After a brief description of the experiment to detect the gravitomagnetic field using high altitude laser ranged artificial satellites, the author studies several non-gravitational perturbations that affect the LAGEOS nodal longitude. It is shown that the error in the calculated value of the secular nodal precession or the value of the secular nodal precession itself is, for each perturbation, less than 1% of the gravitomagnetic drag.

The LAGEOS Lense-Thirring precession and the LAGEOS non-gravitational nodal perturbations.

CIUFOLINI, Ignazio
1987-01-01

Abstract

After a brief description of the experiment to detect the gravitomagnetic field using high altitude laser ranged artificial satellites, the author studies several non-gravitational perturbations that affect the LAGEOS nodal longitude. It is shown that the error in the calculated value of the secular nodal precession or the value of the secular nodal precession itself is, for each perturbation, less than 1% of the gravitomagnetic drag.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11587/370014
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