Hiroyuki Kawano, Haruhiko Shimoji, Shoji Yoshikawa, Katsumasa Miyatake, Kazumori Hama, Shuji Nakamura
Optical Engineering, Vol. 45, Issue 12, 124403, (December 2006) https://doi.org/10.1117/1.2402101
TOPICS: Stray light, Star sensors, Sun, Stars, Light scattering, Scattering, Satellites, Optical engineering, Reflection, Charge-coupled devices
We have developed a light-shielding technique for a star sensor that can shorten the baffle length. We achieved a baffle length of 120 mm, two-thirds that of a conventional two-stage baffle. The key idea is that the first lens of the imaging optics is designed as a near-hemispherical (NHS) lens that can work as an angle filter; high-incidence-angle rays are not permitted to be transmitted but low-incidence-angle rays from stars can be. A star sensor system with the new light-shielding technique onboard the SERVIS-1 satellite was launched in October 2003 as an experimental device. Though the in-orbit data verified its fundamental performance in capturing star images, undesirable solar background noise was observed in two corners of the field of view. Ray-trace simulations revealed that slight scattered light on the specular baffle surface entered the NHS lens and reached the corners of the image sensor through a multireflection path inside the lens. We redesigned the baffle and confirmed that stray light was reduced below maximum acceptable levels in a ground test. The star sensor with redesigned baffles is planned to be installed as the main attitude sensor for the SERVIS-2 satellite to be launched in 2008 or later.