Download Volume II Accomplisments (28 Mb pdf). - IRIS
Download Volume II Accomplisments (28 Mb pdf). - IRIS
Download Volume II Accomplisments (28 Mb pdf). - IRIS
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Velocity Structure of the Western US from Surface Wave Phase<br />
Velocity Measurements<br />
Anna Foster (LDEO, Columbia University), Göran Ekström (LDEO, Columbia University), Vala Hjörleifsdóttir (Instituto<br />
Geofísica, UNAM)<br />
Knowledge of the velocity structure of the crust and upper mantle can improve source studies and aid investigations into<br />
mantle dynamics. Using an initial data set of single-station phase measurements of surface waves recorded on the USArray<br />
Transportable Array, we investigate the phase-velocity structure of the western United States at discrete periods between 25-100<br />
s using two different methods. First, we estimate the local phase velocity at a station by subdividing the array into a set of miniarrays,<br />
defined to include all stations within 2° radius of the station of interest. This is done for each event. We perform a grid<br />
search over back azimuth, and for each trial location, a phase velocity is determined in the least-squares sense that best predicts<br />
the observed phase measurements at all stations within the mini-array. The optimal local phase velocity corresponds to the back<br />
azimuth yielding the smallest misfit to the observed phase. This back azimuth also provides an estimate of the arrival angle of<br />
the energy at the mini-array. Local phase-velocity results from all events for a single station are averaged to produce the map<br />
shown in figure 1a. Our second method is based on the difference in phase anomaly between two stations that record the same<br />
event and lie roughly along the same great-circle path. The resulting phase anomaly is assigned to the inter-station path. This is<br />
done for all events, and data comprised of the median measurement for each path are inverted to obtain a velocity map at a given<br />
period. These results can be further improved by correcting for the estimated arrival angle of the wave energy, since off-greatcircle<br />
arrivals bias the two-station method to higher velocities. We calculate the arrival angle using the previously described<br />
method. The arrival angle is used to correct the inter-station distance to which the two-station phase anomaly is assigned prior<br />
to inversion, resulting in a small change in the final velocity (up to 2%). This correction has been done for the inversion results<br />
shown in figure 1b. Most anomalies observed in both models correspond with well-known geologic features. The strong similarities<br />
between these two maps indicate that the methods are robust, and provide encouragement for the ongoing investigation<br />
into earth structure.<br />
Acknowledgements: This work is funded by NSF award EAR-0952<strong>28</strong>5 under the EarthScope program.<br />
Figure 1: Phase velocity maps for Rayleigh waves at 25 s period. a) Averaged local phase velocity estimates from the mini-array method. b) Results of the inversion of<br />
two-station phase anomaly measurements that were corrected for the wave’s arrival angle.<br />
2010 <strong>IRIS</strong> Core Programs Proposal | <strong>Volume</strong> <strong>II</strong> | Upper Mantle Structure and Dynamics | <strong>II</strong>-171