How well constrained are well-constrained T, B, and P axes in moment tensor catalogs?

被引:98
作者
Frohlich, C
Davis, SD
机构
[1] Univ Texas, Inst Geophys, Austin, TX 78759 USA
[2] Univ Colorado, NOAA, Cooperat Inst Res Environm Sci, Boulder, CO 80309 USA
[3] NOAA, Natl Geophys Data Ctr, Boulder, CO 80303 USA
关键词
D O I
10.1029/1998JB900071
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The T, B and P axes of earthquake moment tensors (MT) are often used to evaluate regional stress directions and other tectonic parameters; we here undertake three comparisons to assess the uncertainty in the orientations of these axes. These are (1) a direct comparison of common MT in the Harvard, U.S. Geological Survey, or Earthquake Research Institute (ERI) catalogs; (2) a comparison of MT slip vectors and plate motion vectors in several tectonically straightforward regions; and (3) an analysis of the axial variability in the Harvard and ERI catalogs implied by the reported uncertainties in individual MT components. All three comparisons indicate that there is considerable variability within the catalog concerning the axial orientation of MT, but all suggest that axis orientations of the majority of Harvard MT have uncertainties of 15 degrees or less. For compensated linear vector dipole (CLVD) components among the three catalogs, the correlation is very low. For the Harvard catalog, three statistics are especially useful for selecting better constrained MT; these are (1) the relative error E-rel, which is the ratio of the scalar moments of the reported error tensor and of the MT itself; (2) f(CLVD), a measure of the strength of the CLVD component; and (3) n(free), the number of MT elements not fixed at zero in the inversion. For selecting better constrained MT, the appropriate statistical cutoffs chosen depend on the problem of interest, the data available, and personal preference. However, for analysis of shallow earthquakes we have used E-rel less than or equal to 0.15, f(CLVD) less than or equal to 0.20, and n(free) = 6. While this eliminates 53% of the catalog, our calculations suggest that nearly all the remaining events have T, B, and P axes with azimuth and inclination angle uncertainties of 5 degrees-10 degrees or less.
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收藏
页码:4901 / 4910
页数:10
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