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南極オゾンホール回復時の輸送・混合過程
https://doi.org/10.15094/00009562
https://doi.org/10.15094/0000956248135602-ce21-4826-b374-2d9c261e5c58
名前 / ファイル | ライセンス | アクション |
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KJ00007134499 (8.1 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 2010-12-28 | |||||
タイトル | ||||||
タイトル | 南極オゾンホール回復時の輸送・混合過程 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Transport and mixing processes during the Antarctic ozone increase | |||||
言語 | ||||||
言語 | jpn | |||||
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 | 10.15094/00009562 | |||||
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) | |||||
論文名よみ | ||||||
その他のタイトル | ナンキョク オゾンホール カイフク ジ ノ ユソウ コンゴウ カテイ | |||||
著者名(日) |
冨川, 喜弘
× 冨川, 喜弘× 佐藤, 薫 |
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著者名(英) |
Tomikawa, Yoshihiro
× Tomikawa, Yoshihiro× Sato, Kaoru |
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著者所属(日) | ||||||
情報・システム研究機構国立極地研究所 | ||||||
著者所属(日) | ||||||
東京大学大学院理学系研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research, Research Organization of Information and Systems, Midori-cho 10-3, Tachikawa, Tokyo 190-8518. | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033. | ||||||
抄録(日) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第44次日本南極地域観測隊は,南極オゾンホールの形成過程に加え,その消滅過程の時間発展とメカニズムを明らかにすることを目的として,2003年6月~ 2004年1月にかけて南極昭和基地(69.0゜S,39.6゜E)でオゾンゾンデ集中観測を行った.上記オゾンゾンデデータと衛星観測データを用いた解析から,極渦崩壊前からブリューワー・ドブソン循環の下降流と中緯度との大気交換による極渦内のオゾン回復が始まっていることがわかった.また,波数1の準停滞性プラネタリー波の活動により,極渦内のオゾン回復の様相が経度によって大きく異なることがわかった.さらに,オゾンホール内に見られるオゾン増大層の解析から,極渦境界領域起源の空気塊が頻繁にオゾンホール内に流入していたことも明らかとなった. | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The 44th Japanese Antarctic Research Expedition (JARE-44) performed intensive ozonesonde observations at Syowa Station (69.0゜S, 39.6゜E) from June 2003 through January 2004 to clarify the time evolution and mechanism of the Antarctic ozone hole dissipation as well as its formation. From analysis of the ozonesonde and satellite observational data, it was found that ozone concentration inside the Antarctic ozone hole began to increase due to the Brewer-Dobson circulation and the lateral mixing between inside and outside the polar vortex even before its breakup. In addition, the ozone increase was dependent on longitude because of the zonal wavenumber 1 quasi-stationary planetary waves. It is also reported that the ozone enhanced layers frequently observed inside the Antarctic ozone hole mostly originated from the vortex boundary region. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00181831 | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00857289 | |||||
書誌情報 |
南極資料 en : Antarctic Record 巻 54, 号 特集号, p. 349-373, 発行日 2010-12-28 |
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国際十進分類法 | ||||||
主題Scheme | UDC | |||||
主題 | 551.5 |