Observations of the near and far ultraviolet background
Observations of the near and far ultraviolet background
复制标题
近紫外背景和远紫外背景的观测
DOI：
10.1007/s10509-008-9855-y
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发表时间：
2009
影响因子：
1.9
通讯作者：
Jayant Murthy
中科院分区：
文献类型：
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作者：
Jayant Murthy
漫射紫外辐射场覆盖整个天空，是星际介质中热成分（以CIV和OVI等线的形式）和冷成分（以星际尘埃或分子氢的形式）的示踪物。在过去的40年里，观测一直在不断地推动现有仪器的界限，但现在在更好地定义辐射和了解其成分方面取得了成果，无论是前景，如气辉或黄道光，还是宇宙。我提出了一个审查的远紫外和近紫外背景观测的现状。
The diffuse ultraviolet radiation field is seen over the entire sky and is a tracer of both the hot (in the form of lines such as CIV and OVI) and cold component (in the form of interstellar dust or molecular hydrogen) of the interstellar medium. Observations over the last 40 years have been continually pushing the boundaries of the available instrumentation but are now bearing fruit in a much better definition of the radiation and an understanding of its constituents, both foreground, such as airglow or zodiacal light, and cosmic. I present a review of the current state of observations of the far and near ultraviolet background.