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  1. 極地研刊行誌
  2. 英文誌
  3. 極域宙空圏
  4. Proceedings of the NIPR Symposium on Upper Atmosphere Physics (ISSN 0914-5613)
  5. No.11 (Jan. 1998)

Study on pixel intensity correction in projection transform of an all-sky auroral image

https://doi.org/10.15094/00004237
https://doi.org/10.15094/00004237
29c33bbd-fe6a-46dd-9ae6-c68264dc3a92
名前 / ファイル ライセンス アクション
KJ00000035940.pdf KJ00000035940 (686.3 kB)
license.icon
Item type 紀要論文(ELS) / Departmental Bulletin Paper(1)
公開日 1998-01-01
タイトル
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 10.15094/00004237
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)
著者名(英) Yang, Hoigen

× Yang, Hoigen

WEKO 7764

en Yang, Hoigen

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Liu, Ruiyuan

× Liu, Ruiyuan

WEKO 65381

en Liu, Ruiyuan

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Sato, Natsuo

× Sato, Natsuo

WEKO 408

en Sato, Natsuo

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著者所属(英)
en
Polar Research Institute of China/Polar Research Institute of China/National Institute of Polar Research
抄録(英)
内容記述タイプ Other
内容記述 The algorithm now in use for the projection of an all-sky auroral image onto the geomagnetic/geographic coordinates is summarized in a matrix form and inspected in this note. It is found that in existing projection transforms, pixel intensity has not been corrected at all, and an assumption has been adopted that aurora luminosity is confined in a thin layer of the ionosphere. Under this assumption, namely, that aurora appears in a thin layer of the ionosphere, an expression for pixel intensity correction in a projection of an all-sky auroral image onto the geomagnetic/geographic coordinates is explicitly derived, in which the visual enhancement due to the all-sky imaging geometry and the extinction due to the atmospheric absorption are concerned. The correction may be represented by a diagonal matrix, and should be added to the existing algorithm.
雑誌書誌ID
収録物識別子タイプ NCID
収録物識別子 AA10756224
書誌情報 Proceedings of the NIPR Symposium on Upper Atmosphere Physics

巻 11, p. 55-60, 発行日 1998-01
出版者
出版者 National Institute of Polar Research
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