WEBVTT Kind: captions Language: en-US 00:00:02.046 --> 00:00:06.160 [silence] 00:00:06.160 --> 00:00:08.640 Hi, everyone. My name is Noha Farghal. 00:00:08.640 --> 00:00:12.800 I’m a Mendenhall postdoctoral fellow at the USGS Earthquake Science Center 00:00:12.800 --> 00:00:16.720 in Moffett Field, California. Today, I will talk about the potential 00:00:16.720 --> 00:00:20.056 of fiber optic sensing in earthquake early warning. 00:00:20.080 --> 00:00:22.640 But first I would like to acknowledge and thank 00:00:22.640 --> 00:00:27.120 my collaborators, Jessie Saunders and Grace Parker. 00:00:31.440 --> 00:00:35.840 Recently, there has been a focus on using data from borehole strainmeters 00:00:35.840 --> 00:00:39.520 in earthquake early warning and creating different strain seismology 00:00:39.520 --> 00:00:44.616 tools to calculate various source and ground motion parameters from strain. 00:00:44.640 --> 00:00:49.920 Using records from the July 2019 Ridgecrest sequence magnitude 7.1 00:00:49.920 --> 00:00:54.320 main shock, we demonstrated that reliable magnitude estimates – 00:00:54.320 --> 00:00:58.480 the blue and yellow lines – can be derived from strain 00:00:58.480 --> 00:01:01.440 through this empirical relation between earthquake moment 00:01:01.440 --> 00:01:06.320 magnitudes, peak dynamic strains, and hypocentral distances. 00:01:06.320 --> 00:01:10.000 And we showed that incorporating strain would have possibly helped the 00:01:10.000 --> 00:01:14.880 ShakeAlert system reach the threshold number of stations for alerting faster 00:01:14.880 --> 00:01:20.310 and possibly contributed to a more accurate system performance. 00:01:21.920 --> 00:01:26.640 In another recent work, we derived a magnitude scale entirely based on 00:01:26.640 --> 00:01:31.576 strain data with corrections for source and site effects. 00:01:31.600 --> 00:01:35.200 Which was also tested using the Ridgecrest main shock records 00:01:35.200 --> 00:01:38.400 and further confirms the utility of strain data 00:01:38.400 --> 00:01:42.645 in providing robust strain magnitude updates. 00:01:43.680 --> 00:01:47.520 It is also worth mentioning that this strain-based magnitude scale is 00:01:47.520 --> 00:01:52.151 currently used by UNAVCO for strain magnitude estimation. 00:01:54.808 --> 00:01:58.000 [silence] 00:01:58.000 --> 00:02:02.400 We also did a proof of concept for calculating peak ground velocities, 00:02:02.400 --> 00:02:07.336 or PGVs, from strain for several recent earthquakes in California 00:02:07.360 --> 00:02:12.480 and found that strain-derived PGVs are practically indistinguishable 00:02:12.480 --> 00:02:17.440 from seismic-derived ones. And we are currently working on 00:02:17.440 --> 00:02:21.360 calculating peak ground accelerations, or PGAs, from strain. 00:02:21.360 --> 00:02:24.400 And so far, we are getting promising results comparing 00:02:24.400 --> 00:02:28.582 strain-derived and seismic-derived PGAs. 00:02:33.040 --> 00:02:36.480 In deriving all these relations, we have been using data from 00:02:36.480 --> 00:02:40.560 borehole strainmeters of the USGS, a Network of the Americas networks 00:02:40.560 --> 00:02:45.200 along the U.S. West Coast, which are sparse, and it’s quite unlikely 00:02:45.200 --> 00:02:49.200 that more such strainmeters will be installed on a large scale in the future 00:02:49.200 --> 00:02:53.709 to complement traditional seismic data in earthquake early warning. 00:02:55.200 --> 00:02:59.600 So we looked to fiber optic distributed acoustic sensing, or fiber optic DAS, 00:02:59.600 --> 00:03:05.600 for its potential for scalability, real-time telemetry, cost-effective dense sensing. 00:03:05.600 --> 00:03:10.400 It has been used for years through arrays of different sizes and layouts, 00:03:10.400 --> 00:03:16.776 vertical and horizontal arrays, for various applications all over the world. 00:03:16.800 --> 00:03:21.360 Dark-fiber-type installations also successfully recorded earthquakes 00:03:21.360 --> 00:03:25.680 with high signal-to-noise ratios, and there is a growing discussion now 00:03:25.680 --> 00:03:29.440 about how to leverage the extensive network of infrastructure 00:03:29.440 --> 00:03:33.896 subsea cables for improving offshore hazard monitoring. 