An End-to-End Identification Algorithm for Smearing Star Image

In the previous study, there were a few direct star identification (star-ID) algorithms for smearing star image. An end-to-end star-ID algorithm is proposed in this article, to directly identify the smearing image from star sensors with fast attitude maneuvering. Combined with convolutional neural n...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Jinliang Han, Xiubin Yang, Tingting Xu, Zongqiang Fu, Lin Chang, Chunlei Yang, Guang Jin
Formato: article
Lenguaje:EN
Publicado: MDPI AG 2021
Materias:
Q
Acceso en línea:https://doaj.org/article/8f4a876727d04fac8f96eb7b077fcbae
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
id oai:doaj.org-article:8f4a876727d04fac8f96eb7b077fcbae
record_format dspace
spelling oai:doaj.org-article:8f4a876727d04fac8f96eb7b077fcbae2021-11-25T18:54:06ZAn End-to-End Identification Algorithm for Smearing Star Image10.3390/rs132245412072-4292https://doaj.org/article/8f4a876727d04fac8f96eb7b077fcbae2021-11-01T00:00:00Zhttps://www.mdpi.com/2072-4292/13/22/4541https://doaj.org/toc/2072-4292In the previous study, there were a few direct star identification (star-ID) algorithms for smearing star image. An end-to-end star-ID algorithm is proposed in this article, to directly identify the smearing image from star sensors with fast attitude maneuvering. Combined with convolutional neural networks and the self-attention mechanism of transformer encoder, the algorithm can effectively classify the smearing image and identify the star. Through feature extraction and position encoding, neural networks learn the position of stars to generate semantic information and realize the end-to-end identification for the smearing star image. The algorithm can also solve the problem of low identification rate due to smearing of long exposure time for images. A dataset of dynamic stars is analyzed and constructed based on multiple angular velocities. Experiment results show that, compared with representative algorithms, the identification rate of the proposed algorithm is improved at high angular velocities. When the three-axis angular velocity is 10°/s, the rate is still 60.4%. At the same time, the proposed algorithm has good robustness to position noise and magnitude noise.Jinliang HanXiubin YangTingting XuZongqiang FuLin ChangChunlei YangGuang JinMDPI AGarticlestar identificationend-to-end identificationsmearing imagetransformer encoderScienceQENRemote Sensing, Vol 13, Iss 4541, p 4541 (2021)
institution DOAJ
collection DOAJ
language EN
topic star identification
end-to-end identification
smearing image
transformer encoder
Science
Q
spellingShingle star identification
end-to-end identification
smearing image
transformer encoder
Science
Q
Jinliang Han
Xiubin Yang
Tingting Xu
Zongqiang Fu
Lin Chang
Chunlei Yang
Guang Jin
An End-to-End Identification Algorithm for Smearing Star Image
description In the previous study, there were a few direct star identification (star-ID) algorithms for smearing star image. An end-to-end star-ID algorithm is proposed in this article, to directly identify the smearing image from star sensors with fast attitude maneuvering. Combined with convolutional neural networks and the self-attention mechanism of transformer encoder, the algorithm can effectively classify the smearing image and identify the star. Through feature extraction and position encoding, neural networks learn the position of stars to generate semantic information and realize the end-to-end identification for the smearing star image. The algorithm can also solve the problem of low identification rate due to smearing of long exposure time for images. A dataset of dynamic stars is analyzed and constructed based on multiple angular velocities. Experiment results show that, compared with representative algorithms, the identification rate of the proposed algorithm is improved at high angular velocities. When the three-axis angular velocity is 10°/s, the rate is still 60.4%. At the same time, the proposed algorithm has good robustness to position noise and magnitude noise.
format article
author Jinliang Han
Xiubin Yang
Tingting Xu
Zongqiang Fu
Lin Chang
Chunlei Yang
Guang Jin
author_facet Jinliang Han
Xiubin Yang
Tingting Xu
Zongqiang Fu
Lin Chang
Chunlei Yang
Guang Jin
author_sort Jinliang Han
title An End-to-End Identification Algorithm for Smearing Star Image
title_short An End-to-End Identification Algorithm for Smearing Star Image
title_full An End-to-End Identification Algorithm for Smearing Star Image
title_fullStr An End-to-End Identification Algorithm for Smearing Star Image
title_full_unstemmed An End-to-End Identification Algorithm for Smearing Star Image
title_sort end-to-end identification algorithm for smearing star image
publisher MDPI AG
publishDate 2021
url https://doaj.org/article/8f4a876727d04fac8f96eb7b077fcbae
work_keys_str_mv AT jinlianghan anendtoendidentificationalgorithmforsmearingstarimage
AT xiubinyang anendtoendidentificationalgorithmforsmearingstarimage
AT tingtingxu anendtoendidentificationalgorithmforsmearingstarimage
AT zongqiangfu anendtoendidentificationalgorithmforsmearingstarimage
AT linchang anendtoendidentificationalgorithmforsmearingstarimage
AT chunleiyang anendtoendidentificationalgorithmforsmearingstarimage
AT guangjin anendtoendidentificationalgorithmforsmearingstarimage
AT jinlianghan endtoendidentificationalgorithmforsmearingstarimage
AT xiubinyang endtoendidentificationalgorithmforsmearingstarimage
AT tingtingxu endtoendidentificationalgorithmforsmearingstarimage
AT zongqiangfu endtoendidentificationalgorithmforsmearingstarimage
AT linchang endtoendidentificationalgorithmforsmearingstarimage
AT chunleiyang endtoendidentificationalgorithmforsmearingstarimage
AT guangjin endtoendidentificationalgorithmforsmearingstarimage
_version_ 1718410601747709952