Independent thesis Advanced level (degree of Master (Two Years)), 20 credits / 30 HE credits
In this paper two Unscented Kalman Filters (UKF) are implemented to solve the
estimation of a satellite's position in orbit and its orientation relative to Earth's Centered
Inertial frame. Their aim is to see if an absolute position accuracy of less than 1 km
and an orientation estimation to less than 1
0 are possible for a 3U CubeSat with GPS,
sun sensors, magnetometers and a star tracker as sensors.
The orbit UKF is based on a Runge Kutta 7(8)
th-order integration method for orbit
propagation. The dynamic model uses perturbational accelerations due to Earth's geopotential,
the gravity of the Moon and the Sun, atmospheric drag and solar pressure.
The state of the lter is identical to the observation vector and consists of position and
velocity vectors of the satellite. The GPS receiver is used for measurements. Emphasis
has been put on the sampling rate of the GPS receiver as its availability is constrained
by the satellite's power limitations. The state of the attitude UKF consists of an error
quaternion, angular velocities and magnetometer bias. The sun sensors, magnetometers
and the star tracker are used for measurements. Dierent sensor combinations have been
simulated with the purpose of determining their inuence on the estimated attitude.
The results of the simulations indicate that an absolute position error of less than
1 km is feasible for sampling times of 15 minutes or less (approximately 6 per orbit).
Furthermore an accuracy of less than 1
0 is achieved by using the star tracker for attitude
determination either alone or in combination with the other sensors.
2015. , 75 p.