00:03:33.920 --> 00:03:38.080 Google is currently working on tracking state of polarization of light 00:03:38.080 --> 00:03:41.920 to detect seismic activity over tens of thousands of kilometers 00:03:41.920 --> 00:03:47.120 using infrastructure cables. They detected the January 28th, 2020, 00:03:47.120 --> 00:03:51.440 magnitude 7.7 earthquake off of Jamaica and were able to 00:03:51.440 --> 00:03:55.496 compare their data to those from traditional seismic stations. 00:03:55.520 --> 00:03:59.360 Although this is not fiber optic DAS, I found it to be an interesting 00:03:59.360 --> 00:04:03.200 recent demonstration of the potential of infrastructure cables 00:04:03.200 --> 00:04:06.045 in hazard monitoring in general. 00:04:09.440 --> 00:04:12.480 Just a quick reminder of how fiber optic DAS works. 00:04:12.480 --> 00:04:16.800 It starts with an interrogator unit generating and sending short laser 00:04:16.800 --> 00:04:21.120 pulses down the optical fiber. Some of this energy is backscattered 00:04:21.120 --> 00:04:24.560 by the naturally occurring scatters in the fiber, which are basically 00:04:24.560 --> 00:04:28.856 imperfections or inconsistencies in the refractive index. 00:04:28.880 --> 00:04:32.160 When the backscattered energy reaches the interrogator unit, 00:04:32.160 --> 00:04:35.440 interferometry is performed, and if the fiber is subjected to 00:04:35.440 --> 00:04:40.240 some acoustic field that causes strain or deformation somewhere on the fiber, 00:04:40.240 --> 00:04:43.520 there will be a resulting phase difference between the pulses. 00:04:43.520 --> 00:04:45.600 And, depending on the optical setup, 00:04:45.600 --> 00:04:49.656 you can end up either measuring strain or strain rate. 00:04:49.680 --> 00:04:53.440 And, of course, the two-way travel time of the received pulse is used 00:04:53.440 --> 00:04:56.776 to determine the location of measurement down the fiber. 00:04:56.800 --> 00:05:02.376 This location is called channel location, or sensing point. 00:05:02.400 --> 00:05:05.920 And the length of fiber in which the strain or strain rate measurement 00:05:05.920 --> 00:05:10.800 is averaged is called the gauge length, which is typically 00:05:10.800 --> 00:05:14.696 8 to 16 meters for earthquake surface recordings 00:05:14.720 --> 00:05:19.929 and 4 to 7 meters for microseismic borehole recordings. 00:05:24.320 --> 00:05:29.336 DAS has many applications, including vertical seismic profiling; 00:05:29.360 --> 00:05:33.040 earthquake detection and monitoring; soil property estimation and 00:05:33.040 --> 00:05:36.720 hydrological characterization; structural monitoring; 00:05:36.720 --> 00:05:41.680 CO2 monitoring; hydraulic fracturing process monitoring in oil and gas plays; 00:05:41.680 --> 00:05:45.520 and long-term strain sensing, such as melting of the permafrost 00:05:45.520 --> 00:05:49.176 and oceanic properties, to mention a few. 00:05:49.200 --> 00:05:51.920 And there are many works that compare the performance of DAS 00:05:51.920 --> 00:05:56.000 to seismometers and geophones that demonstrate the good signal-to-noise 00:05:56.000 --> 00:06:00.080 ratio that DAS is capable of providing. And, while DAS measures strain 00:06:00.080 --> 00:06:04.000 or strain rate, particle velocity can be derived from DAS data 00:06:04.000 --> 00:06:06.880 if apparent slowness in the cable direction is known. 00:06:09.200 --> 00:06:12.560 It is also worth mentioning that one interrogator can be used 00:06:12.560 --> 00:06:19.016 to analyze fiber cables that are 50 or even 100 kilometers long. 00:06:19.040 --> 00:06:22.560 Moreover, an interrogator unit can be placed onshore 00:06:22.560 --> 00:06:26.000 with a marine cable or be placed underwater if needed. 00:06:29.760 --> 00:06:33.040 So now let’s think about the role that fiber optic DAS can play in 00:06:33.040 --> 00:06:37.336 enhancing the performance of various earthquake early warning systems. 00:06:37.360 --> 00:06:41.440 When it comes to earthquake locations and arrival times, the current DAS 00:06:41.440 --> 00:06:45.760 capabilities can provide high signal-to-noise ratios for accurate 00:06:45.760 --> 00:06:50.080 source location and origin time estimation, which are useful for 00:06:50.080 --> 00:06:52.640 point-source source parameter algorithms, 00:06:52.640 --> 00:06:56.383 like the ShakeAlert system EPIC algorithm. 