• 文献检索
  • 文档翻译
  • 深度研究
  • 学术资讯
  • Suppr Zotero 插件Zotero 插件
  • 邀请有礼
  • 套餐&价格
  • 历史记录
应用&插件
Suppr Zotero 插件Zotero 插件浏览器插件Mac 客户端Windows 客户端微信小程序
定价
高级版会员购买积分包购买API积分包
服务
文献检索文档翻译深度研究API 文档MCP 服务
关于我们
关于 Suppr公司介绍联系我们用户协议隐私条款
关注我们

Suppr 超能文献

核心技术专利:CN118964589B侵权必究
粤ICP备2023148730 号-1Suppr @ 2026

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验

硅视像管光谱测定法及其在太阳研究中的红外探测能力。

Silicon vidicon spectrometry and its infrared capabilities for solar research.

作者信息

Pasachoff J M, Muzyka D F, Schierer J P

出版信息

Appl Opt. 1976 Nov 1;15(11):2884-90. doi: 10.1364/AO.15.002884.

DOI:10.1364/AO.15.002884
PMID:20165506
Abstract

A rapid-scanning silicon vidicon spectrometer is described; its sensitivity extends from 300 nm to 1080 nm, where even at that wavelength it has enough sensitivity to allow observation under eclipse conditions of a pair of forbidden spectral lines from twelve-times ionized iron that are sensitive indicators of the electron density in the solar corona. Past observational work on these ir lines is reviewed, and our vidicon observations made during the 1973 total solar eclipse are discussed. The vidicon target, the scanning procedure, and the advantages of the spectrometer are described. At the 1973 eclipse, the 1074.7-nm line was detected and an upper limit set for the 1079.8-nm line at a height of 1.4 solar radii. The resultant limit to the ratio of intensities gives electron densities in agreement with those derived from other methods and is consistent with observations made at lower heights; this indicates that the only previous eclipse observation of the ratio at this height was contaminated by scattered light. Our 1973 eclipse observations were limited by the high ambient temperature of the vidicon, by the less-than-optimum match of the focal ratios of the telescope and spectrometer optics, and by problems with the pointing during totality. These difficulties can be overcome, and the silicon vidicon spectrometer will be useful in both eclipse and noneclipse solar observing to map the coronal ir spectrum and also to study the [Fe XIII] ir and interlocking uv lines.

摘要

本文描述了一种快速扫描硅视像管光谱仪;其灵敏度范围为300纳米至1080纳米,即使在该波长下,它也具有足够的灵敏度,能够在日食条件下观测到来自十二次电离铁的一对禁戒谱线,这些谱线是日冕中电子密度的灵敏指标。回顾了过去对这些红外谱线的观测工作,并讨论了我们在1973年日全食期间进行的视像管观测。描述了视像管靶、扫描程序以及该光谱仪的优点。在1973年日食期间,检测到了1074.7纳米的谱线,并在1.4个太阳半径的高度上为1079.8纳米的谱线设定了上限。由此得出的强度比限制给出的电子密度与从其他方法得出的结果一致,并且与在较低高度进行的观测结果相符;这表明之前在该高度对该比值进行的唯一一次日食观测受到了散射光的影响。我们1973年的日食观测受到视像管周围环境温度过高、望远镜和光谱仪光学系统的焦比匹配不理想以及全食期间指向问题的限制。这些困难是可以克服的,硅视像管光谱仪在日食和非日食太阳观测中都将有助于绘制日冕红外光谱,还可用于研究[Fe XIII]红外谱线和相互关联的紫外谱线。

相似文献

1
Silicon vidicon spectrometry and its infrared capabilities for solar research.硅视像管光谱测定法及其在太阳研究中的红外探测能力。
Appl Opt. 1976 Nov 1;15(11):2884-90. doi: 10.1364/AO.15.002884.
2
Studies of coronal lines with electronic cameras during the eclipse of 7 march 1970.1970年3月7日日食期间用电子相机对日冕谱线的研究。
Appl Opt. 1970 Dec 1;9(12):2643-7. doi: 10.1364/AO.9.002643.
3
Ground-based observation of emission lines from the corona of a red-dwarf star.对红矮星日冕发射线的地面观测。
Nature. 2001 Aug 2;412(6846):508-10. doi: 10.1038/35087513.
4
Radiometric calibration of the telescope and ultraviolet spectrometer SUMER on SOHO.
Appl Opt. 1996 Sep 1;35(25):5125-33. doi: 10.1364/AO.35.005125.
5
Spectral changes in the zenith skylight during total solar eclipses.日全食期间天顶 skylight 的光谱变化。 (注:这里“skylight”可能有误,推测可能是“sky light”即“天空光”,但按照要求未做修改)
Appl Opt. 1971 Jun 1;10(6):1225-31. doi: 10.1364/AO.10.001225.
6
No evidence of a circumsolar dust ring from infrared observations of the 1991 solar eclipse.没有证据表明在 1991 年日蚀的红外观测中有一个环绕太阳的尘埃环。
Science. 1992 Sep 4;257(5075):1377-80. doi: 10.1126/science.257.5075.1377.
7
[Design of optical system for solar extreme-ultraviolet imaging spectrometer].[太阳极紫外成像光谱仪光学系统设计]
Guang Pu Xue Yu Guang Pu Fen Xi. 2012 Mar;32(3):834-8.
8
Intensifier silicon vidicon spectrophotometer for line profile studies in astronomy.
Appl Opt. 1981 Feb 15;20(4):665-9. doi: 10.1364/AO.20.000665.
9
Observing the solar corona with a tunable Fabry-Perot filter.使用可调谐法布里-珀罗滤光片观测日冕。
Appl Opt. 2008 Nov 1;47(31):5744-9. doi: 10.1364/ao.47.005744.
10
Zenith skylight intensity and color during the total solar eclipse of 20 July 1963.
Appl Opt. 1966 May 1;5(5):787-92. doi: 10.1364/AO.5.000787.