Environmental controls on the evolution of alluvial fans in Buena Vista Valley, North Central Nevada, during late Quaternary time
Introduction
Alluvial fan stratigraphy, sedimentology, and geomorphology are governed by a hierarchy of environmental factors, including climatic regimes and their variation, rates and styles of tectonic activity, lithology and geomorphology of the upland source area, and the nature of contiguous environments Bull, 1977, Bull, 1991, Wells et al., 1987, Wells et al., 1997. These factors, particularly, climate and tectonics, force a dynamic interplay between energy and mass availability in the source area and mass transfer to the alluvial fan. This interplay is further complicated by its variability over time and space, perhaps best illustrated by the role climate plays in the aggradation of Quaternary alluvial fans. In presently arid climates, sediment mantles hillslopes during wetter and/or cooler regimes, but is transferred to the fan during transitions to drier and/or warmer, arid regimes (e.g., Wells et al., 1987, Bull, 1991). In contrast, in basins presently located in semiarid climates, sediment is transferred to the fan during wetter and/or cooler regimes (e.g., Pierce and Scott, 1982, Ritter et al., 1993). Although climate is used in the preceding illustration, disagreement exists as to whether climate or tectonics is the primary regulator of mass availability in the source area and mass transfer to the alluvial fan (e.g., DeCelles et al., 1991, Ritter et al., 1995). We believe this disagreement reflects, in part, the historical development of geomorphic inquiry as it relates to alluvial fans as well as discipline-based differences in time and space scales of fan studies.
Early studies of Quaternary alluvial fans were conducted in tectonically active areas (e.g., Eckis, 1928). Most were descriptive in nature and emphasized the role of faulting in initiating erosion in the source area and the aggradation of fans (e.g., Davis, 1905, Blissenbach, 1954). Later, more quantitative studies related tectonism to fan morphology, including segmented radial fan profiles Beaty, 1961, Bull, 1964a, incision of the fan-head Denny, 1967, Hooke, 1967, and the development of complex fans Denny, 1967, Bull, 1977. More recently, tectonism has been considered a first-order control on the creation of accommodation space and energy for the fan system (Fraser and DeCelles, 1992). Alluvial architecture DeCelles et al., 1991, Fraser and DeCelles, 1992 and facies assemblages Blair and McPherson, 1994a, Blair and McPherson, 1994b of alluvial fans have also been described in terms of stages of the evolution of drainage basins following uplift. These more recent studies address fan deposition on time and space-scales appropriate to basin evolution.
The role of climate in the formation of alluvial fan has generally been considered from two perspectives; the first treats the landform as a function of the climate in which it occurs, whereas the second focuses on the paleoclimatic history of the landform. Kochel and Johnson's (1984; Table 1) review of the literature of alluvial fans in various climatic regimes provides a summary of the differences existing in fan morphology, sedimentology, depositional processes, and facies assemblages. This approach is particularly valid in settings where most or all of the surface of the fan is activated by events of moderate to high recurrence (100's of years to seasonal), such as those that occur in humid-alpine climates by catastrophic floods (e.g., Blair, 1987), humid-temperate climates by debris flows (e.g., Wells and Harvey, 1987), and humid-glacial climates by seasonal meltwater (e.g., Boothroyd and Ashley, 1975). The latter historical approach is based on earlier studies which suggested that climatic changes would induce changes in mass availability and mass transfer processes (e.g., Blissenbach, 1954, Bull, 1964b, Lustig, 1965, Bull and Schick, 1979). Such changes would necessarily be widespread and characterized by synchronous periods of aggradation and entrenchment for all fans in a region of uniform environmental factors. With regionally correlative geomorphic surfaces and either absolute-age or relative-age control on those surfaces, more recent fan studies have demonstrated a temporal link between the aggradation of fans and past climates or climatic changes (e.g., Williams, 1970, Wasson, 1977, Pierce and Scott, 1982, Wells et al., 1987, Nemec and Postma, 1993, Ritter et al., 1993, Ritter et al., 1995).
The other three environmental factors affecting alluvial fans, lithology and geomorphology of the source area and the nature of contiguous environments, are generally believed to be subordinate factors. Lithology and geomorphology of the upland source area control various aspects of fan morphology, including size and slope of the fan (e.g., Bull, 1962, Bull, 1977, Hooke and Rohrer, 1977). The drainage basin, mountain front, adjacent fan surfaces, and either axial streams or basins along the distal margins of the fan comprise the contiguous environments of the alluvial fan. Of these, the distal environment of the fan, particularly, as it controls base level of the fan, has received the most attention. Entrenchment of fans and the resultant production of secondary fans have been attributed to lowering the base level (e.g., Eckis, 1928, Blissenbach, 1954, Carryer, 1966, Ryder, 1971). Base-level lowering along the distal fan margin locally oversteepens the fan-channel slope, causing the fan channel to entrench in an upfan direction.
