4.5 Article

Cascadia tremor spectra: Low corner frequencies and earthquake-like high-frequency falloff

Journal

GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS
Volume 12, Issue -, Pages -

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1029/2011GC003759

Keywords

beamforming; source spectrum; tremor

Funding

  1. U.S. Air Force Research Laboratory [FA8718-07-C-0005]
  2. NSF [EAR-0710881, EAR-0844392, EAR-0944109, OCE-1030022]

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The discovery of non-volcanic tremor (NVT) has opened a new window to observe major Earth plate boundaries. However, the spectral characteristics of NVT have not been well studied due to poor signal-to-noise ratio (SNR) on individual seismograms. We estimate the spectral content of Cascadia tremor between 2.5 and 20 Hz by suppressing noise using array analysis, and compute empirical path corrections using nearby small earthquakes. We demonstrate that the displacement spectra of the Cascadia tremor have corner frequencies around 3-8 Hz and fall off at f(-2) to f(-3) at higher frequencies. Our results have the following implications. (1) The high-frequency falloff of tremor agrees with the observations of regular earthquakes, suggesting that tremor can be analyzed using standard spectral models. Prior analyses that have shown a tremor spectral falloff proportional to f(-1) may reflect only the spectral behavior over a limited frequency band. (2) Tremor may be no different from a swarm of microearthquakes with abnormally small stress drops on the order of kPa, likely due to the presence of fluids. Alternatively the low corner frequencies of tremor may reflect abnormally slow ruptures. (3) Fitting a standard Brune (1970) spectral model implies a moment release rate of Cascadia tremor of 3.8 x 10(10) N.m/s assuming the tremor signals are P waves (or 1.4 x 10(10) N.m/s assuming S-waves). This implies that a typical 20-day long tremor episode releases moment equivalent to Mw 5.1 (P-wave) or Mw 4.9 (S-wave), although these may be underestimates if the spectra deviate substantially from the Brune model at very low frequencies.

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