中国惯性技术学报
中國慣性技術學報
중국관성기술학보
JOURNAL OF CHINESE INERTIAL TECHNOLOGY
2014年
3期
352-356
,共5页
崔祥祥%王宏力%陆敬辉%乔兴%邓长智%杨小冈
崔祥祥%王宏力%陸敬輝%喬興%鄧長智%楊小岡
최상상%왕굉력%륙경휘%교흥%산장지%양소강
星敏感器%星图识别%角距匹配%球面多边形%k向量技术
星敏感器%星圖識彆%角距匹配%毬麵多邊形%k嚮量技術
성민감기%성도식별%각거필배%구면다변형%k향량기술
star tracker%star identification%angular distance match%spherical polygon search%k-vector technique
为了实现多视场星敏感器的快速星图识别,针对球面多边形搜索星图识别算法面临单个星对角距匹配无法实现观测星与导航星一一对应造成计算量增加问题,提出了基于公共星检验的改进球面多边形搜索星图识别算法。使用三颗观测星形成的其中两个星对进行角距匹配,并基于两观测星对的公共星连接条件,实现了角距匹配中错误星对结果的剔除,以及匹配星对中观测星与导航星的一一对应,减少了算法计算量;同时,在验证匹配星对时另选三颗观测星之外的一颗观测星,间接实现了四星模式验证,提高了改进算法的识别率。仿真结果表明,改进算法的识别速度和识别率要明显高于原算法,且在星像位置误差为0.1~0.5像素时,改进算法的平均识别时间约为原算法的1/10。
為瞭實現多視場星敏感器的快速星圖識彆,針對毬麵多邊形搜索星圖識彆算法麵臨單箇星對角距匹配無法實現觀測星與導航星一一對應造成計算量增加問題,提齣瞭基于公共星檢驗的改進毬麵多邊形搜索星圖識彆算法。使用三顆觀測星形成的其中兩箇星對進行角距匹配,併基于兩觀測星對的公共星連接條件,實現瞭角距匹配中錯誤星對結果的剔除,以及匹配星對中觀測星與導航星的一一對應,減少瞭算法計算量;同時,在驗證匹配星對時另選三顆觀測星之外的一顆觀測星,間接實現瞭四星模式驗證,提高瞭改進算法的識彆率。倣真結果錶明,改進算法的識彆速度和識彆率要明顯高于原算法,且在星像位置誤差為0.1~0.5像素時,改進算法的平均識彆時間約為原算法的1/10。
위료실현다시장성민감기적쾌속성도식별,침대구면다변형수색성도식별산법면림단개성대각거필배무법실현관측성여도항성일일대응조성계산량증가문제,제출료기우공공성검험적개진구면다변형수색성도식별산법。사용삼과관측성형성적기중량개성대진행각거필배,병기우량관측성대적공공성련접조건,실현료각거필배중착오성대결과적척제,이급필배성대중관측성여도항성적일일대응,감소료산법계산량;동시,재험증필배성대시령선삼과관측성지외적일과관측성,간접실현료사성모식험증,제고료개진산법적식별솔。방진결과표명,개진산법적식별속도화식별솔요명현고우원산법,차재성상위치오차위0.1~0.5상소시,개진산법적평균식별시간약위원산법적1/10。
To realize the rapid identification of the stars in multiple fields-of-view star trackers, a modified star identification algorithm by spherical polygon search is proposed based on common star checking to solve the ambiguity of observed star and corresponding guide star in matched star pairs, which increases the amount of computations in the original spherical polygon search star identification algorithm. Two observed star pairs made up of three observed stars are matched to guide star pairs based on angular distance. The common star connection of the two observed star pairs is utilized to kick out the wrong guide star pair matches and confirm the corresponding guide star to the observed star, which reduces the computation in the modified algorithm. Meanwhile, another observed star, not the aforementioned three observed stars, is selected to verify the matched star pairs, which improves the identification rate for “four-star pattern” is indirectly formed. Simulation results show that the modified algorithm is better than the original algorithm at both velocity and identification rate. When the star position error was between 0.1 pixel and 0.5 pixel, the mean identification time with the modified algorithm was both about 1/10 of that with the original algorithm.