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NVST偏振观测系统的运动控制实现
Alternative TitleThe Movement and Control Realization of NVST Polarization Observation System
覃瑛1; 彭建国1,2; 张涛1; 侯俊峰3; 顾伯忠4; 许骏1
Source Publication天文研究与技术(Astronomical Research & Technology)
2018-07
Volume15Issue:03Pages:315-322
DOI10.14005/j.cnki.issn1672-7673.20180103.010
ClassificationP111.33;tp311.5
Contribution Rank第1完成单位
Indexed ByCSCD
Keyword偏振观测 定标单元 控制方案 远程控制
Abstract

云南天文台的一米新真空太阳望远镜(New Vacuum Solar Telescope,NVST)是我国在太阳物理和空间科学学科上对太阳进行光学和近红外观测的主力设备,其主要科学目标之一是高精度、高时空分辨率的太阳磁场测量。NVST采用机械扫描偏振观测方式,由于其光学系统的结构特性导致望远镜在跟踪太阳的过程中不可避免的引入了随时间变化的偏正效应,因此在进行偏正观测时需要进行系统定标,整个系统由定标单元、分析单元和探测器组成,其间涉及的多个运动部件均有复杂精密的运动要求。针对偏振定标过程和偏振观测过程中各光学件的运动需求,文章给出了定标单元和分析单元的控制要求,实现了不同观测模式时各部件的运动要求。基于TCP/IP协议的远程控制方案,集成了采用串口通讯的各商品驱动控制器,开发了一套在.NET架构下的定标单元控制软件和相应的用户界面,并预留了OCS接口。性能测试表明,系统符合实际观测要求,现已投入使用,为后续的偏振观测奠定了基础。 

Other Abstract

The new Vacuum Solar Telescope (NVST) is one of the most important solar observing systems, one of its main scientific goal includes high precision and high temporal resolution measurement of the solar magnetic field. NVST polarization analysis system should be pre-calibrated before observing, and, due to the structural characteristics of its optical system, NVST inevitably introduces a time-varying biasing effect during the tracking of the sun. Therefore, calibration of the system requires calibration of the system. The whole The system consists of a calibration unit, an analysis unit and a detector. A plurality of moving parts involved in the process have complex and precise movement requirements. This paper is aimed at the motion requirements of each optical component during polarization calibration process and polarization observation, gave the control requirements of the calibration unit and the analysis unit, and realized the movement requirements of the components in different observation modes. Based on TCP/IP protocol remote control program, integrated with serial communication of the commodity drive controller, the software is developed under the .NET architecture and set aside the OCS interface. System performance tests show that, in line with the measured application requirements, is now put into use, for the subsequent polarization observation laid the foundation.

Funding Project国家自然科学基金项目“一米红外太阳望远镜双光束偏振定标测量的理论与技术方法研究”[11373044] ; 国家自然科学基金项目“法珀滤光器控制器研究”[11473067]
Funding Organization国家自然科学基金项目“一米红外太阳望远镜双光束偏振定标测量的理论与技术方法研究”[11373044] ; 国家自然科学基金项目“法珀滤光器控制器研究”[11473067]
Language中文
Subject Area天文学 ; 天文学其他学科 ; 电子、通信与自动控制技术
MOST Discipline Catalogue理学 ; 理学::天文学 ; 工学 ; 工学::电子科学与技术(可授工学、理学学位) ; 工学::信息与通信工程 ; 工学::控制科学与工程
ISSN1672-7673
CSCD IDCSCD:6272012
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/12018
Collection抚仙湖太阳观测站
Corresponding Author许骏
Affiliation1.中国科学院云南天文台,云南 ,昆明 ,650216
2.中国科学院大学,北京 ,100049
3.中国科学院国家天文台,北京 ,100012
4.中国科学院国家天文台南京天文光学技术研究所,江苏 ,南京 ,210042
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
覃瑛,彭建国,张涛,等. NVST偏振观测系统的运动控制实现[J]. 天文研究与技术(Astronomical Research & Technology),2018,15(03):315-322.
APA 覃瑛,彭建国,张涛,侯俊峰,顾伯忠,&许骏.(2018).NVST偏振观测系统的运动控制实现.天文研究与技术(Astronomical Research & Technology),15(03),315-322.
MLA 覃瑛,et al."NVST偏振观测系统的运动控制实现".天文研究与技术(Astronomical Research & Technology) 15.03(2018):315-322.
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