On January 17, 1994, the costliest earthquake in the history of the United States struck the Los Angeles region, killing 57 people, leaving 20,000 homeless, and causing more than $20 billion in damage to homes, public buildings, freeways, and bridges. This magnitude 6.7 quake occurred 10 miles beneath the town of Northridge on a previously unknown ramp-like ("thrust") fault not visible at the Earth's surface. Many faults, including such hidden or "blind" faults, in the Los Angeles region are capable of producing even stronger earthquakes.
In the aftermath of the Northridge earthquake, residents of the Los Angeles region are asking whether a strong quake can strike near their home and, if so, how hard the ground will shake. Scientists are working to answer these questions so that damage can be reduced in the next big earthquake and future quakes. A crucial step is getting an accurate picture of the network of active faults that underlie the Los Angeles region. In 1993, scientists from the Southern California Earthquake Center (SCEC), the U.S. Geological Survey (USGS), and other organizations began the Los Angeles Region Seismic Experiment (LARSE) to collect seismic images, or pictures, of the Earth's crust beneath the region. The goals of LARSE are to obtain images of faults at depth, especially of blind thrust faults, and also to obtain data on the subsurface shapes of sedimentary basins (large valleys filled with sedimentary deposits). Knowing the configuration of buried faults is crucial to understanding how the earthquake-producing "machinery" works in the Los Angeles region, and information on the thickness and shape of the region's sedimentary basins is essential for predicting how hard the ground will shake in future quakes.
LARSE uses sound waves traveling beneath the Earth's surface to produce seismic images. These sound waves are generated by underwater bursts of compressed air in the offshore region and by small underground explosions on land. The sound waves from airgun bursts and buried explosions are received by hundreds of portable recording instruments (seismographs). The recorded data are then analyzed by powerful computers to produce images of the subsurface. LARSE also makes use of seismic waves from natural earthquakes. Because the project's explosive charges are small and are set off at the bottoms of holes drilled to more than 60 feet below the ground surface, they do not cause property damage, and there is no chance of their triggering an earthquake. By 1998, the LARSE project had made several important discoveries. Images of the sedimentary basin beneath the San Gabriel Valley show that its depth reaches 3 miles, 50% more than earlier estimates. Because deeper sedimentary basins have greater shaking potential, earthquake hazards in the San Gabriel Valley need to be reevaluated.
Another major finding is a strongly reflective zone located deep beneath the San Gabriel Mountains. This zone begins at about 12 miles depth near the vertical San Andreas Fault and rises in a ramp-like fashion southward toward the Los Angeles Basin. It appears to connect to the fault system responsible for the 1987 magnitude 5.9 Whittier Narrows earthquake, which occurred on a blind thrust fault. This reflective zone is interpreted as a "master" blind thrust fault that transfers stress and strain upward and southward to a network of faults in the San Gabriel Valley and Los Angeles Basin. The LARSE data obtained so far have provided answers that could not have been obtained in any other way. The LARSE project is completing the onshore part of the second of two major lines of data collection across the Los Angeles region. This 60-mile line (Line 2) extends from the coast to the Mojave Desert. Drilling of holes for the placing of underground charges starts in the summer of 1999, and actual data collection begins in October. The LARSE project uses powerful computers to analyze transmitted and reflected underground sound waves to produce images of the Earth's crust, similar to the way in which medical CAT-scan images (transmitted X-rays) and ultrasound images (reflected sound waves) are created. Transmitted sound waves pass through the area being imaged, revealing the geologic structure by the ways they are bent or slowed. Reflected sound waves bounce off faults and rock layers, showing the shapes and depths of those features. Data collected along Line 1 of LARSE were used to create this composite image of the geologic structure beneath the Los Angeles region. Color bands in the upper part of the image, derived from computer analysis of transmitted sound waves, show the speed at which waves pass through different rock typesÑslower speeds (cooler colors) are in less dense rock. The deeper rectangular part of the image shows results from reflected sound wavesÑstrongly reflective areas are in bright red. The intensely reflective zone deep beneath the San Gabriel Mountains is interpreted by LARSE scientists as a "master" blind thrust faultÑa thrust fault that transfers stress and strain from near the San Andreas Fault to the network of faults in the San Gabriel Valley and Los Angeles Basin. The cooperative efforts of SCEC, USGS, and other scientists in the LARSE project are helping to find hidden faults and areas of potential strong earthquake shaking in the Los Angeles region. This knowledge is essential to making new and existing structures in the region better able to withstand earthquakes. The work of SCEC and USGS scientists in LARSE is only part of the National Earthquake Hazards Reduction Program's ongoing efforts to protect people's lives and property from the earthquakes that are inevitable in southern California and elsewhere in the United States. By Thomas L. Henyey, Gary S. Fuis, Mark L. Benthien, Thomas R. Burdette, Shari A. Christofferson, Robert W. Clayton, Edward E. Criley, Paul M. Davis, James W. Hendley II, Monica D. Kohler, William J. Lutter, John K. McRaney, Janice M. Murphy, David A. Okaya, Trond Ryberg, Gerald W. Simila, and Peter H. Stauffer Web design by Carolyn Donlin Graphics by Sara Boore, Susan Mayfield, and Stephen Scott COOPERATING ORGANIZATIONS
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