Abstract Thorough and accurate models of modern sand sources to the Santa Monica Basin, offshore southern California, are needed to facilitate the interpretation of sediment supply to the Hueneme–Mugu Fan, the largest submarine fan within the basin. Bathymetry and near-seafloor seismic-reflection isopach mapping of basin fill indicate that dominant sources of sand are canyons/channels that enter the basin from the northwest, which are likely fed via longshore drift by the Santa Clara River and Calleguas Creek. Sand within Calleguas Creek varies in composition across its drainage basin, ranging from more quartzofeldspathic in the northeast to more volcaniclastic in the southwest, ultimately producing sand with a compositional fingerprint distinct from that of the Santa Clara River and Santa Monica Mountains. The abundance of volcanic material and lack of metamorphic grains in downstream Calleguas Creek sand stand in stark contrast to the Santa Clara River’s relatively abundant metamorphic lithic fragments. In addition, Calleguas Creek sand can be further differentiated from sand derived from both the Santa Clara River and Santa Monica Mountains because both of these other sources have much higher proportions of plagioclase. The composition of late Pleistocene (<60 ka) sandy turbidites at Ocean Drilling Program Site 1015 on the distal Hueneme–Mugu submarine fan validates Calleguas Creek’s contribution of sandy sediment to this site in the Santa Monica Basin: out of 14 samples, four samples show compositions similar to the Santa Clara River sand, whereas five are similar to Calleguas Creek sand, and six exhibit mixed compositions. There is no indication of input to this distal environment from the southern Santa Monica Mountains. Trends in sand composition within the Santa Monica Basin can be related to alternating and/or mixing of sediment sources, possibly related to sea-level change, as well as frequency of floods/storms, earthquakes, and other destabilizing processes affecting offshore shelf-to-slope regions.

Sediment discharged into the portion of the Southern California Bight extending from Santa Barbara to Dana Point enters a complex system of semi-isolated coastal cells, narrow continental shelves, submarine canyons, and offshore basins. On both the Santa Monica and San Pedro margins, 210 Pb accumulation rates decrease in an offshore direction (from ~0.5 g cm −2 yr −1 to 0.02 g cm −2 yr −1 ), in concert with a fining in sediment grain size (from 4.5φ to 8.5φ), suggesting that offshore transport of wave-resuspended material occurs as relatively dilute nepheloid layers and that hemiplegic sedimentation dominates the supply of sediment to the outer shelf, slope, and basins. Together, these areas are effectively sequestering up to 100% of the annual fluvial input. In contrast to the Santa Monica margin, which does not display evidence of mass wasting as an important process of sediment delivery and redistribution, the San Pedro margin does provide numerous examples of failures and mass wasting, suggesting that intraslope sediment redistribution may play a more important role there. Basin deposits in both areas exhibit evidence of turbidites tentatively associated with both major floods and earthquakes, sourced from either the Redondo Canyon (San Pedro Basin) or Dume Canyon (Santa Monica Basin). On the Palos Verdes shelf, sediment-accumulation rates decrease along and across the shelf away from the White's Point outfall, which has been a major source of contaminants to the shelf deposits. Accumulation rates prior to the construction of the outfall were ~0.2 g cm −2 yr −1 and increased 1.5–3.7 times during peak discharges from the outfall in 1971. The distal rate of accumulation has decreased by ~50%, from 0.63 g cm −2 yr −1 during the period 1971–1992 to 0.29 g cm −2 yr −1 during the period 1992–2003. The proximal rate of accumulation, however, has only decreased ~10%, from 0.83 g cm −2 yr −1 during the period 1971–1992 to 0.73 g cm −2 yr −1 during the period 1992–2003. Effluent-affected sediment layers on the Palos Verdes shelf can be identified in seabed profiles of naturally occurring 238 U, which is sequestered in reducing sediments. The Santa Clara River shelf, just north and west of the Santa Monica and San Pedro margins, is fine-grained and flood-dominated. Core profiles of excess 210 Pb from sites covering the extent of documented major flood deposition exhibit evidence of rapidly deposited sediment up to 25 cm thick. These beds are developing in an active depocenter in water depths of 30–50 m at an average rate of 0.72 g cm −2 yr −1 . Budget calculations for annual and 50-yr timescale sediment storage on this shelf shows that 20%–30% of the sediment discharge is retained on the shelf, leaving 70%–80% to be redistributed to the outer shelf, slope, Santa Barbara Basin, and Santa Monica Basin.

