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Combinations of Earth orientation measurements: SPACE94, COMB94, and POLE94
Author(s) -
Gross Richard S.
Publication year - 1996
Publication title -
journal of geophysical research: solid earth
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/96jb00113
Subject(s) - polar motion , satellite laser ranging , geodesy , series (stratigraphy) , astrometry , very long baseline interferometry , orientation (vector space) , earth's rotation , outlier , kalman filter , geodetic datum , remote sensing , geology , universal time , mathematics , physics , optics , laser , laser ranging , statistics , geometry , astronomy , paleontology , stars
A Kalman filter has been used to combine independent measurements of the Earth's orientation taken by the space‐geodetic observing techniques of lunar laser ranging, satellite laser ranging, very long baseline interferometry, and the Global Positioning System. Prior to their combination, the data series were adjusted to have the same bias and rate, the stated uncertainties of the measurements were adjusted, and data points considered to be outliers were deleted. The resulting combination, SPACE94, consists of smoothed, interpolated polar motion and UT1‐UTC values spanning October 6.0, 1976, to January 27.0, 1995, at 1‐day intervals. The Kalman filter was then used to combine the space‐geodetic series comprising SPACE94 with two different, independent series of Earth orientation measurements taken by the technique of optical astrometry. Prior to their combination with SPACE94, the bias, rate and annual term of the optical astrometric series were corrected, the stated uncertainties of the measurements were adjusted, and data points considered to be outliers were deleted. The adjusted optical astrometric series were then combined with SPACE94 in two steps: (1) the Bureau International de l'Heure (BIH) optical astrometric series was combined with SPACE94 to form COMB94, a combined series of smoothed, interpolated polar motion and UT1‐UTC values spanning January 20.0, 1962, to January 27.0, 1995, at 5‐day intervals, and (2) the International Latitude Service (ILS) optical astrometric series was combined with COMB94 to form POLE94, a combined series of smoothed, interpolated polar motion values spanning January 20, 1900, to January 21, 1995, at 30.4375‐day intervals.

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