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Analysis of earth rotation solution from StarletteEarth rotation parameter (ERP) solutions were derived from the Starlette orbit analysis during the Main MERIT Campaign, using a technique of a consider-covariance analysis to assess the effects of errors on the polar motion solutions. The polar motion solution was then improved through the simultaneous adjustment of some dynamical parameters representing identified dominant perturbing sources (such as the geopotential and ocean-tide coefficients) on the polar motion solutions. Finally, an improved ERP solution was derived using the gravity field model, PTCF1, described by Tapley et al. (1986). The accuracy of the Starlette ERP solution was assessed by a comparison with the LAGEOS-derived ERP solutions.
Document ID
19890062471
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schutz, B. E.
(Texas Univ. Austin, TX, United States)
Cheng, M. K.
(Texas Univ. Austin, TX, United States)
Shum, C. K.
(Texas Univ. Austin, TX, United States)
Eanes, R. J.
(Texas Univ. Austin, TX, United States)
Tapley, B. D.
(Texas, University Austin, United States)
Date Acquired
August 14, 2013
Publication Date
August 10, 1989
Publication Information
Publication: Journal of Geophysical Research
Volume: 94
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
89A49842
Funding Number(s)
CONTRACT_GRANT: NAG5-757
Distribution Limits
Public
Copyright
Other

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