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Matoza et al St. Helens Infrasound JGR 09

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B04305 MATOZA ET AL.: INFRASOUND FROM LPS AT MOUNT ST. HELENS<br />

Figure 2. Infrasonic and seismic waveforms at CDWR for an LP event with high SNR. Origin time of<br />

plot is 0818:35 UTC, 4 March 2005, time in seconds. (a) All sign<strong>al</strong>s filtered 1–15 Hz, from top to<br />

bottom: (1) infrasonic beam (azimuth 153°, speed 330 m/s), (2) infrasonic beam time advanced by 38 s,<br />

(3) vertic<strong>al</strong> seismic velocity, and (4) vertic<strong>al</strong> seismic displacement (integrated velocity). (c) Lower three<br />

traces in Figure 2a expanded to show time from 10 to 25 s. (b and d) same as Figures 2a and 2c but<br />

filtered 5–15 Hz. Note the following features: (1) no coincident seismo-acoustic arriv<strong>al</strong> observed in the<br />

infrasound data of upper trace in Figure 2a, (2) in band 1–15 Hz, infrasonic sign<strong>al</strong> has the same duration<br />

as the broadband trigger ons<strong>et</strong> in seismic LP event (Figure 2c), (3) in band 1–15 Hz, at 17 s, infrasonic<br />

amplitude is decaying into noise while resonant oscillations of the crack are becoming dominant in<br />

seismic record (Figure 2c), (4) dilatation<strong>al</strong> first motion observed in seismic displacement (Figure 2c),<br />

consistent with that of Waite <strong>et</strong> <strong>al</strong>. [2008], (5) in band 5–15 Hz, infrasonic and seismic waveforms have<br />

similar duration (Figures 2b and 2d), and (6) air-ground coupled energy observed in seismic data at 50 s<br />

in Figure 2b. The waveforms have norm<strong>al</strong>ized amplitudes; see Figure S1 for the waveforms shown at<br />

their correct amplitudes.<br />

roll-off at higher frequencies (>3 Hz) is more pronounced in<br />

the seismic data than infrasonic data, emphasizing that the<br />

infrasonic data may be more representative of the broadband<br />

trigger sign<strong>al</strong>. This may <strong>al</strong>so relate to frequencydependent<br />

anelastic attenuation and scattering, which is<br />

more severe for seismic energy in the volcanic edifice than<br />

in the air [Thelen <strong>et</strong> <strong>al</strong>., 20<strong>09</strong>; Sutherland and Bass, 2004].<br />

2.1.3. Amplitudes<br />

[17] Since the amplitudes of infrasonic LPs observed at<br />

CDWR vary significantly, we consider the distribution of<br />

infrasonic to vertic<strong>al</strong> seismic amplitude (P/Vz) ratios for a<br />

Figure 3. Power spectrum estimates for infrasonic and seismic LPs observed at CDWR on 11 November 2004 and 4<br />

March 2005. Events were picked with an STA/LTA d<strong>et</strong>ector, and a multitaper m<strong>et</strong>hod applied to a 12 s window surrounding<br />

the pick (1 s pr<strong>et</strong>rigger, 11 s posttrigger). The spectra for the individu<strong>al</strong> events were then progressively stacked (thick red<br />

line shows fin<strong>al</strong> stack). (a) The 1116 infrasonic LP events on 11 November 2004. (b) Vertic<strong>al</strong> component seismic LP events<br />

corresponding to infrasonic events in Figure 3a. (c) Transfer function formed by dividing fin<strong>al</strong> seismic spectrum stack<br />

(Figure 3b) by fin<strong>al</strong> infrasonic spectrum stack (Figure 3a). (d–f) Same as Figures 3a–3c but for 432 events on 4 March<br />

2005. The energy below 1.2 Hz in Figures 3a and 3d and below 0.5 Hz in Figures 3b and 3e is ambient noise, and not<br />

LP sign<strong>al</strong>.<br />

5of38<br />

B04305

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