00:06:58.800 --> 00:07:02.240 We can further enhance the signal-to-noise ratio if needed 00:07:02.240 --> 00:07:07.819 by using interrogators with higher sensitivities and lower noise floors. 00:07:08.640 --> 00:07:12.400 While data with good signal-to-noise ratios were obtained using standard 00:07:12.400 --> 00:07:18.000 telecom fibers, dedicated installations that require high fiber sensitivity and 00:07:18.000 --> 00:07:23.416 exception signal-to-noise ratios utilize special or engineered fibers. 00:07:23.440 --> 00:07:27.520 Engineered fibers provide higher backscattering capabilities without 00:07:27.520 --> 00:07:31.680 significantly increasing fiber losses, which allows for the detection of 00:07:31.680 --> 00:07:36.880 very small signals at distances of about 1 kilometer from the interrogator. 00:07:36.880 --> 00:07:42.560 They can offer 100 times’ improvement in fiber sensitivity compared to telecom 00:07:42.560 --> 00:07:47.280 fiber varieties and up to 30-decibel enhancement in noise levels. 00:07:47.280 --> 00:07:52.000 However, the cost of engineered fibers can be significantly higher than those 00:07:52.000 --> 00:07:56.480 of standard telecom fibers, which cost about $1 to 2 per meter. 00:07:56.480 --> 00:08:00.800 But we’re not considering only the fibers but the whole cable bundle – 00:08:00.800 --> 00:08:07.421 engineered fiber cables can cost up to 15 times more than telecom fiber cables. 00:08:12.080 --> 00:08:15.920 We also need to make sure that the cables are oriented in such a way 00:08:15.920 --> 00:08:21.896 as to have optimal azimuthal or directional sensitivity to P waves. 00:08:21.920 --> 00:08:26.240 So, if the fiber is oriented this way – horizontally – when a seismic wave 00:08:26.240 --> 00:08:29.840 of wavelength much longer than the gauge length propagates through the 00:08:29.840 --> 00:08:34.720 fiber, the fiber will be highly sensitive to longitudinal waves propagating 00:08:34.720 --> 00:08:40.240 along the fiber and to transverse waves at 45 degrees through the fiber. 00:08:40.240 --> 00:08:42.240 And I will show an example fiber layout 00:08:42.240 --> 00:08:45.530 for multi-components acquisition in a minute. 00:08:48.480 --> 00:08:52.880 One issue that there isn’t an update on is how a DAS array would perform 00:08:52.880 --> 00:08:57.440 when installed very close to a large rupture or a large earthquake and 00:08:57.440 --> 00:09:01.200 whether there is an equivalent of clipping in DAS systems as there is 00:09:01.200 --> 00:09:05.520 in seismometers, for example, as well as the effect of high strain 00:09:05.520 --> 00:09:09.097 and high strain rates on the fiber cables themselves. 00:09:11.040 --> 00:09:15.920 Clipping in the optical system may be thought of as a phase wraparound as a 00:09:15.920 --> 00:09:21.360 result of the signal rising too quickly. This can presumably be adjusted 00:09:21.360 --> 00:09:26.640 by pre-setting the phase quantization increment in the hardware if the 00:09:26.640 --> 00:09:31.440 expected strain rates are known. However, this increment will 00:09:31.440 --> 00:09:35.440 become a hard limit, as it is not user-selectable 00:09:35.440 --> 00:09:39.183 and will not be easy to change afterwards. 00:09:44.720 --> 00:09:47.920 When talking about P wave displacements for rapid magnitude 00:09:47.920 --> 00:09:52.400 estimation, DAS capabilities to provide good signal-to-noise ratio 00:09:52.400 --> 00:09:55.920 is well-established. But several studies show that 00:09:55.920 --> 00:10:00.000 DAS strain amplitude accuracy highly depends on the quality 00:10:00.000 --> 00:10:03.280 of strain coupling between the ground and the fiber 00:10:03.280 --> 00:10:05.884 and the conditions of the installation. 00:10:08.000 --> 00:10:12.240 For example, the top figure shows how the installation conditions, 00:10:12.240 --> 00:10:17.760 being a single conduit, a cased conduit, or an attached conduit, can affect 00:10:17.760 --> 00:10:21.576 recorded data, possibly due to variations in coupling. 00:10:21.600 --> 00:10:26.000 This work by Nate Lindsey and others shows that, while the phase response 00:10:26.000 --> 00:10:30.480 remained practically flat for the entire range of seismic frequencies they 00:10:30.480 --> 00:10:35.200 studied, there is an elevated amplitude response at higher frequencies, 00:10:35.200 --> 00:10:39.280 which the authors think might be due to coupling issues of the cable 00:10:39.280 --> 00:10:43.896 that leads to such frequency-dependent response. 