The effect of gravity gradient torque disturbances (which is an order of magnitude greater than the other torque disturbances and is sinusoidal with a frequency of two cycles per orbit) on pointing accuracy can be predicted very precisely. However, since the sensor noise such as star tracker and gyro inherent noise, is random, their effect can only be predicted statistically. The most common method used is computer simulation with appropriate sensor model and adjusting spacecraft control laws for minimum pointing error, as presented by Harris (1972). The general investigation outlined theoretically relates spacecraft controls to pointing accuracy in terms of the sensor noise power spectrum. The results are presented in graphical form.
Rigid body mode pointing accuracy and stability criteria for an orbiting spacecraft
1974-08-01
Miscellaneous
No indication
English
Galileo spacecraft pointing accuracy analysis
NTRS | 1982
|Galileo spacecraft pointing accuracy analysis
AIAA | 1982
|