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Guide Star Selection for the Three-FOV Daytime Star Sensor
To realize the application of the star sensor in the all-day carrier platform, a three-field-of-view (three-FOV) star sensor in short-wave infrared (SWIR) band is considered. This new prototype employs new techniques that can improve the detection capability of the star sensor, when the huge size of...
Autores principales: | , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
MDPI
2019
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6470773/ https://www.ncbi.nlm.nih.gov/pubmed/30934629 http://dx.doi.org/10.3390/s19061457 |
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author | Wu, Liang Xu, Qian Wang, Haojing Lyu, Hongwu Li, Kaipeng |
author_facet | Wu, Liang Xu, Qian Wang, Haojing Lyu, Hongwu Li, Kaipeng |
author_sort | Wu, Liang |
collection | PubMed |
description | To realize the application of the star sensor in the all-day carrier platform, a three-field-of-view (three-FOV) star sensor in short-wave infrared (SWIR) band is considered. This new prototype employs new techniques that can improve the detection capability of the star sensor, when the huge size of star identification feature database becomes a big obstacle. Hence, a way to thin the guide star catalog for three-FOV daytime star sensor is studied. Firstly, an introduction of three-FOV star sensor and an example of three-FOV daytime star sensor with narrow FOV are presented. According to this model and the requirement of triangular star identification method, two constraints based on the number and the brightness of the stars in FOV are put forward for guide star selection. Then on the basis of these constraints, the improved spherical spiral method (ISSM) is proposed and the optimal number of reference points of ISSM is discussed. Finally, to demonstrate the performance of the ISSM, guide star catalogs are generated by ISSM, magnitude filter method (MFM), 1st order self-organizing guide star selection method (1st-SOPM) and the spherical spiral method (SSM), respectively. The results show that the guide star catalog generated by ISSM has the smallest size and the number and brightness characteristics of its guide stars are better than the other methods. ISSM is effective for the guide star selection in the three-FOV daytime star sensor. |
format | Online Article Text |
id | pubmed-6470773 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2019 |
publisher | MDPI |
record_format | MEDLINE/PubMed |
spelling | pubmed-64707732019-04-26 Guide Star Selection for the Three-FOV Daytime Star Sensor Wu, Liang Xu, Qian Wang, Haojing Lyu, Hongwu Li, Kaipeng Sensors (Basel) Article To realize the application of the star sensor in the all-day carrier platform, a three-field-of-view (three-FOV) star sensor in short-wave infrared (SWIR) band is considered. This new prototype employs new techniques that can improve the detection capability of the star sensor, when the huge size of star identification feature database becomes a big obstacle. Hence, a way to thin the guide star catalog for three-FOV daytime star sensor is studied. Firstly, an introduction of three-FOV star sensor and an example of three-FOV daytime star sensor with narrow FOV are presented. According to this model and the requirement of triangular star identification method, two constraints based on the number and the brightness of the stars in FOV are put forward for guide star selection. Then on the basis of these constraints, the improved spherical spiral method (ISSM) is proposed and the optimal number of reference points of ISSM is discussed. Finally, to demonstrate the performance of the ISSM, guide star catalogs are generated by ISSM, magnitude filter method (MFM), 1st order self-organizing guide star selection method (1st-SOPM) and the spherical spiral method (SSM), respectively. The results show that the guide star catalog generated by ISSM has the smallest size and the number and brightness characteristics of its guide stars are better than the other methods. ISSM is effective for the guide star selection in the three-FOV daytime star sensor. MDPI 2019-03-25 /pmc/articles/PMC6470773/ /pubmed/30934629 http://dx.doi.org/10.3390/s19061457 Text en © 2019 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/). |
spellingShingle | Article Wu, Liang Xu, Qian Wang, Haojing Lyu, Hongwu Li, Kaipeng Guide Star Selection for the Three-FOV Daytime Star Sensor |
title | Guide Star Selection for the Three-FOV Daytime Star Sensor |
title_full | Guide Star Selection for the Three-FOV Daytime Star Sensor |
title_fullStr | Guide Star Selection for the Three-FOV Daytime Star Sensor |
title_full_unstemmed | Guide Star Selection for the Three-FOV Daytime Star Sensor |
title_short | Guide Star Selection for the Three-FOV Daytime Star Sensor |
title_sort | guide star selection for the three-fov daytime star sensor |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6470773/ https://www.ncbi.nlm.nih.gov/pubmed/30934629 http://dx.doi.org/10.3390/s19061457 |
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