VC++.net在计算天文偏振光QU平面参数中的应用  

The Application of Caculating the QU Plane Parameters Using Astronomical Polarization Data Based on VC++.net Development Environment

作　　者：韦伟[1] 刘伟[2] 史建春[2] 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)

机构地区：[1]南京理工大学紫金学院,江苏南京210046 [2]中国科学院紫金山天文台,江苏南京210023

出　　处：《软件》2019年第1期22-25,共4页Software

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.

关 键 词：偏振观测 MFC编程 数据处理 

分 类 号：TP311.11[自动化与计算机技术—计算机软件与理论]