Shallow geophysical characterization of the Pahrump Valley fault zone, California-Nevada border

John Louie, Gene Ichinose, Gordon Shields, Michael Hasting

Seismological Lab (174), University of Nevada, Reno, NV 89557-0141
(775) 784-4219; fax (775) 784-1833; louie@seismo.unr.edu

Gabriel Plank, Steve Bowman

Geological Sciences (172), University of Nevada, Reno, NV 89557

Abstract

The Pahrump Valley fault zone (PVFZ) is active and represents a potential seismic hazard for Las Vegas. Combining as many as six segments over a total length of more than 100 km, the PVFZ may be able to produce a magnitude 7 event only 50 km from the metropolitan area. We employ the seismic reflection, magnetic, and electromagnetic geophysical techniques to locate segments of the PVFZ and examine their subsurface geometry. Geophysical techniques can provide clues to segmentation and rates of activity in advance of detailed trench studies, and can uncover deeper and older displacements. On the PVFZ segment in southern Pahrump Valley we can locate fault strands below three Holocene scarps with pronounced magnetic and soil conductivity anomalies. We also observe truncations and limit the vertical offsets of reflective ash beds in shallow seismic profiles across two of these scarps. The sharpness of the magnetic and soil conductivity anomalies appears to correlate with the relative geomorphic youth of the scarps. These three geophysical techniques in combination can locate faults that lack clear surface expressions. A similar study of PVFZ strands in southern Stewart Valley shows clear evidence for more than 18 m of Holocene dextral displacement in a 3-d seismic survey, but without any vertical component of displacement. The Pahrump Valley fault zone appears to have little potential for earthquake rupture-limiting segmentation anywhere in Pahrump Valley, suggesting ruptures as long as 100 km. The 18 m minimum displacement of Wisconsin and pre-Wisconsin age lacustrine formations likely results from a Holocene dextral slip rate above 0.1 mm/yr; the rate is certainly larger than 0.03 mm/yr, and probably less than 2 mm/yr.

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Objectives

We employ the seismic reflection, magnetic, and electromagnetic geophysical techniques to locate segments of the Pahrump Valley fault zone (PVFZ) and examine their subsurface geometry. Geophysical techniques can provide clues to segmentation and rates of activity in advance of detailed trench studies, and can uncover deeper and older displacements.

1) Project location map of the Pahrump Valley fault zone (PVFZ). The PVFZ is the longest seismogenic structure within 100 km of the Las Vegas metropolitan area, only 50 km distant at its closest reach. Possible rupture lengths range from 60 to 150 km, with potential for events having magnitudes between 6.9 and 7.2.

2) Shallow ground conductivity and magnetic measurements across the PVFZ in southern Pahrump Valley. Note that both types of anomaly suggest that all three scarps are fault-line scarps, with the topographic scarps having eroded back between 50 and 300 m from their respective fault traces.

3) View of southern Pahrump Valley, looking SW over scarp 1. The red line follows a tephra bed, not yet identified, exposed by headward erosion from a branch of the fault.

4) Attempts to model the magnetic anomaly at scarp 1. Model A shows a vertical fault displacement of a magnetic layer; Model B shows a magnetic body as an inclusion within the steeply-dipping fault plane. The inclusion model fits the symmetry of the anomaly better.

5) Analysis of three time-domain electromagnetic (TEM) soundings shows distinct high-conductivity layers at about 10 m depth away from the fault zone at scarp 1, with only evidence of a very shallow conductivity high at the scarp. The exposed, conductive tephra at the scarp agrees well with the coincident shallow ground conductivity high.

6) Two-dimensional seismic reflection profiles of scarps 1 and 2. The sections confirm the lack of absolute vertical offset of the lake beds and tephra layers by the PVFZ. The slumping evident in the profiles appears due to negative flower structures within the PVFZ. The scarp 2 section may suggest either substantial slumping or absolute vertical offset of more than 10 m. Note that the vertical scale bar applies only to the scarp profile.

Click on the image for a large JPEG-format enhanced air photo, or here for an annotated large JPEG photo.

