> 00:12:33.848 approximately 95,000 earthquakes in this area, and much more precisely. 00:12:35.600 --> 00:12:40.616 And, from that, we were able to develop a 3D tomography model 00:12:40.640 --> 00:12:48.320 for the – both P and S for the region. Just an example to look, here is 00:12:48.320 --> 00:12:54.880 a slice at 12 kilometers’ depth comparing the new model with the 00:12:54.880 --> 00:12:58.000 SCEC Community Velocity Model, and you see there’s much more 00:12:58.000 --> 00:13:00.880 resolution on the new model using the nodal data. 00:13:04.080 --> 00:13:07.760 We’ve also conducted a number of active-source surveys, 00:13:07.760 --> 00:13:11.096 mainly for site characterization and guided wave studies, 00:13:11.120 --> 00:13:17.328 but also some noise studies using the nodes. 00:13:18.000 --> 00:13:25.736 So, in summary, ESC has a new nodal seismometer facility. 00:13:25.760 --> 00:13:31.336 We have about 500 three-component nodes and auxiliary equipment. 00:13:31.360 --> 00:13:35.496 The nodes are available to ESC scientists and their collaborators. 00:13:35.520 --> 00:13:40.296 And the node schedule is available at the website shown here. 00:13:40.320 --> 00:13:45.040 If you want to use any of the nodes, you should contact someone from 00:13:45.040 --> 00:13:52.056 the Nodal Committee, and those people are shown here below. 00:13:52.080 --> 00:13:54.520 Thank you very much. 00:13:55.710 --> 00:13:59.148 [silence]