TY - JOUR
T1 - Statistical analysis of ULF seismomagnetic phenomena at Kakioka, Japan, during 2001-2010
AU - Han, Peng
AU - Hattori, Katsumi
AU - Hirokawa, Maiko
AU - Zhuang, Jiancang
AU - Chen, Chieh Hung
AU - Febriani, Febty
AU - Yamaguchi, Hiroki
AU - Yoshino, Chie
AU - Liu, Jann Yenq
AU - Yoshida, Shuji
PY - 2014/6
Y1 - 2014/6
N2 - To clarify and verify the ultralow frequency (ULF) seismomagnetic phenomena, we have performed statistical studies on the geomagnetic data observed at the Kakioka (KAK) station, Japan, during 2001-2010. We investigated the energy of ULF geomagnetic signals of the frequency around 0.01-Hz using wavelet transform analysis. To minimize the influences of artificial noises and global geomagnetic perturbations, we used only the geomagnetic data observed at nighttime (LT 2:30 A.M. to 4:00 A.M.) and utilized observations from a remote station, Kanoya, as a reference. Statistical results of superposed epoch analysis have indicated that ULF magnetic anomalies are more likely to appear before sizable earthquake events (Es->-108) rather than after them, especially 6-15-days before the events. Further statistical investigations show clearly that the ULF geomagnetic anomalies at KAK station are more sensitive to larger and closer events. Finally, we have evaluated the precursory information of ULF geomagnetic signals for local sizable earthquakes using Molchan's error diagram. The probability gain is around 1.6 against a Poisson model. The above results have indicated that the ULF seismomagnetic phenomena at KAK clearly contain precursory information and have a possibility of improving the forecasting of large earthquakes.
AB - To clarify and verify the ultralow frequency (ULF) seismomagnetic phenomena, we have performed statistical studies on the geomagnetic data observed at the Kakioka (KAK) station, Japan, during 2001-2010. We investigated the energy of ULF geomagnetic signals of the frequency around 0.01-Hz using wavelet transform analysis. To minimize the influences of artificial noises and global geomagnetic perturbations, we used only the geomagnetic data observed at nighttime (LT 2:30 A.M. to 4:00 A.M.) and utilized observations from a remote station, Kanoya, as a reference. Statistical results of superposed epoch analysis have indicated that ULF magnetic anomalies are more likely to appear before sizable earthquake events (Es->-108) rather than after them, especially 6-15-days before the events. Further statistical investigations show clearly that the ULF geomagnetic anomalies at KAK station are more sensitive to larger and closer events. Finally, we have evaluated the precursory information of ULF geomagnetic signals for local sizable earthquakes using Molchan's error diagram. The probability gain is around 1.6 against a Poisson model. The above results have indicated that the ULF seismomagnetic phenomena at KAK clearly contain precursory information and have a possibility of improving the forecasting of large earthquakes.
KW - Molchan's error diagram
KW - ULF seismo-magnetic phenomena
KW - statistical study
KW - superposed epoch analysis (SEA)
KW - wavelet transform analysis
UR - http://www.scopus.com/inward/record.url?scp=84904641690&partnerID=8YFLogxK
U2 - 10.1002/2014JA019789
DO - 10.1002/2014JA019789
M3 - 期刊論文
AN - SCOPUS:84904641690
SN - 2169-9380
VL - 119
SP - 4998
EP - 5011
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 6
ER -