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INFRARED SPECTROSCOPIC MEASUREMENT AT SYOWA STATION
https://doi.org/10.15094/00003718
https://doi.org/10.15094/000037180a811feb-4774-47ca-ac33-da08d14caeac
名前 / ファイル | ライセンス | アクション |
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KJ00002409947 (63.6 kB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1992-02-01 | |||||
タイトル | ||||||
タイトル | INFRARED SPECTROSCOPIC MEASUREMENT AT SYOWA STATION | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00003718 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
記事種別(英) | ||||||
en | ||||||
ABSTRACT | ||||||
論文名よみ | ||||||
その他のタイトル | INFRARED SPECTROSCOPIC MEASUREMENT AT SYOWA STATION | |||||
著者名よみ |
ムラタ, イサオ
× ムラタ, イサオ× キタ, カズユキ× イワガミ, ナオモト× オガワ, トシヒロ |
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著者名(英) |
MURATA, Isao
× MURATA, Isao× KITA, Kazuyuki× IWAGAMI, Naomoto× OGAWA, Toshihiro |
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著者所属(英) | ||||||
en | ||||||
Geophysics Research Laboratory, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Geophysics Research Laboratory, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Geophysics Research Laboratory, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Geophysics Research Laboratory, University of Tokyo | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Solar infrared spectroscopic measurements are planned for the 32th Japanese Antarctic Research Expedition 1990-1992 at Syowa Station. The observations will be made by using a 10cm telescope and a 1.5m double pass monochromator. The instrument resolution is 0.09(cm)^<-1> at 3000(cm)^<-1>. Although observations of trace gases in Antarctica have increased in recent years, many of them have been carried out in springtime to study the ozone hole. These observations will be carried out through out the year, and seasonal variation will be deduced. The vertical column abundance of atmospheric HCl, HF, N_2O and OCS will be deduced. HCl is important as a reservoir of ClO_x. In Antarctica HCl forms Cl_2 on the surface of the polar stratospheric clouds as a preliminary step in the development of the ozone hole. There are few measurements after September although the change before that is intensively interesting. HF and N_2O are poor reactive species, so these are good tracers of atmospheric transportation. OCS, one of the sources of sulfuric acid, has not been measured in Antarctica so far. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA10756213 | |||||
書誌情報 |
Proceedings of the NIPR Symposium on Polar Meteorology and Glaciology 巻 5, p. 180, 発行日 1992-02 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |