ISM Research Memorandum
No.
1073
Title:
Seismicity shadows in space-time aftershock activity
Author(s):
Ogata, Yosihiko (Institute of Statistical Mathematics)
Key words:
Aseismic slip, Coulomb failure stress, Focal mechanisms, Omori-Utsu formula, Aftershock deficit, Stress shadows
Abstract:
This paper retrospectively examines space-time aftershock coordinates before a large
aftershock that enlarges the primary aftershock region significantly, triggering a large
number of secondary aftershocks. For this analysis, the time elapsed from the main
shock is transformed using the standard aftershock decay rate in the entire aftershock
area. Here, it is assumed that, for the period until such a large aftershock, the occurrence
rates in all aftershock sub-regions obey the same Omori-Utsu function except for the
parameter K that depends only on the location. Then, in the typically normal aftershock
activity, each location should have a constant occurrence rate with respect to the
transformed time. Otherwise, there are space-time zones where the aftershocks appear
more frequently or less frequently than those are in the previous or succeeding period.
The more frequent anomaly includes secondary aftershock activity or triggered swarms.
The less frequent anomaly, which we call the seismicity shadow in this paper, indicates
aftershock deficit relative to the normal decay rate in a region and a period. We
investigate a number of recent aftershock sequences in and around Japan in conjunction
with the fault location and orientations of the focal large aftershocks. The possible cause
of the seismicity shadow of the considered aftershock activity is aseismic slip on the
large aftershock fault or its adjacent extension. According to the present case studies,
they are not only preseismic slips of the large aftershock but also postseismic slips of
the main shock.