Source complexity of the 2016 MW7.8 Kaikoura (New Zealand) earthquake revealed from teleseismic and InSAR data

被引:0
|
作者
HaiLin Du [1 ]
Xu Zhang [1 ]
LiSheng Xu [1 ]
WanPeng Feng [2 ]
Lei Yi [3 ]
Peng Li [4 ]
机构
[1] Institute of Geophysics,China Earthquake Administration
[2] Canada Center for Mapping and Earth Observation, Natural Resources Canada
[3] School of Geodesy and Geomatics, Wuhan University
[4] College of Marine Geosciences, Ocean University of China
关键词
2016 MW7.8 Kaikoura earthquake; back-projection of array recordings; ASTFs-analysis of global recordings; joint inversion of teleseismic and InSAR data; complexity of source;
D O I
暂无
中图分类号
P315.7 [地震观测预报];
学科分类号
070801 ;
摘要
On November 13, 2016, an MW7.8 earthquake struck Kaikoura in South Island of New Zealand. By means of back-projection of array recordings, ASTFs-analysis of global seismic recordings, and joint inversion of global seismic data and co-seismic In SAR data, we investigated complexity of the earthquake source. The result shows that the 2016 MW7.8 Kaikoura earthquake ruptured about 100 s unilaterally from south to northeast(~N28°–33°E), producing a rupture area about 160 km long and about 50 km wide and releasing scalar moment 1.01×1021 Nm. In particular, the rupture area consisted of two slip asperities, with one close to the initial rupture point having a maximal slip value ~6.9 m while the other far away in the northeast having a maximal slip value ~9.3 m. The first asperity slipped for about 65 s and the second one started 40 s after the first one had initiated. The two slipped simultaneously for about 25 s.Furthermore, the first had a nearly thrust slip while the second had both thrust and strike slip. It is interesting that the rupture velocity was not constant, and the whole process may be divided into 5 stages in which the velocities were estimated to be 1.4 km/s, 0 km/s, 2.1 km/s, 0 km/s and 1.1 km/s, respectively. The high-frequency sources distributed nearly along the lower edge of the rupture area, the highfrequency radiating mainly occurred at launching of the asperities, and it seemed that no high-frequency energy was radiated when the rupturing was going to stop.
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页码:310 / 326
页数:17
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