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Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions
Under the dynamic working conditions of a star sensor, motion blur of the star will appear due to its energy dispersion during imaging, leading to the degradation of the star centroid accuracy and attitude accuracy of the star sensor. To address this, a restoration method of a blurred star image for...
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/PMC6806066/ https://www.ncbi.nlm.nih.gov/pubmed/31554196 http://dx.doi.org/10.3390/s19194127 |
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author | Mu, Zhiya Wang, Jun He, Xin Wei, Zhonghui He, Jiawei Zhang, Lei Lv, You He, Dinglong |
author_facet | Mu, Zhiya Wang, Jun He, Xin Wei, Zhonghui He, Jiawei Zhang, Lei Lv, You He, Dinglong |
author_sort | Mu, Zhiya |
collection | PubMed |
description | Under the dynamic working conditions of a star sensor, motion blur of the star will appear due to its energy dispersion during imaging, leading to the degradation of the star centroid accuracy and attitude accuracy of the star sensor. To address this, a restoration method of a blurred star image for a star sensor under dynamic conditions is presented in this paper. First, a kinematic model of the star centroid and the degradation function of blurred star image under different conditions are analyzed. Then, an improved curvature filtering method based on energy function is proposed to remove the noise and improve the signal-to-noise ratio of the star image. Finally, the Richardson Lucy algorithm is used and the termination condition of the iterative equation is established by using the star centroid coordinates in three consecutive frames of restored images to ensure the restoration effect of the blurred star image and the accuracy of the star centroid coordinates. Under the dynamic condition of 0~4°/s, the proposed algorithm can effectively improve the signal-to-noise ratio of a blurred star image and maintain an error of the star centroid coordinates that is less than 0.1 pixels, which meets the requirement for high centroid accuracy. |
format | Online Article Text |
id | pubmed-6806066 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2019 |
publisher | MDPI |
record_format | MEDLINE/PubMed |
spelling | pubmed-68060662019-11-07 Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions Mu, Zhiya Wang, Jun He, Xin Wei, Zhonghui He, Jiawei Zhang, Lei Lv, You He, Dinglong Sensors (Basel) Article Under the dynamic working conditions of a star sensor, motion blur of the star will appear due to its energy dispersion during imaging, leading to the degradation of the star centroid accuracy and attitude accuracy of the star sensor. To address this, a restoration method of a blurred star image for a star sensor under dynamic conditions is presented in this paper. First, a kinematic model of the star centroid and the degradation function of blurred star image under different conditions are analyzed. Then, an improved curvature filtering method based on energy function is proposed to remove the noise and improve the signal-to-noise ratio of the star image. Finally, the Richardson Lucy algorithm is used and the termination condition of the iterative equation is established by using the star centroid coordinates in three consecutive frames of restored images to ensure the restoration effect of the blurred star image and the accuracy of the star centroid coordinates. Under the dynamic condition of 0~4°/s, the proposed algorithm can effectively improve the signal-to-noise ratio of a blurred star image and maintain an error of the star centroid coordinates that is less than 0.1 pixels, which meets the requirement for high centroid accuracy. MDPI 2019-09-24 /pmc/articles/PMC6806066/ /pubmed/31554196 http://dx.doi.org/10.3390/s19194127 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 Mu, Zhiya Wang, Jun He, Xin Wei, Zhonghui He, Jiawei Zhang, Lei Lv, You He, Dinglong Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions |
title | Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions |
title_full | Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions |
title_fullStr | Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions |
title_full_unstemmed | Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions |
title_short | Restoration Method of a Blurred Star Image for a Star Sensor Under Dynamic Conditions |
title_sort | restoration method of a blurred star image for a star sensor under dynamic conditions |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6806066/ https://www.ncbi.nlm.nih.gov/pubmed/31554196 http://dx.doi.org/10.3390/s19194127 |
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