Ajala, RasheedPersaud, PatriciaStock, Joann M.Fuis, Gary S.Hole, John A.Goldman, MarkScheirer, Daniel2020-06-252020-06-252019-052169-9313http://hdl.handle.net/10919/99139The Coachella Valley in the northern Salton Trough is known to produce destructive earthquakes, making it a high seismic hazard area. Knowledge of the seismic velocity structure and geometry of the sedimentary basins and fault zones is required to improve earthquake hazard estimates in this region. We simultaneously inverted first P wave travel times from the Southern California Seismic Network (39,998 local earthquakes) and explosions (251 land/sea shots) from the 2011 Salton Seismic Imaging Project to obtain a 3-D seismic velocity model. Earthquakes with focal depths <= 10 km were selected to focus on the upper crustal structure. Strong lateral velocity contrasts in the top similar to 3 km correlate well with the surface geology, including the low-velocity (<5 km/s) sedimentary basin and the high-velocity crystalline basement rocks outside the valley. Sediment thickness is similar to 4 km in the southeastern valley near the Salton Sea and decreases to <2 km at the northwestern end of the valley. Eastward thickening of sediments toward the San Andreas fault within the valley defines Coachella Valley basin asymmetry. In the Peninsular Ranges, zones of relatively high seismic velocities (similar to 6.4 km/s) between 2- and 4-km depth may be related to Late Cretaceous mylonite rocks or older inherited basement structures. Other high-velocity domains exist in the model down to 9-km depth and help define crustal heterogeneity. We identify a potential fault zone in Lost Horse Valley unassociated with mapped faults in Southern California from the combined interpretation of surface geology, seismicity, and lateral velocity changes in the model.application/pdfenCreative Commons CC0 1.0 Universal Public Domain DedicationSan Andreas faultCoachella ValleySalton TroughPeninsular RangesEastern Transverse RangesLost Horse ValleyArticle - Refereedhttps://doi.org/10.1029/2018JB01626012452169-9356