On Increasing the Accuracy of Star Trackers to Subsecond Levels


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详细

Modern star trackers are based on photodetector arrays such as CCD or CMOS arrays. The accuracy of commercially available devices is ~1–3 arcseconds. However, the development of the space industry calls for higher orientation accuracies, which are needed in laser space communications, monitoring of near-Earth space and space debris, high-precision global mapping, and remote sensing of the Earth. The problems associated with enhancing the accuracy of modern star trackers are discussed.

作者简介

A. Zacharov

Sternberg Astronomical Institute

编辑信件的主要联系方式.
Email: zakh@sai.msu.ru
俄罗斯联邦, Moscow, 119234

N. Krusanova

Sternberg Astronomical Institute

Email: zakh@sai.msu.ru
俄罗斯联邦, Moscow, 119234

I. Moskatiniev

Lavochkin Association

Email: zakh@sai.msu.ru
俄罗斯联邦, Khimki, Moscow oblast, 141400

M. Prohorov

Sternberg Astronomical Institute

Email: zakh@sai.msu.ru
俄罗斯联邦, Moscow, 119234

O. Stekol’shchikov

Sternberg Astronomical Institute

Email: zakh@sai.msu.ru
俄罗斯联邦, Moscow, 119234

V. Sysoev

Lavochkin Association

Email: zakh@sai.msu.ru
俄罗斯联邦, Khimki, Moscow oblast, 141400

M. Tuchin

Sternberg Astronomical Institute

Email: zakh@sai.msu.ru
俄罗斯联邦, Moscow, 119234

A. Yudin

Lavochkin Association

Email: zakh@sai.msu.ru
俄罗斯联邦, Khimki, Moscow oblast, 141400

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