TY - JOUR
T1 - Particle swarm optimization for magnetometer calibration with rotation axis fitting using in-orbit data
AU - Riwanto, Bagus Adiwiluhung
AU - Niemela, Petri
AU - Ehrpais, Hendrik
AU - Slavinskis, Andris
AU - Mughal, Muhammad Rizwan
AU - Praks, Jaan
PY - 2022/4
Y1 - 2022/4
N2 - This article demonstrates the performance of an improved particle swarm optimization (PSO) algorithm with scalar checking and rotation axis fitting objectives using in-orbit data, which is obtained from two CubeSats missions, Aalto-1 and ESTCube-1, as well as simulation as reference. The improved algorithm uses sequential objectives refinement process to combine the two optimization objectives. This improvement addresses some challenges of magnetometer calibration when using in-orbit data. First, the change in the magnetic field vector direction at different points in orbit which is uncorrelated to the rotation of the spacecraft itself. Second, the uncertainty of the rotation axis information used as the reference, e.g., from gyroscope noise. Third, the available data set is heavily affected by the rotation mode of the spacecraft, which imposes some limitation in the rotation axis information needed by the algorithm. The improved PSO algorithm is applied on simulated data in order to analyze the calibration performance under different spacecraft tumbling rates and noise levels. In ideal condition (varying rotation axis during measurements and sufficient sampling rate relative to the spin rate), the rotation axis fitting objective can reach ∼0.1° of correction accuracy.
AB - This article demonstrates the performance of an improved particle swarm optimization (PSO) algorithm with scalar checking and rotation axis fitting objectives using in-orbit data, which is obtained from two CubeSats missions, Aalto-1 and ESTCube-1, as well as simulation as reference. The improved algorithm uses sequential objectives refinement process to combine the two optimization objectives. This improvement addresses some challenges of magnetometer calibration when using in-orbit data. First, the change in the magnetic field vector direction at different points in orbit which is uncorrelated to the rotation of the spacecraft itself. Second, the uncertainty of the rotation axis information used as the reference, e.g., from gyroscope noise. Third, the available data set is heavily affected by the rotation mode of the spacecraft, which imposes some limitation in the rotation axis information needed by the algorithm. The improved PSO algorithm is applied on simulated data in order to analyze the calibration performance under different spacecraft tumbling rates and noise levels. In ideal condition (varying rotation axis during measurements and sufficient sampling rate relative to the spin rate), the rotation axis fitting objective can reach ∼0.1° of correction accuracy.
KW - Calibration
KW - calibration
KW - Gyroscopes
KW - Magnetic separation
KW - Magnetometer
KW - Magnetometers
KW - Mathematical models
KW - nanosatellite
KW - particle swarm optimization
KW - rotation axis fitting
KW - Rotation measurement
KW - Space vehicles
UR - http://www.scopus.com/inward/record.url?scp=85118577278&partnerID=8YFLogxK
U2 - 10.1109/TAES.2021.3122514
DO - 10.1109/TAES.2021.3122514
M3 - Article
AN - SCOPUS:85118577278
SN - 0018-9251
VL - 58
SP - 1211
EP - 1223
JO - IEEE Transactions on Aerospace and Electronic Systems
JF - IEEE Transactions on Aerospace and Electronic Systems
IS - 2
ER -