Revisiting the three M~7 Miyagi-oki earthquakes in the 1930s: Possible seismogenic slip on asperities that were re-ruptured during the 1978 M=7.4 Miyagi-oki earthquake

Norihito Umino, Toshio Kono, Tomomi Okada, Junichi Nakajima, Toru Matsuzawa, Naoki Uchida, Akira Hasegawa, Yoshiaki Tamura, Gen Aoki

Research output: Contribution to journalArticlepeer-review

29 Citations (Scopus)

Abstract

Hypocenters of main shocks and aftershocks of the 1933 M=7.1, 1936 M=7.4, 1937 M=7.1 and 1978 M=7.4 Miyagi-oki earthquakes are relocated using S-P times reported in the Seismological Bulletin of the Japan Meteorological Agency (JMA) and those re-read from original smoked-paper seismograms observed at the Mizusawa station of the National Astronomical Observatory of Japan (NAOJ) and the Mukaiyama station of Tohoku University. In order to reduce the error caused by inaccuracies of the arrival times and the small number of seismic observation stations, we determined the hypocenters by using a grid search method that assumed that the events occurred at the boundary between the subducting Pacific plate and the overriding plate. The main shock epicenters of these four earthquakes were determined to be close to each other, while the distributions of their aftershocks seem to disperse on the upper boundary of the Pacific plate. These distributions show that aftershock areas of the 1933, 1936 and 1937 events partly ov rlap with that of the 1978 event and occupy its easternmost, central and westernmost portions, respectively. This result suggests that the 1933, 1936 and 1937 events possibly ruptured a part of the source area of the 1978 event, i.e., its eastern, central and western portions, respectively.

Original languageEnglish
Pages (from-to)1587-1592
Number of pages6
Journalearth, planets and space
Volume58
Issue number12
DOIs
Publication statusPublished - 2006

Keywords

  • Miyagi-oki earthquake
  • asperity
  • interplate earthquake
  • smoked-paper seismogram
  • subduction zone

ASJC Scopus subject areas

  • Geology
  • Space and Planetary Science

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