• 主题
高级搜索  >
历史搜索 清空历史
首页> 外文会议>International Conference on Optics and Photonics 2015 >Two-channel imaging system for the White light Active Region Monitor (WARM) telescope at Kodaikanal Observatory: design, development, and first images
【24h】

Two-channel imaging system for the White light Active Region Monitor (WARM) telescope at Kodaikanal Observatory: design, development, and first images

机译：Kodaikanal天文台的白光有源区域监视器（WARM）望远镜的两通道成像系统：设计，开发和第一张图像

获取原文
获取原文并翻译 | 示例
页面导航
  • 摘要
  • 著录项
  • 相似文献
  • 相关主题

摘要

One of the three planned back-end systems for the proposed National Large Solar Telescope (NLST) is the Solar Dynamics Imaging System (SDIS) which is intended to obtain near simultaneous images in multiple wavelengths. As a first step, a prototype system with two channel imaging has been developed and installed at the back-end of the White light Active Region Monitor (WARM) telescope at Kodaikanal Observatory. A two-mirror Coelostat serves as a light feeding system to a refracting objective while an optical breadboard serves as a platform for the back-end instruments. A re-imaging system is used before the prime focus to get two light channels for the observations in two wavelengths. The re-imaging system is designed using ZEMAX and the alignment of the system is done using a laser. Full disk images are obtained using a red filter (674.2nm/10nm) and a G-band filter (430.5nm/0.84nm). Design aspects of the re-imaging system, preliminary observations and image reduction methods are described in this paper.
机译：拟议的国家大型太阳望远镜（NLST）计划的三个后端系统之一是太阳动力学成像系统（SDIS），该系统旨在获取近乎同时的多种波长的图像。第一步，开发了具有两个通道成像的原型系统，并将其安装在Kodaikanal天文台的白光有源区域监视器（WARM）望远镜的后端。两面镜腔镜用作折射物镜的光馈送系统，而光学面包板则用作后端仪器的平台。在主焦点之前使用重新成像系统，以获取用于观察两个波长的两个光通道。使用ZEMAX设计重新成像系统，并使用激光对系统进行对准。使用红色滤镜（674.2nm / 10nm）和G波段滤镜（430.5nm / 0.84nm）获得全盘图像。本文介绍了重新成像系统的设计方面，初步观察和图像缩小方法。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱：kefu@zhangqiaokeyan.com

京公网安备：11010802029741号 ICP备案号：京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有

  • 客服微信

  • 服务号