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An Assessment of the Systematic Uncertainty in Present and Future Tests of the Lense-Thirring Effect with Satellite Laser Ranging

2008/09/30 by Lorenzo Iorio · 3 citations
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #GNSS positioning and interference #Geophysics and Gravity Measurements #Ionosphere and magnetosphere dynamics #astro-ph #gr-qc #physics.geo-ph #physics.space-ph

paper · pdf · doi:10.1007/s11214-008-9478-1

published as Space Sci.Rev.148: 363-381,2009 · LaTex, 19 pages, 1 figure, 12 tables. Invited and refereed contribution to The ISSI Workshop, 6-10 October 2008, on The Nature of Gravity Confronting Theory and Experiment in Space To appear in Space Science Reviews

arxiv created 2008/12/05 · openalex publication_date 2008/12/25 · arxiv updated 2010/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01

Abstract

We deal with the attempts to measure the Lense-Thirring effect with the Satellite Laser Ranging (SLR) technique applied to the existing LAGEOS and LAGEOS II terrestrial satellites and to the recently approved LARES spacecraft.The first issue addressed here is: are the so far published evaluations of the systematic uncertainty induced by the bad knowledge of the even zonal harmonic coefficients JL of the multipolar expansion of the Earth's geopotential reliable and realistic? Our answer is negative. Indeed, if the differences Delta JL among the even zonals estimated in different Earth's gravity field global solutions from the dedicated GRACE mission are assumed for the uncertainties delta JL instead of using their covariance sigmas sigmaJL, it turns out that the systematic uncertainty δμin the Lense-Thirring test with the nodes Omega of LAGEOS and LAGEOS II may be up to 3 to 4 times larger than in the evaluations so far published (5-10%) based on the use of the sigmas of one model at a time separately. The second issue consists of the possibility of using a different approach in extracting the relativistic signature of interest from the LAGEOS-type data. The third issue is the possibility of reaching a realistic total accuracy of 1% with LAGEOS, LAGEOS II and LARES, which should be launched in November 2009 with a VEGA rocket. While LAGEOS and LAGEOS II fly at altitudes of about 6000 km, LARES will be likely placed at an altitude of 1450 km. Thus, it will be sensitive to much more even zonals than LAGEOS and LAGEOS II. Their corrupting impact has been evaluated with the standard Kaula's approach up to degree L=60 by using Delta JL and sigmaJL; it turns out that it may be as large as some tens percent.

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