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Shallow repeating seismic events under an alpine glacier at Mount Rainier, Washington, USA

Published online by Cambridge University Press:  10 July 2017

Weston A. Thelen
Affiliation:
Cascade Volcano Observatory, Vancouver, WA, USA E-mail: wthelen@usgs.gov
Kate Allstadt
Affiliation:
Pacific Northwest Seismic Network, Department of Earth and Space Sciences, University of Washington, Seattle, WA, USA
Silvio De Angelis
Affiliation:
Pacific Northwest Seismic Network, Department of Earth and Space Sciences, University of Washington, Seattle, WA, USA
Stephen D. Malone
Affiliation:
Pacific Northwest Seismic Network, Department of Earth and Space Sciences, University of Washington, Seattle, WA, USA
Seth C. Moran
Affiliation:
Cascade Volcano Observatory, Vancouver, WA, USA E-mail: wthelen@usgs.gov
John Vidale
Affiliation:
Pacific Northwest Seismic Network, Department of Earth and Space Sciences, University of Washington, Seattle, WA, USA
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Abstract

We observed several swarms of repeating low-frequency (1–5 Hz) seismic events during a 3 week period in May–June 2010, near the summit of Mount Rainier, Washington, USA, that likely were a result of stick–slip motion at the base of alpine glaciers. The dominant set of repeating events (‘multiplets’) featured >4000 individual events and did not exhibit daytime variations in recurrence interval or amplitude. Volcanoes and glaciers around the world are known to produce seismic signals with great variability in both frequency content and size. The low-frequency character and periodic recurrence of the Mount Rainier multiplets mimic long-period seismicity often seen at volcanoes, particularly during periods of unrest. However, their near-surface location, lack of common spectral peaks across the recording network, rapid attenuation of amplitudes with distance, and temporal correlation with weather systems all indicate that ice-related source mechanisms are the most likely explanation. We interpret the low-frequency character of these multiplets to be the result of trapping of seismic energy under glacial ice as it propagates through the highly heterogeneous and attenuating volcanic material. The Mount Rainier multiplet sequences underscore the difficulties in differentiating low-frequency signals due to glacial processes from those caused by volcanic processes on glacier-clad volcanoes.

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 2013
Figure 0

Fig. 1. Seismic station locations (triangles) and location of main multiplet of 2010 seismic sequence (star). RCM indicates the location of the Camp Muir seismic station and weather station. LON and LO2 seismometers are co-located.

Figure 1

Fig. 2. Example of various types of waveforms (a) and their spectra (b) recorded on Mount Rainier at short-period vertical station RCS. The amplitude scale is normalized for each waveform, with the maximum amplitudes for each waveform given in counts on the left. Gray triangles indicate time windows for spectra. In order from the top of the plot: glacial earthquake, multiplet 5 of this sequence; inferred icequake; M1.2 tectonic earthquake located ∼20 km east of Mount Rainier; M0.6 volcano-tectonic earthquake located 2.5 km below the mountain from a September 2009 swarm; M2.3 deep long-period earthquake 13.6 km below Mount Rainier; avalanche on 5 June 2010; inferred rockfall near Willis Wall 7 June 2010.

Figure 2

Fig. 3. (a) Timeline of multiplet occurrence, 15 May–18 June 2010. Each circle represents an earthquake; earthquakes on the same line are part of the same multiplet. Only multiplets with five or more events are shown. Gray rectangle shows the period when no multiplets occurred. (b) Comparison of number of detected non-multiplet events (gray line) to detected multiplets calculated every hour (black line). Gray rectangle shows the period when no multiplets occurred.

Figure 3

Fig. 4. Fifteen representative waveforms from (a) multiplet 5, and (b) multiplet 6, as recorded on station STAR (Fig. 1). Waveforms are filtered between 0.5 and 8 Hz.

Figure 4

Fig. 5. (a, c, e) Recurrence interval (a), pseudo-energy (c) and cross-correlation coefficient (e) of individual events within multiplet 5 recorded on station STAR (Fig. 1). (b, d, f) Recurrence interval (b), pseudo-energy (d) and cross-correlation coefficient (f) of individual events within multiplet 6 recorded on STAR. The dark bars in (d) show periods of daylight. The cross-correlation coefficient is calculated with respect to the first detected event within the multiplet. The faint doubling at twice the main recurrence interval reflects missed events in the automatic detection scheme. The gray rectangles in (a), (c) and (e) are times when the multiplets paused between phases.

Figure 5

Fig. 6. Stacked normalized waveforms (a) and spectra (b) of multiplet 5 on several stations (see Fig. 1 for station locations). Gray vertical lines indicate time windows taken for the spectra. Seismograms for distant stations RER, FMW and LO2 were bandpass-filtered at 0.5–10 Hz to improve clarity. Arrows show first arrival times for each station.

Figure 6

Fig. 7. Plot showing connection of multiplet activity with weather. (a) Temperatures recorded at Paradise and Camp Muir; (b) cumulative precipitation recorded at Paradise; (c) stream gauge heights for the White River downstream of Winthrop and Emmons Glaciers and the Puyallup River downstream of glaciers on western slopes; (d) upper-air barometric pressure interpolated to 4200 m from the nearest NCEP/ NCAR reanalysis gridpoint (http://ingrid.ldgo.columbia.edu/ SOURCES/.NOAA/.NCEP-NCAR/.CDAS-1/); and (e) number of multiplet events detected per hour. Vertical dashed line 1 indicates the onset of the repeating sequences, 2 shows the onset of the 20 May storm, 3 indicates the gap where multiplet activity ceases, and 4 indicates the onset of the second multiplet episode of activity coinciding with the onset of the 2 June storm and rising stream-gauge levels.