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Amplitude of the Earth's free oscillations and long‐period characteristics of the earthquake source
Author(s) -
Kanamori Hiroo,
Anderson Don L.
Publication year - 1975
Publication title -
journal of geophysical research
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/jb080i008p01075
Subject(s) - amplitude , shock (circulatory) , seismology , physics , geology , seismic moment , period (music) , excited state , geophysics , atomic physics , optics , acoustics , medicine , fault (geology)
Amplitude spectra of the spheroidal modes 0 S l ( l = 2–40) excited by the 1960 Chilean earthquake and observed at Pasadena, Los Angeles, and Isabella show distinct holes at 0 S 10 ( T = 580 s) and 0 S 21 ( T = 336 s). These holes can be explained as an interference pattern caused by a composite source consisting of a finite propagating source (main shock) and a slow precursory source, 15 min before the main shock. A total seismic moment of 4–5 × 10 30 dyn cm is required to explain the observed amplitude.

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