摘要
偏振光观测是天文光学观测的重要方法,尤其在观测恒星爆发,研究黑洞结构和宇宙微波背景方面优势明显。斯托克斯参数组成的QU平面可以反应出偏振光的状态信息。本文介绍了在VC++.net环境下编程计算斯托克斯参数,处理数据的方法。
Polarization observation is an important method of astronomical observation. It has a great advantage in optical band, especially in the research of stars explosion, the structure around the large black hole and the cosmic microwave background and so on. QU plane composed with stokes parameters can reflect the the state information of polarized light. This paper introduce the calculation and process method under VC++.net development environment.
作者
韦伟
刘伟
史建春
WEI Wei;LIU Wei;SHI Jian-chun(Nanjing University of Science and Technology ZiJin College,Nanjing 210046, China;Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China)
出处
《软件》
2019年第1期22-25,共4页
Software
关键词
偏振观测
MFC编程
数据处理
Polarization observation
MFC programing
Data processing