Evidence for different scaling of earthquake source parameters for large earthquakes depending on faulting mechanism

Details Evidence for different scaling of earthquake source parameters for large earthquakes depending on faulting mechanism Evidence for different scaling of earthquake source parameters for large earthquakes depending on faulting mechanism

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000geoji.143..157s&link_type=abstract

Geophysical Journal International, Volume 143, Issue 1, pp. 157-162.

Astronomy and Astrophysics

Astronomy

5

Earthquake-Source Mechanism, Faulting, Scale Effect, Seismic Moment

Scientific paper

Scaling relationships between seismic moment, rupture length, and rupture width have been examined. For this purpose, the data from several previous studies have been merged into a database containing more than 550 events. For large earthquakes, a dependence of scaling on faulting mechanism has been found. Whereas small and large dip-slip earthquakes scale in the same way, the self-similarity of earthquakes breaks down for large strike-slip events. Furthermore, no significant differences in scaling could be found between normal and reverse earthquakes and between earthquakes from different regions. Since the thickness of the seismogenic layer limits fault widths, most strike-slip earthquakes are limited to rupture widths of between 15 and 30km while the rupture length is not limited. The aspect ratio of dip-slip earthquakes is similar for all earthquake sizes. Hence, the limitation in rupture width seems to control the maximum possible rupture length for these events. The different behaviour of strike-slip and dip-slip earthquakes can be explained by rupture dynamics and geological fault growth. If faults are segmented, with the thickness of the seismogenic layer controlling the length of each segment, strike-slip earthquakes might rupture connected segments more easily than dip-slip events, and thus could produce longer ruptures than dip-slip events of the same width

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