HR: 1340h
AN: S23A-1107 [Abstracts]
TI: Broadband Ocean Bottom Instruments Record Earth's Free Oscillations during the Hawaiian PLUME Experiment
AU: * Laske, G
EM: glaske@ucsd.edu
AF: Cecil H. and Ida M. Green Institute of Geophysics and Planetary Physics-0225, UC San
Diego, 9500 Gilman Dr., La Jolla, CA 92093-0225, United States
AU: Orcutt, J A
AF: Cecil H. and Ida M. Green Institute of Geophysics and Planetary Physics-0225, UC San
Diego, 9500 Gilman Dr., La Jolla, CA 92093-0225, United States
AU: Collins, J A
AF: Geology and Geophysics Department, Woods Hole Oceanographic Institution, MS24, 360
Woods Hole Road, Woods Hole, MA 02543-1050, United States
AU: Detrick, R S
AF: Geology and Geophysics Department, Woods Hole Oceanographic Institution, MS24, 360
Woods Hole Road, Woods Hole, MA 02543-1050, United States
AU: Wolfe, C J
AF: Hawaii Institute of Geophysics and Planetology, U. Hawaii at Manoa, 1680 East-West Rd.,
POST 819A, Honolulu, HI 96822, United States
AU: Solomon, S C
AF: Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad
Branch Road, NW, Washington, DC 20015-1305, United States
AU: Bercovici, D A
AF: Geology and Geophysics Department, Yale University, P.O. Box 208109, New Haven, CT
06520-8109, United States
AU: Hauri, E H
AF: Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad
Branch Road, NW, Washington, DC 20015-1305, United States
AB:
Ocean islands are usually thought of as being noisy sites for the global seismic network (GSN).
For example, in the microseism band between 15 and 5~s, noise levels can easily be 10-20~dB higher than at
stations in the interiors of continents. On the other hand, and somewhat curiously, several Pacific island sites are
some of the quietest to record vertical ground movement in the free oscillation band beyond 200~s. This includes
station KIP (Kipapa, on Oahu/Hawaii) that is operated jointly by the USGS and the French GEOSCOPE group.
During the Hawaiian PLUME (Plume-Lithosphere Undersea Melt Experiment) deployment, we collected
continuous seismic data from January 2005 through June 2007, using a variety of seismic sensors deployed on
land and on the ocean floor. Ten broadband land stations were equipped with Wielandt--Streckeisen STS--2
seismometers, and about 70 ocean bottom sites were occupied with Güralp CMG-3T, Nanometrics Trillium 40
or Trillium 240 seismometers, and a Cox--Webb differential pressure gauge (DPG). This experiment gives us the
unique opportunity to assess the quality and variability of ultra--long period seismic signals, for specific sensors,
and evaluate the benefit and limits of deploying broad--band sensors on the ocean floor.
In 2005, we recorded five very large earthquakes with scalar seismic moments of M0=2x1020~Nm or
larger. One of these was the MS=8.2 28 March aftershock of the great 26 December 2004 Sumatra--Andaman
earthquake. At station KIP, which is equipped with a very broad--band STS--1, the free oscillation spectrum is of
extremely high quality. We can identify mode 0S2 (~0.31~mHz) that is observed only for the largest
earthquakes, and only at the quietest GSN stations. Even on the STS--2 record, mode 0S3
(~0.47~mHz) is clearly discernible. The quality of spectra recorded on the OBSs varies greatly, but at some
sites we observe mode 0S6 (~1.04~mHz). These records are greatly superior to those at GSN stations
POHA (island of Hawaii), whose record has no seismic signal, and MIDW (Midway Island), whose record is noisy
for this event. With M0=111x1020~Nm, events such as the 28 March aftershock occur only once every few
decades and high-quality spectra should be expected. On the other hand, we can observe modes on OBS
records also for the other four 2005 events, down to 0S13 (~2.11~mHz) and at a noise level that is not
met by many land stations in broadband seismic monitoring arrays. PLUME may well be the first OBS experiment
recording free oscillation spectra since the OSN1 pilot experiment recorded the great 25 March 1998 Balleny
Island earthquake.
Higher ambient noise levels in the pressure signal as well as the lower sensor sensitivity at ultra--long periods
hamper the observation of free oscillations on the DPG. For the 25 March event, we can observe modes down to
0S20 (~2.88~mHz) but not much beyond that.
UR: http://mahi.ucsd.edu/Gabi/plume.html
DE: 3050 Ocean observatories and experiments
DE: 3094 Instruments and techniques
DE: 7255 Surface waves and free oscillations
DE: 7294 Seismic instruments and networks (0935, 3025)
SC: Seismology [S]
MN: 2007 Fall Meeting