Ophiolites, fragments of oceanic lithosphere exposed on land, are typically found as isolated klippen in intensely deformed fold-thrust belts spanning hundreds to thousands of kilometers along-strike. Ophiolites whose geochemistry indicates that they formed above subduction zones, may have been relics of larger, once-coherent, oceanic lithosphere tracts that formed the leading edge of an upper plate below which subduction occurred; such tracts were subsequently dismembered by deformation and erosion during orogenesis and uplift. However, to what extent the first-order original coherence is maintained between ophiolitic klippen is difficult to assess. Here, we aim to evaluate whether the Jurassic forearc ophiolites overlying subduction complex rocks in California, now scattered over 1000 km and dismembered by the wider San Andreas Fault Zone, still maintain their original lithospheric coherence. To this end we (i) compile available crustal ages from all ophiolite klippen exposed in the Jurassic ophiolite belt of the western United States; (ii) review and kinematically reconstruct post-middle Jurassic deformation that occurred between the modern western coast and the stable North American craton to restore the original positions of the ophiolite fragments relative to each other and to North America, and (iii) perform a paleomagnetic analysis of a sheeted dyke sections of the Mt. Diablo and Josephine ophiolites to estimate the orientation of the spreading axis at which the Jurassic Californian forearc ophiolites formed. The latter analysis reveals that the original ridge orientation likely trended ~080-260°, near-perpendicular to the orientation of the trench along the western margin of the ophiolite belt. We show that with these constraints, a straightforward ridge-transform system can explain the age distributions of the ophiolites with spreading rates of 7-10 cm/a. Our analysis shows that the Jurassic ophiolites of California may be considered klippen of a single sheet of oceanic lithosphere that accreted at a forearc spreading ridge. In addition, we show that kinematic and paleomagnetic analysis of ophiolite belts may provide novel constraints on the kinematic evolution of accretionary orogens and the plates now lost to subduction.