Finite strain and rotation from fault-slip data

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Abstract

The moment tensor summation (MTS) characterizes the infinitesimal strain of a region due to fault rupture during an earthquake. Tectonic strain on a much longer time scale can be found by applying the MTS to fault-slip data, which represent cumulative fault displacement. However, the traditional MTS assumes infinitesimal strain, which may not be appropriate for cumulative displacement on faults. Therefore, it is necessary to examine whether a finite strain treatment is more appropriate. We develop a method to find finite strain from fault-slip data (FSFS) and use it to illuminate two general faulting problems: finite strain and block rotation.

First, the FSFS method is compared to the MTS using both synthetic and real fault data. Strain due to faults must be high (> 60% elongation) before the infinitesimal strain approximation produces errors greater than the variation of typical field data. However, some regions do exhibit very high fault strains and require finite strain analysis.

Second, the FSFS method is used to solve for rotation in regions cut by domino-style faults, a common model for high fault strains and rotation. Given an arbitrary rigid boundary, the method can be used to relate fault strain and block rotation. For example, a paleomagnetic rotation of 40° requires fault strain with a minimum finite elongation of 41%.

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