dot
Detailansicht
Katalogkarte GBA
Katalogkarte ISBD
Suche präzisieren
Drucken
Download RIS
Hier klicken, um den Treffer aus der Auswahl zu entfernen
Titel The study on the coefficients of Earth's gravitational field using Scaled Sensitivity Matrix method
VerfasserIn Weijing Qu, Danan Dong, Bin Wu
Konferenz EGU General Assembly 2015
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 17 (2015)
Datensatznummer 250105362
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2015-4884.pdf
 
Zusammenfassung
The estimated monthly mean gravitational field parameters from one or two satellites only represent the linear combinations of a few primary spherical harmonic coefficients due to the limited sensitivity to the Earth’s gravitational field. Using multiple satellites at various altitudes and inclinations increase the sensitivity and mitigate the non-unique problem. In practice, however, the explorations with a few satellites are still inevitable, such as the moon and deep space missions. Furthermore, the problem of the estimated parameters contaminated by the other un-estimated parameters due to the high correlation exists widely among various disciplines. Thus the quantitative assessment of the influence of un-estimated parameters on the estimated parameters provides important insight into the nature of the obtained solutions. In this paper, we study the estimated monthly mean, uncorrelated gravitational field parameters ( , , and ) from the Lageos1 and Lageos2 Satellite Laser Ranging (SLR) data for the 10 years period (2004-2013). Using the Scaled Sensitivity Matrix (SSM) method, we investigate the contributions from the other 73 un-estimated gravitational coefficients from degrees and orders 2 through 8 to the 4 estimated gravitational parameters. Our results confirm the reasonableness of the previous zonal combination coefficients from the orbital node analysis. Meanwhile our results reveal time-dependent correlations between the estimated non-zonal parameters and the un-estimated gravitational coefficients.