Mm. Withers et al., HIGH-FREQUENCY ANALYSIS OF SEISMIC BACKGROUND-NOISE AS A FUNCTION OF WIND-SPEED AND SHALLOW DEPTH, Bulletin of the Seismological Society of America, 86(5), 1996, pp. 1507-1515
We used a deep (1500 m) cased borehole near the town of Datil in west-
central New Mexico to study high-frequency (>1 Hz) seismic noise chara
cteristics. The remote site had very low levels of cultural noise, but
strong winds (winter and spring) made the site an excellent candidate
to study the effects of wind noise on seismograms. Along with a three
-component set of surface sensors (Teledyne Geotech GS-13), a vertical
borehole seismometer (GS-28) was deployed at a variety of depths (5,
43, and 85 m) to investigate signal and noise variations. Wind speed w
as measured with an anemometer. Event-triggered and time-triggered dat
a streams were recorded on a RefTek 72-02 data acquisition system loca
ted at the site. Our data show little cultural noise and a strong corr
elation between wind speed and seismic background noise. The minimum w
ind speed at which the seismic background noise appears to be influenc
ed varies with depth: 3 m/sec at the surface, 3.5 m/sec at 43 m in dep
th, and 4 m/sec at 85 m in depth. For wind speed below 3 to 4 m/sec, w
e observe omni-directional background noise that is coherent at freque
ncies below 15 Hz. This coherence is destroyed when wind speeds exceed
3 to 4 m/sec. We use a test event (M(d) similar to 1.6) and superimpo
sed noise to investigate signal-to-noise ratio (SNR) improvement with
sensor depth. For the low Q valley fill of the Datil borehole (DBH) si
te, we have found that SNR can be improved by as much as 20 to 40 dB b
etween 23 and 55 Hz and 10 to 20 dB between 10 and 20 Hz, by deploying
at a 43-m depth rather than at the surface. At the surface, there is
little signal above noise in the 23- to 55-Hz frequency band for wind
speeds greater than 8 m/sec. Thus, high-frequency signal information t
hat is lost at the surface can be recorded by deploying at the relativ
ely shallow depth of 40 m. Because we observe only minor further reduc
tions in seismic background noise (SBN) at deeper depths, 40 m is like
ly to be a reasonable deployment depth for other high-frequency-monito
ring sites in similar environmental and geologic conditions.