7) Low-sun-angle aerial photography of the PVFZ at the southern end of Stewart Valley. The PVFZ is shown by a series of continuous scarps within 200 m of the state line. The highway running E-W across the middle of the photo is California 178/Nevada 372.

8) This section of the air photo shows the locations of our geophysical surveys in Stewart Valley. The 3-d seismic reflection survey area is outlined in yellow; shallow ground conductivity and magnetic measurements in red; and TEM measurements in blue.

9) Gravity and conductivity measurements across the PVFZ in Stewart Valley. The possible fault locations are noted on the topographic profile. Several anomalies also exist that we have not been able to associate with any fault break.

10) Stewart Valley TEM survey. No discrete conductive layers were identified, possibly due to the relatively shallow water table. At fault 2 a low-conductivity anomaly near the surface (blue) suggests abundant silica cementation within a Pluvial spring mound.

11) Ultra high-resolution three-dimensional seismic reflection surveying across fault 1 of the PVFZ in Stewart Valley. Depth imaging yielded this reflectivity volume, rendered to emphasize the positive reflectivities of greatest amplitude as opaque 3-d objects in warm colors. The front face of the image volume shows interruptions in flat reflectors between 24 and 48 m depth that locate the subsurface fault break with a near-vertical dip.

12) The upward curving of deeper reflectors near the sides of the volume is an artifact of low fold coverage there. No measurable vertical offset of any of the layers is apparent, limiting the dip slip of SVFZ fault 1 in Stewart Valley to less than one meter. The depth slice at 48 m shows the interruption of a layer by the fault trace at that depth, without vertical displacement.

13) The depth slice at 24 m shows a lateral discontinuity on the northeast side of fault 1 that could arise at a fluvial channel wall, a facies change, or the side of a Pluvial spring mound structure. The layer on the southwest side of the PVFZ fault 1 shows no similar lateral discontinuity within the image volume, proving that the discontinuity was dextrally displaced a minimum of 18 m into the image volume by PVFZ fault motion.

Conclusions

Geophysical surveys across two sections of a major right-lateral strike-slip fault zone on the California/southern Nevada border have established that the Pahrump Valley Fault Zone maintains an almost completely strike-slip character from southern Pahrump Valley to southern Stewart Valley. Despite apparent changes in tectonic setting that suggested segmentation, the PVFZ is straight, continuous, purely strike-slip, and shows Holocene activity over a distance of almost 100 km.

While this length of the fault may be a segment of a longer system possibly extending south into Mesquite Valley and north into Ash Meadows, segmentation hypotheses would propose that the main 100 km length in Pahrump Valley could rupture completely, producing an earthquake having a moment magnitude Mw as large as 7.2.

Contrary to current assessments of regional seismic hazards to the Las Vegas metropolitan area, the 18 m minimum Holocene dextral displacement found by high-resolution 3-d seismic surveying in Stewart Valley establishes a displacement rate much greater than the average for faults in southern Nevada, and likely above the 0.1 mm/yr average for faults in the Great Basin overall.

As little as 50 km from the metropolitan area, the Pahrump Valley Fault Zone could pose the most significant seismic hazard to Las Vegas after the very active 4 mm/yr Death Valley fault system.

Acknowledgments

This research was generously supported by the National Science Foundation under project EAR-9405534, by the S. F. Hunt Fund of the UNR Mackay School of Mines, and by the W. M. Keck Foundation. Electromagnetic instruments were provided by Dr. Ken Taylor of the Desert Research Institute, and by Chet Lide of Zonge Geoscience Inc. The authors acknowledge the kind assistance of the California Dept. of Transportation, Inyo County, the Nevada Dept. of Transportation, Clark County, and Nye County. Students participating in the 1994 and 1996 field exercises were David Aglietti, Kip Allander, Steve Bowman, Russell Brigham, Ryan Crosbie, Michael Hasting, Andrew Hessel, Gene Ichinose, Zakir Kanbur, Sheander Ni, Jim Ollerton, Gordon Shields, Mike Sleeman, Lorenzo Trimble, Richard Tucker, and Hongbin Zhan.


Poster presented at 1996 Fall American Geophysical Union Meeting, Dec. 17, San Francisco

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