Solar spectroscopy in the far-ultraviolet-X-ray wavelength regions - Status and prospects
Solar spectroscopy in the far-ultraviolet-X-ray wavelength regions - Status and prospects
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远紫外 X 射线波长区域的太阳光谱 - 现状和前景
DOI：
10.1364/josab.5.002237
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发表时间：
1988
期刊：
影响因子：
--
通讯作者：
J. Seely
中科院分区：
文献类型：
--
作者：
U. Feldman;G. Doschek;J. Seely
本文综述了太阳光谱学在远紫外X射线波段的研究现状和前景。我们将太阳光谱划分为多个波长区域，这些区域由光谱仪器的特征决定。讨论了在每个区域获得的可用光谱的质量，集中在光谱分辨率，波长覆盖范围和准确性，以及线强度和线轮廓信息。我们的讨论主要限于包含谱线列表的论文，这样可以获得给定光谱区域的全局视图。血浆诊断和线路识别没有讨论，因为这些主题以前已经审查了很多次。我们讨论了绝对波长和线轮廓信息的需要，并简要地提到计划为这些情况下，信息是可用的未来的光谱调查。我们通过给出我们对最佳可用谱线列表的意见进行总结。
We review the status and prospects of solar spectroscopy in the far-UV–x-ray wavelength regions between approximately 1.7 and 2000 A. We divide the solar spectrum into a number of wavelength regions, determined by characteristics of spectroscopic instrumentation. The quality of the available spectra obtained in each region is discussed, concentrating on spectral resolution, wavelength coverage and accuracy, and line intensity and line-profile information. We limit the discussion primarily to papers that contain lists of spectral lines such that a global view of a given spectral region can be obtained. Plasma diagnostics and line identifications are not discussed because these topics have been reviewed many times previously. We discuss the need for absolute wavelength and line-profile information and briefly mention plans for future spectroscopic investigations for those cases for which information is available. We summarize by giving our opinion of the best available spectral line lists.