How to reach a few percent level in determining the Lense-Thirring effect?

Details How to reach a few percent level in determining the Lense-Thirring effect? How to reach a few percent level in determining the Lense-Thirring effect?

2004-04-13

arxiv.org/abs/gr-qc/0404062v6

Gen.Rel.Grav. 37 (2005) 1059-1074

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Latex2e, 22 pag. 1 table, 2 figures, 45 references. Changes in the Abstract, Introduction and Conclusions. Discussion on the n

Scientific paper

10.1007/s10714-005-0091-2

In this paper we discuss and compare a node-only LAGEOS-LAGEOS II combination and a node-only LAGEOS-LAGEOS II-Ajisai-Jason1 combination for the determination of the Lense-Thirring effect. The new combined EIGEN-CG01C Earth gravity model has been adopted. The second combination cancels the first three even zonal harmonics along with their secular variations but introduces the non-gravitational perturbations of Jason1. The first combination is less sensitive to the non-conservative forces but is sensitive to the secular variations of the uncancelled even zonal harmonics of low degree J4 and J6 whose impact grows linearly in time.

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