This study evaluates the relative influences of the environmental factors on the evolution of alluvial fans in Buena Vista Valley, north-central Nevada (Fig. 1). We selected this basin because the presently arid climatic regime of the basin had been wetter and/or cooler during the late Pleistocene. Rates and styles of tectonic activity, source area lithology, and distal-fan base level vary along the perimeter of the basin. In addition, the well-exposed stratigraphic relations between the alluvial fan deposits, shoreline features and deposits associated with paleolakes, and faults provide at least a relative temporal framework for evaluating the relationship between fan process, climatic change, and tectonic activity. The objectives of this study include: (1) delineating the surficial stratigraphy of the alluvial fan deposits; (2) relating the stratigraphy of alluvial fans to geomorphic features and deposits associated with the climatic and tectonic history of the basin; (3) establishing a temporal framework for the stratigraphy and comparing it to that developed regionally by Hawley and Wilson (1965); and, (4) examining the driving forces of aggradation and entrenchment on alluvial fans in Buena Vista Valley. If a causative link indeed exists between the activity of Quaternary alluvial fans and either tectonics or climate, this study has important implications for using alluvial fans in reconnaissance studies as a first-order indicator for either tectonic activity or climatic change.
Section snippets
Description of the study region
Buena Vista Valley is located in southwestern Pershing County, NV, in the Basin and Range province of the western United States (Fig. 1). This north-trending basin is bordered on the west by the Humboldt Range and on the east and southeast by the East and Stillwater Ranges, respectively Fig. 1, Fig. 2. These ranges are east tilting, bounded on their western margins by active faults (Wallace, 1987). Extension during the past 14 Ma. (Zoback and Thompson, 1978) has produced range bounding, normal
Methodology
The location and extent of 10 alluvial fans in Buena Vista Valley have been mapped from air photographs onto orthophotoquad and topographic basemaps at a scale of 1:24,000. Morphometric properties of the fans and the respective drainage basins have been derived from these maps by digitization. The fans are composed of three to four mappable, time-stratigraphic units. The stratigraphy has been defined on the basis of topography, stratigraphic relationships, development of soil profiles, and
Results
The alluvial fans in the study area exhibit the characteristic fan shape in proximal fan areas but coalesce to form an alluvial slope (after Hawley and Wilson, 1965) along most distal margins of the fans. The area of fan range from approximately 13 to 40 km2 and increase with size of the source area (Fig. 4a). Radial fan slopes decrease downfan forming a concave-up profile (Fig. 5). The average slope of the radial fan profile, measured over the entire length of the profile, decreases with size
Discussion
The geomorphology and stratigraphy of fan deposits and the relation to deposits or features of contiguous environments indicate similar styles and synchronous periods of aggradation, entrenchment, and reworking on alluvial fans in Buena Vista Valley. In particular, units Qf2 and Qf3 dominate these fans and characterize a sequence of aggradation, entrenchment and reworking of fan deposits that we will use to evaluate the environmental controls on the evolution of fans.
Conclusions
Alluvial fans in Buena Vista Valley, north-central Nevada, formed during synchronous periods of aggradation, stability, and entrenchment in the late Quaternary. They are composed of four fan-stratigraphic units: Qf1, Qf2, Qf3, and Qf4, from oldest to youngest. Units Qf2, an early late-Pleistocene aggradational fan, and Qf3, a late Pleistocene–Holocene secondary fan, dominate the fan complexes. The timing and stratigraphic relation of Qf3 to remnant beach ridge deposits of pluvial Lake Lahontan
Acknowledgements
This work was supported by a cooperative agreement between the Desert Research Institute (Miller) and DOE (DE-DCO-93NV11417); however, such support does not constitute an endorsement by DOE of the views expressed in this article. In addition, Ritter gratefully acknowledges support from the Department of Geology and Faculty Research Fund Board at Wittenberg University and the capable field assistance of Christopher Coonfare. The quality of the manuscript was significantly improved by the
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2018, Sedimentary GeologyCitation Excerpt :The combination of these morphodynamic characteristics may lead to different sediment transport processes from basin to fan. There are colluvial fans dominated by mass transport processes with greater participation of gravity (debris flow) and debris cones (Chamyal et al., 1997; Blair and McPherson, 1998; Blikra and Nemec, 1998; Blair, 1999b, 1999c; Nemec and Kazanci, 1999; Harvey, 2011; Kochel and Trop, 2012) and also fans dominated by sheetfloods or concentrated flows (i.e., channel streams) (Blair, 1999a; Ritter et al., 2000; Nichols and Thompson, 2005; Van Dijk et al., 2012). Most fans, however, reflect a combination of both processes, but with varying contributions along different parts of the fan (Bull, 1977; Blair and McPherson, 1994).
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- 1
Present address: Department of Geosciences and Natural Resources Management, Western Carolina University, Cullowhee, NC 28723, USA.
- 2
Present address: Golder Associates, 200 Union Boulevard, Suite 500, Lakewood, CO 80228, USA.