机载星跟踪器在日间的设计考虑

Zhu Hailong, Bin Liang, Zhang Tao, Hua Junpeng
{"title":"机载星跟踪器在日间的设计考虑","authors":"Zhu Hailong, Bin Liang, Zhang Tao, Hua Junpeng","doi":"10.1109/CCDC.2015.7162682","DOIUrl":null,"url":null,"abstract":"This paper aims at determining several designing considerations for star tracker which uses on aircraft during daytime at altitudes around 10 km. From analysis of operational environment, the sky background radiation caused by the sun is the main factor which affects the performance of star tracker. In order to research insight, star magnitude model is established to calculate stellar radiation and MODTRAN software is used to obtain the sky background radiation. The contrast of detection, the ratio of stellar radiation and sky background radiation, is defined as the criterion to determine these considerations. Finally, H-band waveband, from 1.5μm to 1.7μm, is chose as the optimal detection waveband due to better comprehensive performance in detection. InGaAs detector is selected for the airborne star tracker after trade-off studies included a comparison in terms of detector format, cost and cooling requirements. Simultaneous measurements with three field of view are determined as the preferred design prototype because of higher detectable limiting magnitude and star detection probability.","PeriodicalId":273292,"journal":{"name":"The 27th Chinese Control and Decision Conference (2015 CCDC)","volume":"45 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2015-05-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"6","resultStr":"{\"title\":\"Designing considerations for airborne star tracker during daytime\",\"authors\":\"Zhu Hailong, Bin Liang, Zhang Tao, Hua Junpeng\",\"doi\":\"10.1109/CCDC.2015.7162682\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"This paper aims at determining several designing considerations for star tracker which uses on aircraft during daytime at altitudes around 10 km. From analysis of operational environment, the sky background radiation caused by the sun is the main factor which affects the performance of star tracker. In order to research insight, star magnitude model is established to calculate stellar radiation and MODTRAN software is used to obtain the sky background radiation. The contrast of detection, the ratio of stellar radiation and sky background radiation, is defined as the criterion to determine these considerations. Finally, H-band waveband, from 1.5μm to 1.7μm, is chose as the optimal detection waveband due to better comprehensive performance in detection. InGaAs detector is selected for the airborne star tracker after trade-off studies included a comparison in terms of detector format, cost and cooling requirements. Simultaneous measurements with three field of view are determined as the preferred design prototype because of higher detectable limiting magnitude and star detection probability.\",\"PeriodicalId\":273292,\"journal\":{\"name\":\"The 27th Chinese Control and Decision Conference (2015 CCDC)\",\"volume\":\"45 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2015-05-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"6\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The 27th Chinese Control and Decision Conference (2015 CCDC)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/CCDC.2015.7162682\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"The 27th Chinese Control and Decision Conference (2015 CCDC)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/CCDC.2015.7162682","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 6

摘要

本文的目的是确定在10公里高度左右的白天飞机上使用的星跟踪器的几个设计注意事项。从运行环境分析来看,太阳引起的天空背景辐射是影响星跟踪器性能的主要因素。为了研究洞察力,建立星等模型计算恒星辐射,使用MODTRAN软件获取天空背景辐射。探测的对比,即恒星辐射与天空背景辐射的比值,被定义为确定这些考虑因素的标准。最终选择1.5μm ~ 1.7μm的h波段作为最优检测波段,其综合检测性能更好。经过权衡研究,包括探测器格式、成本和冷却要求的比较,InGaAs探测器被选择用于机载星跟踪器。由于三视场同时测量具有较高的可探测极限星等和检星概率,因此确定了三视场同时测量作为优选的设计原型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Designing considerations for airborne star tracker during daytime
This paper aims at determining several designing considerations for star tracker which uses on aircraft during daytime at altitudes around 10 km. From analysis of operational environment, the sky background radiation caused by the sun is the main factor which affects the performance of star tracker. In order to research insight, star magnitude model is established to calculate stellar radiation and MODTRAN software is used to obtain the sky background radiation. The contrast of detection, the ratio of stellar radiation and sky background radiation, is defined as the criterion to determine these considerations. Finally, H-band waveband, from 1.5μm to 1.7μm, is chose as the optimal detection waveband due to better comprehensive performance in detection. InGaAs detector is selected for the airborne star tracker after trade-off studies included a comparison in terms of detector format, cost and cooling requirements. Simultaneous measurements with three field of view are determined as the preferred design prototype because of higher detectable limiting magnitude and star detection probability.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信