On Increasing the Accuracy of Star Trackers to Subsecond Levels
- 作者: Zacharov A.I.1, Krusanova N.L.1, Moskatiniev I.V.2, Prohorov M.E.1, Stekol’shchikov O.Y.1, Sysoev V.K.2, Tuchin M.S.1, Yudin A.D.2
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隶属关系:
- Sternberg Astronomical Institute
- Lavochkin Association
- 期: 卷 52, 编号 7 (2018)
- 页面: 636-643
- 栏目: Article
- URL: https://journals.rcsi.science/0038-0946/article/view/171168
- DOI: https://doi.org/10.1134/S0038094618070201
- ID: 171168
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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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