| 2005 Salt Lake City Annual Meeting (October 16–19, 2005) | |
| Paper No. 216-10 | |
| Presentation Time: 11:05 AM-11:20 AM | ||
CLIMATE LINKAGE WITH HILLSLOPE PROCESSES, HURRICANE ESCARPMENT, NORTHWESTERN ARIZONA | ||
|
AMOROSO, Lee, Western Earth Surface Processes Team, U.S. Geological Survey, 2255 N. Gemini Drive, MS 7420, Flagstaff, AZ 86001, lamoroso@usgs.gov and MAHAN, Shannon, US Geol Survey, Box 25046 Federal Center, Denver, CO 80225 Alluvial fans, derived from Paleozoic sedimentary rock units, are common along the Hurricane escarpment. Morphology, topographic position, and soil chronosequence were used to assign ages from middle-late Pleistocene to late Holocene. Most of the Holocene fluvial and associated minor debris flow deposits consist of unconsolidated gravel and boulders with little fine materials. In contrast, the Pleistocene alluvial fans consist of debris-flow deposits with minor slopewash and stream alluvium. Pedogenic carbonate accumulation is common; a calibrated carbonate rind chronosequence was used to estimate that many surficial fan deposits are > 45 ka. The initiation of the debris-flow dominated alluvial fan deposition is probably older than ~ 75 ± 40 ka, estimated using morphologic (diffusion) modeling of a faulted late Pleistocene fan. These fans, confined to locations near the escarpment base, are composed of partly to well-consolidated deposits of gravels, cobbles, and boulders; most deposits are matrix supported. The sand-size and finer matrix materials appear to be derived from higher on the hillslope rather than weathered in place or generated during downslope transport. At approximately the Pleistocene-Holocene transition there may have been a change in transport process from dominantly debris-flow failure to fluvial. The matrix-rich debris flows may have been triggered by hillslope erosion during the wetter-to-drier climate transition. The source of this debris-flow material is weathered colluvium that likely mantled hillslopes during Pleistocene pluvial periods. The matrix-poor Holocene deposits suggest that much of this colluvial mantle was removed by the end of the Pleistocene. Buried soils (5 YR hue, silty and carbonate rich) were found overlying/within two of the five debris-flow deposits. The modern alluvium contains considerable silt and sand coming from the frequent dust-laden windstorms. Analogously, the buried soils have significant silt to very fine sand that may be of eolian origin. Others have suggested that eolian activity is related to changes in climate or sediment availability. Because the silts in the buried soil are probably eolian, Optically Stimulated Luminescence (OSL) dating is in progress to confirm the minimum age of the buried debris flow deposits. | ||
|
2005 Salt Lake City Annual Meeting (October 16–19, 2005)
General Information for this Meeting | ||
| Session No. 216--Booth# 0 Recent Advances in Numerical Dating Techniques for Developing Quantitative Chronostratigraphies in Arid and Semi-Arid Environments Salt Palace Convention Center: Ballrooms AC 8:00 AM-12:00 PM, Wednesday, 19 October 2005 Geological Society of America Abstracts with Programs, Vol. 37, No. 7, p. 480 | ||
© Copyright 2005 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions. | ||