NAOC Open IR
三轴稳定GEO卫星漫反射光变特性
唐轶峻; 姜晓军; 王建峰; 魏建彦; 胡景耀
2009
Source Publication光子学报
ISSN1004-4213
Volume000Issue:011Pages:2863
Abstract利用天文测光方法研究了地球同步轨道卫星可见光波段的反射光变特性.以三轴稳定地球同步轨道通讯卫星为研究样本,进行了可见光波段的光学非高分辨成像观测,并使用天文标准星进行定标.基于相位角序列的测光观测数据表明:在大相位角区域卫星光变曲线分布与漫反射光照数学模型计算结果有很好的一致性,以卫星主体和太阳能电池板的漫反射效应为主;而在小相位角区域与漫反射模型计算结果有明显的差异,为卫星的太阳帆板镜面反射效应影响所致.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/53830
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
唐轶峻,姜晓军,王建峰,等. 三轴稳定GEO卫星漫反射光变特性[J]. 光子学报,2009,000(011):2863.
APA 唐轶峻,姜晓军,王建峰,魏建彦,&胡景耀.(2009).三轴稳定GEO卫星漫反射光变特性.光子学报,000(011),2863.
MLA 唐轶峻,et al."三轴稳定GEO卫星漫反射光变特性".光子学报 000.011(2009):2863.
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