1999
DOI: 10.1029/1998jb900019
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Geophysical interpretation of observed geocenter variations

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Cited by 98 publications
(138 citation statements)
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“…The four test cases are: (1) the GRACE C 20 coefficient is omitted; (2) the GRACE C 20 coefficient is retained; (3) SLR values for C 20 and seasonal C 11 , S 11 , and C 10 are used (Chen et al 1999); and (4) SLR seasonal C 11 , S 11 , and C 10 are used, GRACE values of C 21 and S 21 are replaced with estimates from Earth Orientation Parameters (EOP) (Chen et al 2004), and SLR annual and semi-annual C 20 are substituted for GRACE values (Cheng and Tapley 2002).…”
Section: Grace Observationsmentioning
confidence: 99%
See 1 more Smart Citation
“…The four test cases are: (1) the GRACE C 20 coefficient is omitted; (2) the GRACE C 20 coefficient is retained; (3) SLR values for C 20 and seasonal C 11 , S 11 , and C 10 are used (Chen et al 1999); and (4) SLR seasonal C 11 , S 11 , and C 10 are used, GRACE values of C 21 and S 21 are replaced with estimates from Earth Orientation Parameters (EOP) (Chen et al 2004), and SLR annual and semi-annual C 20 are substituted for GRACE values (Cheng and Tapley 2002).…”
Section: Grace Observationsmentioning
confidence: 99%
“…Degree-2 coefficients in GRACE products are currently not well determined (e.g., in the 0001 release as we use in this study) limited probably by orbit geometry and other unknown reasons (Tapley et al 2004b), and we experiment by replacing them with independent estimates from Earth rotation changes (Chen and Wilson 2003;Chambers et al 2004) and satellite laser ranging (SLR) observations (Cheng and Tapley 2002). GRACE does not measure degree-1 spherical harmonics, related to geocenter motion, but these are available from SLR observations (Chen et al 1999), and have a measurable effect on GRACE-derived sea level estimates.…”
Section: Introductionmentioning
confidence: 99%
“…To be consistent with the reference frame used for T/P, the degree 1 coefficients, which are estimated from the variations of the Earth's center of mass proposed by Chen et al (1999), are added to the GRACE data.…”
Section: Gracementioning
confidence: 99%
“…Geocenter motion is typically derived from satellite laser ranging (SLR) observations to geodetic satellites as, e.g., LAGEOS and STELLA, that relate the kinematic orbits of those satellites to stations realizing the terrestrial reference frame (Chen et al, 1999;Eanes, 2000;Cretaux et al, 2002). Alternatively, observations of the global network of GPS permanent stations allow also for the derivation of geocenter variations (Blewitt et al, 2001;Lavallée et al, 2006;Fritsche et al, 2010).…”
Section: Introductionmentioning
confidence: 99%