HR: 09:35h
AN: S11C-07 INVITED [Abstracts]
TI: Excitation of earth's incessant free oscillations by Atmosphere-Ocean-Seafloor coupling
AU: * Romanowicz, B A
EM: barbara@seismo.berkeley.edu
AF: Berkeley Seismological Laboratory, 215 McCone Hall, Berkeley, CA 94720
United States
AU: RHIE, J
EM: rhie@seismo.berkeley.edu
AF: Berkeley Seismological Laboratory, 215 McCone Hall, Berkeley, CA 94720
United States
AB:
The observation on long period seismograms of continuously excited free oscillations of the Earth was first made by japanese
scientists in 1998,
during intervals free of significant earthquakes.
Since then, attention has focused on elucidating the physical mechanism
responsible for them. The sum of all small earthquakes remaining in the records cannot explain the observed level of
excitation. The mechanism must be shallow, as fundamental modes appear to be preferentially excited. It shows seasonal
variability, with peaks in the northern and southern hemisphere winters.
Stochastic mechanisms involving turbulent motion in the atmosphere have been
proposed as well as random distribution of sources around the world.
An alternative potential source of excitation of the continuous oscillations
is in the oceans, but so far the observations, based on the computation of
spectra or correlations of signals across long time series, do not have the
spacial and temporal resolution to locate these sources.
We have developed an array-based method to detect and locate sources of
very long period surface wave energy, utilizing the dispersive properties of
Rayleigh waves. Our basic approach uses data from two large aperture arrays of very long period seismometers (BDSN in
California and F-NET in Japan). We
stack the data after projection to the center of each array, and look for
directions of arrival of maximum amplitude in the stacks as a function of
back-azimuth, taking into account the array response. We show that, for each
array, there is a well defined preferential direction, which is stable over
one season but changes significantly from winter to summer. The fluctuation as a function of time of the maximum stack
amplitudes
are correlated across the two arrays and point to the northern Pacific ocean
in the northern hemisphere winter and the southern Oceans in the summer,
correlating with changes in the global distribution of maximum wave height.
We infer that the background oscillations originate primarily in the oceans,
and are caused by a non-linear coupling mechanism involving the atmosphere
(winds), the oceans (transfer of energy from ocean waves to infragravity
waves) and the seafloor (transfer of energy to elastic waves).
DE: 7255 Surface waves and free oscillations
DE: 7294 Instruments and techniques
DE: 4504 Air/sea interactions (0312)
DE: 4544 Internal and inertial waves
SC: Seismology [S]
MN: 2004 AGU Fall Meeting