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Figure 5. Map of California showing locations of the three OHV pilot study areas and other OHV areas where site visits were made during development of the updated standard/guidelines. Hollister Hills SVRA is underlain primarily by Tertiary-age fine-grained sandstone, siltstone, and shale in fault contact with older granite and schist typical of the Coast Ranges. The Foresthill OHV area is composed of a variety of Sierra Nevada rock formations, including Tertiary volcanics, metamorphosed sedimentary rocks, serpentinite, and other ultramafic rocks. The Dove Springs OHV Area is underlain predominantly by erodible Quaternary alluvial fan deposits, tuffs, and volcanic mudflows in a semi-arid desert environment. Other sites visited by CGS included a diverse set of ecosystems with multiple soil and vegetation types representative of the state's complex topographic, geologic, and climatic framework. (Graphics by Mel Patel)
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