
The rupture on a fault resulting in an earthquake is clearly a complex process. In order to better understand this process the continuum version of the slider-block model has been considered in some detail. In particular, the role of a cohesive breakaway zone is considered. Solutions of a "piston" problem and a "shock-tube" problem are obtained. For the "dirven" problem the cohesive breakaway solution is combined with a viscous resistance on the fault to obtain solutions that are reasonably realistic in terms of fault rupture.
QC801-809, Science, Physics, QC1-999, Q, Geophysics. Cosmic physics
QC801-809, Science, Physics, QC1-999, Q, Geophysics. Cosmic physics
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