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Implementation of a real-time star centroid extraction algorithm with high speed and superior denoising ability
Star tracker is the most precise attitude measuring device, and its advantages include a high resolution and high update rate. Star centroid extraction, which is a very time-consuming process, has great influence on the attitude update rate. This paper proposes a real-time star centroid extraction a...
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Published in: | Applied optics (2004) 2022-04, Vol.61 (11), p.3115 |
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container_issue | 11 |
container_start_page | 3115 |
container_title | Applied optics (2004) |
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creator | Ding, Jianqun Dai, Dongkai Tan, Wenfeng Wang, Xingshu Qin, Shiqiao |
description | Star tracker is the most precise attitude measuring device, and its advantages include a high resolution and high update rate. Star centroid extraction, which is a very time-consuming process, has great influence on the attitude update rate. This paper proposes a real-time star centroid extraction algorithm based on a field programmable gate array. First, a 1D top-hat filter is used for star segmentation, which is suitable for both uniform and nonuniform background conditions. Second, multichannel image data is reorganized together into a complete frame through image stitching, which prevents the star spots on the channel boundary from being divided into different parts. Finally, star coordinates are extracted by the center-of-mass algorithm. For an image sensor with a resolution of 2048×2048 pixels, simulation results conducted by a ModelSim simulator show that the star centroid processing time of a single frame is roughly 5.2 ms. Real night experiments demonstrate that the standard deviation of a star centroid error is within 10
pixel and the standard deviation of attitude is (2.6 2.2 12.0) arcseconds, which proves that the proposed star centroid extraction algorithm can work continuously and stably. |
doi_str_mv | 10.1364/AO.450502 |
format | article |
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pixel and the standard deviation of attitude is (2.6 2.2 12.0) arcseconds, which proves that the proposed star centroid extraction algorithm can work continuously and stably.</description><subject>Algorithms</subject><subject>Attitudes</subject><subject>Centroids</subject><subject>Field programmable gate arrays</subject><subject>Image segmentation</subject><subject>Measuring instruments</subject><subject>Pixels</subject><subject>Real time</subject><subject>Standard deviation</subject><subject>Stitching</subject><issn>1559-128X</issn><issn>2155-3165</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNo9kMtOwzAQRS0EoqWw4AeQJVYsUvyInXhZIR6VKnUDErvIjp3WVRIH2xH07zG0sJk7mjlzR7oAXGM0x5Tn94v1PGeIIXICpgQzllHM2SmYplZkmJTvE3ARwg4hynJRnINJ0iLNiylwy25oTWf6KKN1PXQNlNAb2WbRdgaGKD2s09Y7q6H5il7Wv5xsN87buO3gZ6pwazdbGAZjNJS9hmEcjLfOQ216Z4PtN1Aq29q4vwRnjWyDuTrqDLw9Pb4-vGSr9fPyYbHKaszKIiO4FIxqlROpOC6KQnFNiaSEaiSERhw1uq4xIqosUY25ErlgSguFjRIYF3QGbg--g3cfowmx2rnR9-llRXgKgadbkai7A1V7F4I3TTV420m_rzCqfqKtFuvqEG1ib46Oo-qM_if_sqTfOgV0Dw</recordid><startdate>20220410</startdate><enddate>20220410</enddate><creator>Ding, Jianqun</creator><creator>Dai, Dongkai</creator><creator>Tan, Wenfeng</creator><creator>Wang, Xingshu</creator><creator>Qin, Shiqiao</creator><general>Optical Society of America</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7SP</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20220410</creationdate><title>Implementation of a real-time star centroid extraction algorithm with high speed and superior denoising ability</title><author>Ding, Jianqun ; Dai, Dongkai ; Tan, Wenfeng ; Wang, Xingshu ; Qin, Shiqiao</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1587-218953db42ab61777b6d32a323d099d060fdcc102b880c16b9495bd9b1eb91173</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Algorithms</topic><topic>Attitudes</topic><topic>Centroids</topic><topic>Field programmable gate arrays</topic><topic>Image segmentation</topic><topic>Measuring instruments</topic><topic>Pixels</topic><topic>Real time</topic><topic>Standard deviation</topic><topic>Stitching</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ding, Jianqun</creatorcontrib><creatorcontrib>Dai, Dongkai</creatorcontrib><creatorcontrib>Tan, Wenfeng</creatorcontrib><creatorcontrib>Wang, Xingshu</creatorcontrib><creatorcontrib>Qin, Shiqiao</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>Electronics & Communications Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Applied optics (2004)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ding, Jianqun</au><au>Dai, Dongkai</au><au>Tan, Wenfeng</au><au>Wang, Xingshu</au><au>Qin, Shiqiao</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Implementation of a real-time star centroid extraction algorithm with high speed and superior denoising ability</atitle><jtitle>Applied optics (2004)</jtitle><addtitle>Appl Opt</addtitle><date>2022-04-10</date><risdate>2022</risdate><volume>61</volume><issue>11</issue><spage>3115</spage><pages>3115-</pages><issn>1559-128X</issn><eissn>2155-3165</eissn><abstract>Star tracker is the most precise attitude measuring device, and its advantages include a high resolution and high update rate. Star centroid extraction, which is a very time-consuming process, has great influence on the attitude update rate. This paper proposes a real-time star centroid extraction algorithm based on a field programmable gate array. First, a 1D top-hat filter is used for star segmentation, which is suitable for both uniform and nonuniform background conditions. Second, multichannel image data is reorganized together into a complete frame through image stitching, which prevents the star spots on the channel boundary from being divided into different parts. Finally, star coordinates are extracted by the center-of-mass algorithm. For an image sensor with a resolution of 2048×2048 pixels, simulation results conducted by a ModelSim simulator show that the star centroid processing time of a single frame is roughly 5.2 ms. Real night experiments demonstrate that the standard deviation of a star centroid error is within 10
pixel and the standard deviation of attitude is (2.6 2.2 12.0) arcseconds, which proves that the proposed star centroid extraction algorithm can work continuously and stably.</abstract><cop>United States</cop><pub>Optical Society of America</pub><pmid>35471287</pmid><doi>10.1364/AO.450502</doi></addata></record> |
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source | Optica Publishing Group Journals |
subjects | Algorithms Attitudes Centroids Field programmable gate arrays Image segmentation Measuring instruments Pixels Real time Standard deviation Stitching |
title | Implementation of a real-time star centroid extraction algorithm with high speed and superior denoising ability |
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