色球-光球望远镜

The Chromospheric-Photospheric Telescope Group
{"title":"色球-光球望远镜","authors":"The Chromospheric-Photospheric Telescope Group","doi":"10.1016/0146-6364(80)90021-3","DOIUrl":null,"url":null,"abstract":"<div><p>A twin tube chromospheric-photospheric telescope patrols and observes the solar chromosphere in H<sub>α</sub> and the photosphere photographically and visually at the same time. Both objectives have apertures of 180 mm, and the polarizing interference filter in the main optical path of the chromospheric part has a working wavelength of 6562.78 a (H<sub>α</sub>), a transmission half-width of 0.5 A, and is composed of 10 birefringent crystal elements, of which the last 4 are wide-field elements. Interference filters to cut down light are used in both the chromospheric and the photospherice paths and the solar image is, respectively, 25 and 71 mm in size. Test photographs show a quality that is better than any attained so far in China.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":"4 4","pages":"Pages 329-333"},"PeriodicalIF":0.0000,"publicationDate":"1980-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90021-3","citationCount":"0","resultStr":"{\"title\":\"A chromospheric-photospheric telescope\",\"authors\":\"The Chromospheric-Photospheric Telescope Group\",\"doi\":\"10.1016/0146-6364(80)90021-3\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>A twin tube chromospheric-photospheric telescope patrols and observes the solar chromosphere in H<sub>α</sub> and the photosphere photographically and visually at the same time. Both objectives have apertures of 180 mm, and the polarizing interference filter in the main optical path of the chromospheric part has a working wavelength of 6562.78 a (H<sub>α</sub>), a transmission half-width of 0.5 A, and is composed of 10 birefringent crystal elements, of which the last 4 are wide-field elements. Interference filters to cut down light are used in both the chromospheric and the photospherice paths and the solar image is, respectively, 25 and 71 mm in size. Test photographs show a quality that is better than any attained so far in China.</p></div>\",\"PeriodicalId\":100241,\"journal\":{\"name\":\"Chinese Astronomy\",\"volume\":\"4 4\",\"pages\":\"Pages 329-333\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1980-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0146-6364(80)90021-3\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Chinese Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/0146636480900213\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0146636480900213","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

摘要

双管色球-光球望远镜同时对太阳α中的色球和光球进行摄影和视觉上的巡视和观测。两个物镜的孔径均为180 mm,色球部分主光路的偏振干涉滤光片工作波长为6562.78 a (Hα),透射半宽为0.5 a,由10个双折射晶元组成,其中后4个为宽视场晶元。在色球和光球路径上都使用干涉滤光片来减少光线,太阳图像的尺寸分别为25毫米和71毫米。测试照片显示,其质量比目前在中国获得的任何产品都要好。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
A chromospheric-photospheric telescope

A twin tube chromospheric-photospheric telescope patrols and observes the solar chromosphere in Hα and the photosphere photographically and visually at the same time. Both objectives have apertures of 180 mm, and the polarizing interference filter in the main optical path of the chromospheric part has a working wavelength of 6562.78 a (Hα), a transmission half-width of 0.5 A, and is composed of 10 birefringent crystal elements, of which the last 4 are wide-field elements. Interference filters to cut down light are used in both the chromospheric and the photospherice paths and the solar image is, respectively, 25 and 71 mm in size. Test photographs show a quality that is better than any attained so far in China.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
期刊最新文献
Subject index Errata Author index Supernova remnants of known age and X-radiation The effect of an ellipsoidal distribution of star velocities on galactic density waves
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1