Seismological Research Letters; July/August 2008; v. 79; no. 4;
p. 504-509; DOI: 10.1785/gssrl.79.4.504
© 2008 Seismological Society of America
Broadband Seismic Noise Analysis of the Soufrière Hills Volcano Network
Silvio De Angelis
Montserrat Volcano
Observatory
| The first 20% of the full text of this article appears below.
|
 |
INTRODUCTION
|
|---|
The Soufrière Hills Volcano (SHV), Montserrat, West Indies, is an
active andesitic dome-building volcano at the northern end of the Lesser
Antilles volcanic arc. The ongoing eruption, characterized by cyclic growth
and collapse of an andesite lava dome with associated pyroclastic flows (PF),
vulcanian explosions, and debris flows, began on 18 July 1995
(Young et al. 1998;
Aspinall et al. 1998)
after a three-year period of precursor seismic activity.
Prior to this eruption, volcanic activity in Montserrat was monitored by
the Seismic Research Unit (SRU), based at the University of West Indies, St.
Augustine, Trinidad, as part of its regional seismic network, with two
stations located on-island. In 1994, prompted by the increased seismic
activity, SRU expanded the seismic network on Montserrat by installing four
additional stations (Luckett et
al. 2007). During July 1995, coincident with the onset of
phreatic activity at SHV, the U.S. Geological Survey installed three seismic
stations (Power et al.
1998) to complement the existing network. In October 1996, the
British Geological Survey (BGS) established a new digital seismic network of
broadband instruments. The configuration of the SHV digital network has
changed through the years until its latest upgrade in 2005. The present SHV
digital seismic network (figure
1) consists of eight broadband, three-component Guralp CMG-40T
seismometers and two short-period, vertical-component Mark Products L4
(Luckett et al. 2007).
Seismic data are digitized onsite by Guralp DM24 24-bit digitizers and
time-stamped using GPS clocks. Continuous data are telemetered from the sites
using spread spectrum Freewave radio modems operating at 900 Mhz. Two repeater
sites facilitate data transmission to the observatory where they are archived
and analyzed. A detailed description of the history of the seismic network at
SHV and its present configuration can be found in . . . [Full Text of this Article]
Montserrat Volcano Observatory
Flemmings, Montserrat, West
Indies
silvio@mvo.ms
Copyright © 2009 by Seismological Society of America