The trip commences on Lavigia Hill where we gain an overview the physiography of the Transverse Ranges and to consider the framework and petroleum activity of the Santa Barbara Channel. The route proceeds westward from Santa Barbara to active tar seeps and exposures of fractured Monterey Formation at Carpinteria. Then we visit Conoco’s San Miguelito oil field to see the magnificent anticline in the core of the field and to examine turbidite sedimentation. We cross the axis of the fabled Ventura Avenue oil field, drive through Ventura, and turn northeast on to Hwy 126 and follow the Santa Clara River Valley up to Santa Paula. There we visit Texaco’s South Mountain oil field to observe depositional features of part of the Sespe Formation in the anticline. We continue to the Bardsdale oil field to consider the unique structure of the central Ventura basin and to reflect on the early history of its exploration and development. The trip concludes at the Torrey Canyon oilfield where the remarkable geologic structure of the Ventura basin is clearly displayed.

We used tephrochronology for upper Neogene deposits in the Española Basin and the adjoining Jemez Mountains volcanic field in the Rio Grande rift, northern New Mexico, to correlate key tephra strata in the study area, identify the sources for many of these tephra, and refine the maximum age of an important stratigraphic unit. Electron-microprobe analyses on volcanic glass separated from 146 pumice-fall, ash-fall, and ash-flow tephra units and layers show that they are mainly rhyolites and dacites. Jemez Mountains tephra units range in age from Miocene to Quaternary. From oldest to youngest these are: (1) the Canovas Canyon Rhyolite and the Paliza Canyon Formation of the lower Keres Group (ca. <12.4–7.4 Ma); (2) the Peralta Tuff Member of the Bearhead Rhyolite of the upper Keres Group (ca. 6.96–6.76 Ma); (3) Puye Formation tephra layers (ca. 5.3–1.75 Ma); (4) the informal San Diego Canyon ignimbrites (ca. 1.87–1.84 Ma); (5) the Otowi Member of the Bandelier Tuff, including the basal Guaje Pumice Bed (both ca. 1.68–1.61 Ma); (6) the Cerro Toledo Rhyolite (ca. 1.59–1.22 Ma); (7) the Tshirege Member of the Bandelier Tuff, including the basal Tsankawi Pumice Bed (both ca. 1.25–1.21 Ma); and (8) the El Cajete Member of the Valles Rhyolite (ca. 60–50 ka). The Paliza Canyon volcaniclastic rocks are chemically variable; they range in composition from dacite to dacitic andesite and differ in chemical composition from the younger units. The Bearhead Rhyolite is highly evolved and can be readily distinguished from the younger units. Tuffs in the Puye Formation are dacitic rather than rhyolitic in composition, and their glasses contain significantly higher Fe, Ca, Mg, and Ti, and lower contents of Si, Na, and K. We conclude that the Puye is entirely younger than the Bearhead Rhyolite and that its minimum age is ca. 1.75 Ma. The San Diego Canyon ignimbrites can be distinguished from all members of the overlying Bandelier Tuff on the basis of Fe and Ca. The Cerro Toledo tephra layers are readily distinguishable from the overlying and underlying units of the Bandelier Tuff primarily by lower Fe and Ca contents. The Tshirege and Otowi Members of the Bandelier Tuff are difficult to distinguish from each other on the basis of electron-microprobe analysis of the volcanic glass; the Tshirege Member contains on average more Fe than the Otowi Member. Tephra layers in the Española Basin that correlate to the Lava Creek B ash bed (ca. 640 ka) and the Nomlaki Tuff (Member of the Tuscan and Tehama Formations, ca. 3.3 Ma) indicate how far tephra from these eruptions traveled (the Yellowstone caldera of northwestern Wyoming and the southern Cascade Range of northern California, respectively). Tephra layers of Miocene age (16–10 Ma) sampled from the Tesuque Formation of the Santa Fe Group in the Española Basin correlate to sources associated with the southern Nevada volcanic field (Timber Mountain, Black Mountain, and Oasis Valley calderas) and the Snake River Plain–Yellowstone hot spot track in Idaho and northwestern Wyoming. Correlations of these tephra layers across the Santa Clara fault provide timelines through various stratigraphic sections despite differences in stratigraphy and lithology. We use tephra correlations to constrain the age of the base of the Ojo Caliente Sandstone Member of the Tesuque Formation to 13.5–13.3 Ma.