The radial orbit error was computed for circular orbits at the altitudes of 525 and 830 km, using linear orbit perturbation theory and the gravity field error covariances [Rosborough , 1986] from JGM2, JGM3, and EGM96, as a function of satellite inclination. Orbit perturbations longer than ten days were excluded, and the analysis does not include the long period perturbations due to the odd zonals. The structure of the radial error vs inclination shows the weakness of JGM2/JGM3 at the low inclinations (i <35 degrees). The poor behavior at these low inclinations is a consequence of the dearth of tracking data from satellites at such inclinations in JGM2 and JGM3. In EGM96, significant new data from the EUVE satellite (i=28.5 degres, mean altitude=525 km) was included.
EGM96 also shows an improvement at the polar inclinations (i=82 to 93 degrees) which may be attributed in part to the addition of tracking data from the Hilat and Radcal spacecraft.References:
Kaula, W. M., Theory of satellite geodesy, Blaisdell Publishing Co., Waltham, MA 1966.
Rosborough, G. W., Satellite orbit perturbations due to the geopotential , Center for Space Research, The University of Texas at Austin, January 1986.
The Hilat and Radcal data benefit the EGM96 solution by reducing the predicted radial orbit error in this altitude and inclination band by up to 20 cm.
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