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• W2340647231 abstract "Abstract We have examined the historical seismicity of the Mexicali-Imperial Valley. Since about 1850, the largest observed earthquake in the area has been the magnitude ( M w ) 7.1 December 1934 event. The magnitude distribution for large plate-boundary rupturing earthquakes ( M > 5.8) is not well fit by the Gutenberg-Richter type ( b value) model. Models which better fit the observed magnitude distribution are derived from a lognormal distribution of stress drops on faults of constant size and from an exponential distribution of rupture lengths, as might be expected from randomly distributed rupture-stopping asperities along the length of the fault. This may be among the best data in the world for testing earthquake recurrence models (e.g., time predictability, slip predictability) on a strike-slip fault, but the uncertainties are still too great to permit a unique interpretation." @default.
• W2340647231 created "2016-06-24" @default.
• W2340647231 creator A5029296476 @default.
• W2340647231 creator A5075599701 @default.
• W2340647231 date "1987-04-01" @default.
• W2340647231 modified "2023-09-24" @default.
• W2340647231 title "Earthquake recurrence models and historical seismicity in the Mexicali-Imperial Valley" @default.
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• W2340647231 doi "https://doi.org/10.1785/bssa0770020562" @default.
• W2340647231 hasPublicationYear "1987" @default.
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