00:10:43.920 --> 00:10:48.160 Even in dedicated installations, poor strain coupling has resulted 00:10:48.160 --> 00:10:51.840 in mismatches between DAS data and co-located geophones 00:10:51.840 --> 00:10:55.976 and uncemented fiber segments were thought to be problematic. 00:10:56.000 --> 00:11:00.160 A few studies of cable packaging have shown some minor differences in 00:11:00.160 --> 00:11:03.840 cable response compared to the more prominent effect of 00:11:03.840 --> 00:11:08.000 the strength of strain coupling. So this is also a need for further 00:11:08.000 --> 00:11:11.920 research for different array installations and to investigate 00:11:11.920 --> 00:11:15.120 whether infrastructure or dark fiber installations 00:11:15.120 --> 00:11:19.286 would be suitable for earthquake early warning applications. 00:11:21.040 --> 00:11:25.440 PGVs or PGAs used in ground motion-based finite fault parameter 00:11:25.440 --> 00:11:29.920 estimation algorithms, such as FinDer, or wavefield propagation algorithms 00:11:29.920 --> 00:11:34.776 such as PLUM, can be derived from dynamic strains. 00:11:34.800 --> 00:11:38.720 But they additionally require multi-component DAS acquisition, 00:11:38.720 --> 00:11:42.536 which can be achieved with helically wound fibers. 00:11:42.560 --> 00:11:47.200 And you can reconstruct the full strain tensor from this layout of five helically 00:11:47.200 --> 00:11:51.256 wound fibers and one straight fiber that isn’t shown in the figure. 00:11:51.280 --> 00:11:55.040 And it’s been confirmed in field tests that at least the P wave response 00:11:55.040 --> 00:11:59.280 of the cable was angle independent. I know the cable looks large in the 00:11:59.280 --> 00:12:03.120 figure, but the next-generation cables have diameters as small as 00:12:03.120 --> 00:12:07.360 1.8 centimeter, and you can get multi-component response 00:12:07.360 --> 00:12:09.840 without complicated layouts. 00:12:14.400 --> 00:12:18.560 Finally, since we derived a number of useful relations between dynamic 00:12:18.560 --> 00:12:22.160 strains and earthquake magnitudes and ground motion parameters, 00:12:22.160 --> 00:12:26.240 if at some point in the future, we can develop a new algorithm 00:12:26.240 --> 00:12:30.400 based on strain data from fiber optic sensors or strainmeters, 00:12:30.400 --> 00:12:33.920 it can be used for calculating different earthquake source parameters 00:12:33.920 --> 00:12:37.440 and ground motion metrics directly from strain and sent to 00:12:37.440 --> 00:12:38.960 the earthquake early warning system. 00:12:41.731 --> 00:12:45.760 [silence] 00:12:45.760 --> 00:12:49.360 In summary, there are many ways that DAS data can contribute to 00:12:49.360 --> 00:12:52.720 different types of earthquake early warning algorithms through 00:12:52.720 --> 00:12:56.640 contributing ground motion observations directly to existing 00:12:56.640 --> 00:13:00.800 earthquake early warning algorithms after conversion to the data types 00:13:00.800 --> 00:13:04.880 ingested by these algorithms and through augmenting the current 00:13:04.880 --> 00:13:08.720 earthquake early warning systems by supplying additional earthquake source 00:13:08.720 --> 00:13:14.790 parameters through the development of an independent strain-based algorithm. 00:13:16.160 --> 00:13:20.400 In our upcoming paper, we highlighted a few DAS-related issues in need 00:13:20.400 --> 00:13:24.080 of further investigation, such as amplitude accuracy 00:13:24.080 --> 00:13:27.520 in weak or non-uniform coupling installations and 00:13:27.520 --> 00:13:31.719 array performance very close to large ruptures. 00:13:34.240 --> 00:13:38.480 I would like to thank Martin Karrenbach, Sarah Minson, 00:13:38.480 --> 00:13:44.456 Andrew Barbour, Scott DeWolf, Evelyn Roeloffs, John Lanbein, Julian Bunn, 00:13:44.480 --> 00:13:48.320 and Elizabeth Cochran for their feedback and help with this work. 00:13:48.320 --> 00:13:50.880 And, with that, I thank you very much for your attention, 00:13:50.880 --> 00:13:54.440 and I look forward to your questions and the discussion. 00:13:56.624 --> 00:14:02.340 [silence]