紫外線天文学
1. Ultraviolet astronomyUltraviolet astronomy is generally used to refer to observations of electromagnetic radiation at ultraviolet wavelengths between approximately 10 and 320 nanometres; shorter wavelengths—higher energy photons—are studied by X-ray astronomy and gamma ray astronomy. Light at these wavelengths is absorbed by the Earth's atmosphere, so observations at these wavelengths must be performed from the upper atmosphere or from space.
Read “Ultraviolet astronomy” on English Wikipedia
Read “紫外線天文学” on Japanese Wikipedia
Read “Ultraviolet astronomy” on DBpedia
Read “Ultraviolet astronomy” on English Wikipedia
Read “紫外線天文学” on Japanese Wikipedia
Read “Ultraviolet astronomy” on DBpedia
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