<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>Ray J. Weldon II</dc:contributor>
  <dc:contributor>Thomas Parsons</dc:contributor>
  <dc:contributor>Chris J. Wills</dc:contributor>
  <dc:contributor>Timothy E. Dawson</dc:contributor>
  <dc:contributor>Ross S. Stein</dc:contributor>
  <dc:contributor>Mark D. Petersen</dc:contributor>
  <dc:creator>Edward H. Field</dc:creator>
  <dc:date>2008</dc:date>
  <dc:description>This appendix discusses how we compute the magnitude and rate of earthquake ruptures for the seven Type-A faults (Elsinore, Garlock, San Jacinto, S. San Andreas, N. San Andreas, Hayward-Rodgers Creek, and Calaveras) in the WGCEP/NSHMP Earthquake Rate Model 2 (referred to as ERM 2. hereafter). By definition, Type-A faults are those that have relatively abundant paleoseismic information (e.g., mean recurrence-interval estimates). The first section below discusses segmentation-based models, where ruptures are assumed be confined to one or more identifiable segments. The second section discusses an un-segmented-model option, the third section discusses results and implications, and we end with a discussion of possible future improvements. General background information can be found in the main report.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.3133/ofr20071437G</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>U.S. Geological Survey</dc:publisher>
  <dc:title>Development of final a-fault rupture models for WGCEP/ NSHMP Earthquake Rate Model 2</dc:title>
  <dc:type>reports</dc:type>
</oai_dc:dc>