Tilt-to-length coupling in the grace follow-on laser ranging interferometer

authored by
Henry Wegener, Vitali Müller, Gerhard Heinzel, Malte Misfeldt
Abstract

The Laser Ranging Interferometer onboard the Gravity Recovery and Climate Experiment Follow-On satellites is the first laser interferometer in space measuring satellite-to-satellite distance variations. One of its main noise sources at low frequencies is the so-called tilt-to-length coupling, caused by satellite pointing variations. This error is estimated by fitting a linear coupling model, making use of the so-called center-of-mass calibration maneuvers. These maneuvers are performed regularly for the original purpose of center-of-mass determination. Here, the results of the tilt-to-length estimations for the Laser Ranging Interferometer are presented in terms of coupling factors, which are all within 200 μm ⋅ rad−1 and thus meet the requirements. From these parameters, estimations of nadir and cross-track components of the spacecraft center-of-mass positions with respect to the interferometer reference point are derived, providing an additional method to track center-of-mass movement over time.

Organisation(s)
Institute of Gravitation Physics
External Organisation(s)
Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
Type
Article
Journal
Journal of Spacecraft and Rockets
Volume
57
Pages
1362-1372
No. of pages
11
ISSN
0022-4650
Publication date
27.07.2020
Publication status
Published
Peer reviewed
Yes
ASJC Scopus subject areas
Aerospace Engineering, Space and Planetary Science
Electronic version(s)
https://doi.org/10.2514/1.A34790 (Access: Open)