Polarization method to detect the co-seismic magnetic oscillations

被引:8
作者
Guglielmi, A.
Hayakawa, M.
Potapov, A.
Tsegmed, B.
机构
[1] Russian Acad Sci, Inst Solar Terr Phys, Siberian Branch, Irkutsk 664003, Russia
[2] Russian Acad Sci, Schmidt United Inst Phys Earth, Moscow 123995, Russia
[3] Univ Electrocommun, Dept Elect Engn, Chofu, Tokyo 1828585, Japan
[4] Mongolian Acad Sci, Res Ctr Astron & Geophys, Ulaanbaatar 51, Mongolia
基金
俄罗斯基础研究基金会;
关键词
seismomagnetic signals; polarization method;
D O I
10.1016/j.pce.2006.02.006
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A method for detecting seismomagnetic signals is considered. These signals are generated during the course of the propagation of surface seismic Love wave from far earthquakes. Magnetic field vector of the seismomagnetic signal rotates counterclockwise and has a circular polarization, which allows us to extract the signal against the background noise. By using the described method of polarization filter the seismomagnetic signals from the earthquake on 4 June 2000 have been detected at two remote magnetic observatories. In the other case, the two signals from the disastrous tsunami 2004 earthquake were detected both for the first arrival of Love wave coming directly from the epicenter along the minor great circle arc, and for the second wave propagating along the major great circle arc. (c) 2006 Elsevier Ltd. All rights reserved.
引用
收藏
页码:299 / 304
页数:6
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