The Digital Database of Long-Term Solar Chromospheric Variation
スポンサーリンク
概要
- 論文の詳細を見る
From 1926 to 1969, a long term solar full disk observation was done by Kyoto University. Daily, Ca II K (393.4 nm) spectroheliographic images and white light images were recorded on photographic plates. In this report, we will give the current status of our project to digitize all these images and to construct a database of these images for public use through the IUGONET system. In addition, we will discuss our perspective on the scientific analysis of the database by taking the solar CaII K brightness as a proxy measure of the solar UV irradiance on the terrestrial upper atmosphere.
著者
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Maehara H
Kwasan And Hida Observatories Kyoto University
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Tomita Y
Department Of Basic Medical Research And Education Ehime University Graduate School Of Medicine
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Hayashi H
Research Center For Disaster Reduction Systems Dpri Kyoto University
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Kitai R
Kwasan And Hida Observatories Kyoto University
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Ueno S
Kwasan And Hida Observatories Kyoto University
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Hada Y
Kwasan and Hida Observatories, Graduate School of Science, Kyoto University, Kyoto, Japan
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Shirakawa S
Kwasan and Hida Observatories, Graduate School of Science, Kyoto University, Kyoto, Japan
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Katoda M
Kwasan and Hida Observatories, Graduate School of Science, Kyoto University, Kyoto, Japan
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Asai A
Unit for Synergetic Studies of Space, Kyoto University, Kyoto, Japan
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Isobe H
Unit for Synergetic Studies of Space, Kyoto University, Kyoto, Japan
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Goto H
The Kyoto University Museum, Kyoto University, Kyoto, Japan
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Yamashita S
The Kyoto University Museum, Kyoto University, Kyoto, Japan
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Kitai R
Kwasan and Hida Observatories, Graduate School of Science, Kyoto University, Kyoto, Japan
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- The Digital Database of Long-Term Solar Chromospheric Variation