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| The first 20% of the full text of this article appears below. |
| INTRODUCTION |
|---|
1.0 mHz
(Van Camp 1999;
Rosat et al. 2003;
Widmer-Schnidrig 2003;
Park et al. 2005).
SGs can therefore make a significant contribution to the illumination of
long-wavelength density heterogeneities in the Earth's mantle
(Widmer-Schnidrig 2003). For
reasons of price and complexity, the number of SGs is small compared to the
number of sensors deployed in the Global Seismic Network (GSN). However, the
potential of a sparse network of gravimeters for normal-mode research has been
demonstrated by the International Deployment of Accelerometers (IDA) network
(Agnew et al. 1986).
Another point worth noting is the stability and accuracy (
0.1% level) of
the calibration factor of SGs (Francis
et al. 1998) requested to validate Earth and ocean tide
models using tidal gravity measurements
(Baker and Bos 2003). This
compares well with seismic networks, where results are barely better than 1%
(http://ida.ucsd.edu/pdf/DMSSC_2005_10.pdf;
Park et al. 2005;
Davis et al. 2005).
Such accuracy is quite unacceptable for geodesy.
Since 1997, most of the SG data have been collected under the framework of
the Global Geodynamics Project (GGP) global network
(Crossley et al. 1999)
that presently includes about 25 instruments. The GGP aims to look at seismic
normal modes, the Slichter triplet, tidal gravity, ocean tidal loading, core
nutations, core modes, and hydrology. Up to now the data have been gathered in
an ad hoc database, using the ASCII PRETERNA format, which acts as a standard
for tidal analysis (Wenzel
1996). These data are available to non-GGP members after a
six-month delay. In order
Royal Observatory of Belgium, Seismology
Avenue Circulaire, 3,
BE-1180 Uccle,
Belgium
mvc@oma.be
(M.V.C.)
Quanterra, Inc., 325 Ayer Road
Harvard, Massachusetts 01451
U.S.A.
steim@quanterra.com
(J.
S.)
École et Observatoire des Sciences de la Terre
5 rue
René Descartes
FR-67084 Strasbourg Cedex,
France
luis.rivera@eost.u-strasbg.fr
(L.
R.)
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