Modulation of seismic noise near the San Jacinto fault in southern California: origin and observations of the cyclical time dependence and associated crustal properties. Issue 1 (26th December 2020)

• Record Type: Journal Article
• Authors: Martynov, Vladislav G; Astiz, Luciana; Kilb, Debi; Vernon, Frank L
• Is Part Of: Geophysical journal international. Volume 225:Issue 1(2021)
• Page Start: 127
• Page End: 139
• Publication Date: 2020-12-26
• Subjects: Permeability and porosity -- Tides and planetary waves -- North America -- Seismic anisotropy -- Seismic attenuation -- Seismic noise; Geophysics -- Periodicals; 550
• DOI: 10.1093/gji/ggaa585
• Languages: English
• ISSNs: 0956-540X

Abstract

SUMMARY: We examine the cyclic amplitude variation of seismic noise recorded by continuous three-component broad-band seismic data with durations spanning 91–713 d (2008–2011) from three different networks: Anza seismic network, IDA network and the transportable seismic array. These stations surround the San Jacinto Fault Zone (SJFZ) in southern California. We find the seismic noise amplitudes exhibit a cyclical variation between 0.3 and 7.2 Hz. The high-frequency (≥0.9 Hz) noise variations can be linked to human activity and are not a concern. Our primary interest is signals in the low frequencies (0.3–0.9 Hz), where the seismic noise is modulated by semi-diurnal tidal mode M 2 . These long-period (low-frequency) variations of seismic noise can be attributed to a temporal change of the ocean waves breaking at the shoreline, driven by ocean tidal loading. We focus on the M 2 variation of seismic noise at f = 0.6 Hz, travelling distances of ∼92 km through the crust from offshore California to the inland Anza, California, region. Relative to the shoreline station, data from the inland stations show a phase lag of ∼ –12°, which we attribute to the cyclic change in M 2 that can alter crustal seismic attenuation. We also find that for mode M 2 at 0.6 Hz, the amplitude variations of the seismic quality factor ( Q ) depend on azimuth and varies from 0.22 per cent (southeast to northwest) to 1.28 per cent (northeast to southwest) with Q = 25 for Rayleigh waves. We propose the direction dependence of the Q variation at 0.6 Hz reflects the preferred orientation of subfaults parallel to the main faulting defined by the primarily N45°W strike of the SJFZ.