TY - JOUR
T1 - The ionospheric anomalies prior to the M9.0 Tohoku-Oki earthquake
AU - Le, Huijun
AU - Liu, Libo
AU - Liu, Jann Yeng
AU - Zhao, Biqiang
AU - Chen, Yiding
AU - Wan, Weixing
N1 - Funding Information:
The authors are grateful to the IGS community for providing global TEC maps. This research was supported by the Special Fund for State Seismology Bureau (Grant No. 201008007 ) and National Natural Science Foundation of China ( 41004069 ), National Key Basic Research Program of China ( 2012CB825604 ), and China Postdoctoral Science Foundation funded project ( 20090460045 ).
PY - 2013/1/30
Y1 - 2013/1/30
N2 - The GPS total electron content (TEC) data were used to investigate the ionospheric abnormal behaviors prior to the 2011 Tohoku-Oki earthquake. The observations show a significant enhancement in TEC on March 8, 2011, and during the same period the solar activity also has a large increase. Both an empirical model and a theoretical model were used to check whether the TEC anomalies were entirely contributed by the increase in solar radiation. The comparison between the observations and the simulation results shows that only the solar radiation enhancement was not enough to produce the observed significant TEC enhancement. It means that some additional mechanisms, such as the per-earthquake ionospheric disturbance or the geomagnetic activities, may play a significant role in the significant TEC enhancement on March 8. The temporal-spatial distribution of the extreme TEC enhancement within 30. days before the earthquake was particularly pursued. It is found that the extreme enhancement was persistently located in the region adjacent to the epicenter and the magnetic conjugate point for a long time of 16. h. In addition, a geomagnetic disturbance with Kp. =4 occurred on March 7. Therefore, the significant TEC enhancement on March 8 might be related to the M9.0 Tohoku-Oki earthquake and the geomagnetic disturbance.
AB - The GPS total electron content (TEC) data were used to investigate the ionospheric abnormal behaviors prior to the 2011 Tohoku-Oki earthquake. The observations show a significant enhancement in TEC on March 8, 2011, and during the same period the solar activity also has a large increase. Both an empirical model and a theoretical model were used to check whether the TEC anomalies were entirely contributed by the increase in solar radiation. The comparison between the observations and the simulation results shows that only the solar radiation enhancement was not enough to produce the observed significant TEC enhancement. It means that some additional mechanisms, such as the per-earthquake ionospheric disturbance or the geomagnetic activities, may play a significant role in the significant TEC enhancement on March 8. The temporal-spatial distribution of the extreme TEC enhancement within 30. days before the earthquake was particularly pursued. It is found that the extreme enhancement was persistently located in the region adjacent to the epicenter and the magnetic conjugate point for a long time of 16. h. In addition, a geomagnetic disturbance with Kp. =4 occurred on March 7. Therefore, the significant TEC enhancement on March 8 might be related to the M9.0 Tohoku-Oki earthquake and the geomagnetic disturbance.
KW - Ionosphere
KW - Seismo-ionospheric anomaly
KW - Total electron content
UR - http://www.scopus.com/inward/record.url?scp=84872777011&partnerID=8YFLogxK
U2 - 10.1016/j.jseaes.2012.10.034
DO - 10.1016/j.jseaes.2012.10.034
M3 - 期刊論文
AN - SCOPUS:84872777011
SN - 1367-9120
VL - 62
SP - 476
EP - 484
JO - Journal of Asian Earth Sciences
JF - Journal of Asian Earth Sciences
ER -