Determination of Spacecraft Attitude and Source Position Using Non-aligned Detectors in Spin-stabilized Satellites

TL;DR

This paper presents methods to determine the attitude of spin-stabilized satellites and the position of celestial sources using non-aligned detectors, accounting for statistical fluctuations and extending to three-axis stabilized satellites.

Contribution

It introduces techniques to estimate satellite orientation and source position from light curves with non-aligned detectors, including cases with known inclination and three-axis stabilization.

Findings

Detector orientation can be estimated from observed light curves.

Satellite attitude and source position can be determined using inclined detectors.

Methods account for statistical fluctuations in measurements.

Abstract

The modulation of high-energy transients' (or steadily emitting sources') light curves due to the imperfect alignment of the detector's view axis with the spin axis in a spin-stabilized satellite is derived. It is shown how the orientation of the detector's view axis with respect to the satellite's spin axis may be estimated using observed light curves. The effects of statistical fluctuations are considered. Conversely, it is shown how the attitude of a spin-axis stabilized satellite as well as the unknown position of a celestial source of high-energy photons may be determined using a detector whose view-axis is intentionally kept inclined and is known accurately beforehand. The case of three-axes stabilized satellites is also discussed.