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.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom