seismic refraction analysis of california wash and astor pass
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Seismic Refraction Analysis of California Wash and Astor Pass. Stephen Hein Mason Kreidler. Overview. Project Objectives Field methods Analyses Interpretations Discussions. Project Objectives. California Wash - PowerPoint PPT PresentationTRANSCRIPT
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Seismic Refraction Analysis of California Wash and Astor Pass
Stephen HeinMason Kreidler
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Overview Project Objectives Field methods Analyses Interpretations Discussions
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Project Objectives California Wash
Analyze the fault running through California Wash, to evaluate seismic hazards for Las Vegas
Astor Pass Examine regions that were not previously
drilled, to see if more promising geophysical prospects exist
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Equipment: All lines 7 kg sledgehammer
Seismic source
100 Hz Geophones Seismic vibration monitor
Seismic cable with 48 channel Data transfer
Bison Galileo-21 Data logger
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Analysis: All lines First arrival picks using Viewmat
Better images through Band-Pass filters, TEGain,
Simple calculations using a time-distance plot in excel V1 and V2 velocities: Refractor depth: Dip angle Estimated low and high velocities Possible third layers
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Analysis: All lines Dr. Pullammanappallil created P-wave seismic
velocity sections from our first-arrival pick times using SeisOpt® @2D ( 2011 Optim) Cross Section with velocities
Refractor depths Layer velocities
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Seismic cable oriented East-West with a total length of 100 meters 2 meter spacing between each takeout
6 geophones per takeout oriented parallel to the seismic cable
Sledgehammer hits used to propagate waves into the ground 10 hammer hits at each source point A total of 74 source points were taken
14 to the East of the first geophone at a spacing of 4 meters 48 at each channel along the line 12 to the West of the last geophone at a spacing of 4 meters
Total length of hammer hits: 200 meters
Field Methods: California Wash Line
1
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Layout of seismic cable and geophones (Louie, 2011)
Producing waves using a sledgehammer and layout of
geophones (Louie, 2011
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Results: California Wash Line 1
V1: 666-1104.7 m/s with an average of 885.4 m/s
V2: 1301.2 m/s Refractor depth
between 2.4-15 m Dip angle of 1.3
degrees
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Optim's SeisOpt®@2DTM Results: California Wash Line 1
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SeisOpt®
Interpretation: California Wash Line1 P-Wave velocity was 600-900 m/s, consistent
with simple calculations average of 880 m/s V2 of ~ 1400 m/s consistent with simple
calculations Estimated refractor depth of 1-10 m, also
consistent Very low eastward dip in first refractor
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Seismic cable oriented East-West with a total length of 48 meters 1 meter spacing between each takeout
6 geophones per takeout oriented perpendicular to the seismic cable
Sledgehammer hits used to propagate waves into the ground 10 hammer hits at each source point A total of 48 source points were taken
48 at each channel along the line Total length of hammer hits: 48 meters
Field Methods: California Wash Line
2
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Example of geophone arrangement and wave propagation at line 2 (Louie, 2011)
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Results: California Wash Line 2
V1: 216.7-326.1 m/s with an average of 271.4 m/s
V2: 1274.5 m/s Refractor depth
between 0.69-0.90 m
Dip angle of 0.24 degrees
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Optim's SeisOpt®@2DTM Results: California Wash Line 2
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SeisOpt®
Interpretation: California Wash Line2 P-Wave velocity was 200-400 m/s, consistent
with simple calculations average of 270 m/s V2 of ~ 1200 m/s consistent with simple
calculations Estimated refractor depth of 1-2 m, slightly
higher than estimated in simple calculations Minimal evidence of any dip in the first
refractor
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Interpretation of California Wash Lines 1
and 2 Conformation of good results by overlaying CW2 onto CW1
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Discussion: California Wash Lines 1 and 2
Results from Line 1 give a good indication of the dip of the fault running through the wash
Line 2 shows evidence of the amount of slip that occurred that last time on this fault, by the amount of recent, slower velocity, sediment on top of older, higher velocity alluvium
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Seismic cable oriented East-West with a total length of 144 meters 3 meter spacing between each takeout
6 geophones per takeout oriented parallel to the seismic cable
Sledgehammer hits used to propagate waves into the ground 10 hammer hits at each source point A total of 60 source points were taken
48 at each channel along the line 12 to the West of the last geophone, at a spacing of 6 meters
Total length of hammer hits: 220 meters
Field Methods: Astor Pass
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Layout of seismic cables and geophones at Astor Pass
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Results: Astor Pass V1 of 275-400 m/s with
an average of 337.5 m/s
V2 of 1090 m/s
Refractor depth between 15-30 m
Dip angle of 1-5 degrees 0 20 40 60 80 100 120 140 1600.00
0.05
0.10
0.15
0.20
0.25
0.30
Source Downdip TimesSource Updip TimesDowndip Source
Receiver X Coordinate, meter
Tim
e, s
econ
d
Astor Pass Time-Distance plot
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Optim's SeisOpt®@2DTM Results: Astor Pass
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SeisOpt®
Interpretation: Astor Pass P-Wave velocity was 300-400 m/s, consistent
with simple calculations of 275-400 m/s V2 of ~ 1000 m/s consistent with simple
calculations of 1090 Estimated refractor depth of 12-16 m, also
consistent with previous calculations No dip in first refractor
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Basic Interpretation
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Discussion: Astor Pass
Results from SeisOpt® did not agree with the hypothesis of seeing faster velocities near the middle of the plot where tufa layers were thought to exist.
These results actually lean towards a hypothesis that most if not all of the tufa is already on the surface.
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Possible Sources of Errors
Wind creating noise on the seismic line. People walking around on the seismic line
while recording data. First arrival picks may have been off slightly;
however, refractor depth and data was consistent throughout the plot, suggesting picks were valid.
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Conclusion of Astor Pass Refraction Microtremor results agreed with
our Refraction results of not seeing faster velocities near the tufa mounds.