Open AccessPolarized Earth's ambient microseismic noise
Author(s) -
Schimmel M.,
Stutzmann E.,
Ardhuin F.,
Gallart J.
Publication year - 2011
Publication title -
geochemistry, geophysics, geosystems
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.928
H-Index - 136
ISSN - 1525-2027
DOI - 10.1029/2011gc003661
Subject(s) - microseism , ambient noise level , geology , azimuth , seismogram , seismic noise , polarization (electrochemistry) , seismology , noise (video) , rayleigh wave , frequency domain , geophysics , acoustics , surface wave , physics , optics , computer science , oceanography , sound (geography) , chemistry , artificial intelligence , image (mathematics) , computer vision
We quantify, analyze, and characterize the frequency‐dependent microseismic noise recorded by worldwide distributed seismic stations. Microseismic noise is generated through the interaction of ocean waves. It is the strongest ambient noise, and it is observed everywhere on Earth. We introduce a new approach which permits us to detect polarized signals in the time‐frequency domain and which we use to characterize the microseismic noise. We analyze 7 years of continuous seismograms from the global GEOSCOPE network. Microseisms are dominated by Rayleigh waves, and we therefore focus on elliptically polarized signals. The polarized signals are detected in the time‐frequency domain through a degree of polarization measure. We design polarization spectra and show that microseismic noise is more strongly polarized than noise in other frequency bands. This property is used to measure the directions of the polarized noise at individual stations as a function of time and frequency. Seasonal variations are found for the back azimuths and for the number of polarized signals at many stations. We show that the back azimuth directions are robust measurements that point toward the source areas computed from ocean wave models.