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)