Abstract
The scale factor and bias of the magnetometer must be determined in order to appropriately estimate satellite dynamics and control orientation. The magnetometer scale factor and bias are not constant due to temperature variation and thermal distortion of the structure, which causes a relatively large magnitude error, and these effects must be eliminated to meet the requirements of the mission. This study proposes a nonlinear two-stage Kalman filter (NTSKF)based method for in-orbit calibration of a magnetometer. The magnetometer bias and scale factor error are combined to form the equivalent non-steady bias noise, which is removed from the magnetometer measurements as bias noise. Each iteration of the estimation process has two stages: the first stage uses the Kalman filter to estimate equivalent magnetometer biases as well as three state parameters; the second stage uses the extension of the Kalman filter proposed in this study to estimate three magnetometer biases and three scale factors. If the magnetometer biases and scale factors change insignificantly in the long-time interval, then biases and scale factors can be accepted as constant and estimated using the proposed extension of the Kalman filter under the conditions defined in this work.
Original language | English |
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Journal | Proceedings of the International Astronautical Congress, IAC |
Volume | 2023-October |
Publication status | Published - 2023 |
Event | 74th International Astronautical Congress, IAC 2023 - Baku, Azerbaijan Duration: 2 Oct 2023 → 6 Oct 2023 |
Bibliographical note
Publisher Copyright:Copyright © 2023 by the International Astronautical Federation (IAF). All rights reserved.
Keywords
- Small satellite
- attitude dynamics
- bias
- calibration
- magnetometer
- nonlinear Kalman filter
- scale factor