The Coso volcanic field (CVF) is situated in a tectonically complex region in southern California, bounded by the Basin and Range in the east, the Sierra Nevada block in the west, the Owens Valley in the north, and the Garlock Fault in the south (Figure 1). The CVF is well-known for its compositionally bimodal Pleistocene magmatism, represented by the coexistence of high-silica rhyolite and basalts erupted at a constant rate during the past ∼0.5 Ma (e.g., Bacon, 1982;Manley & Bacon, 2000). The evolution of the CVF is closely related to a releasing bend between the Airport Lake Fault and the Owens Valley Fault, which was developed following the earlier extensional regime introduced by the westward propagating Basin and Range extension (e.g., Duffield et al., 1980;McQuarrie & Oskin, 2010;Monastero et al., 2005). The present-day transtensional deformation results in widely distributed crustal shearing and strike-slip faulting of the brittle upper crust, leading to intensive earthquake activities in this region (Monastero et al., 2005).Geochemical and thermobarometric studies indicate the existence of a long-lasting magma reservoir beneath the CVF in the upper to middle crust, which directly feeds the Pleistocene volcanic activities and supplies the