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  1. 極地研刊行誌
  2. 英文誌
  3. 極域宙空圏
  4. Advances in polar upper atmosphere research (ISSN 1345-1065)
  5. No.19 (Aug. 2005)

Inner magnetospheric plasma interactions and coupling with the ionosphere

https://doi.org/10.15094/00006407
https://doi.org/10.15094/00006407
0f62338e-7d06-4630-b8f8-29024531c4f9
名前 / ファイル ライセンス アクション
KJ00003387706.pdf KJ00003387706 (3.3 MB)
license.icon
Item type 紀要論文(ELS) / Departmental Bulletin Paper(1)
公開日 2005-08-01
タイトル
言語
言語 eng
キーワード
言語 en
主題Scheme Other
主題 inner magnetosphere
キーワード
言語 en
主題Scheme Other
主題 hot-cold interactions
キーワード
言語 en
主題Scheme Other
主題 magnetosphere-ionosphere coupling
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 10.15094/00006407
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) Fok, Mei-Ching

× Fok, Mei-Ching

WEKO 10229

en Fok, Mei-Ching

Search repository
Ebihara, Yusuke

× Ebihara, Yusuke

WEKO 20178

en Ebihara, Yusuke

Search repository
Moore, Thomas E.

× Moore, Thomas E.

WEKO 35543

en Moore, Thomas E.

Search repository
著者所属(英)
en
NASA Goddard Space Flight Center
著者所属(英)
en
National Institute of Polar Research
著者所属(英)
en
NASA Goddard Space Flight Center
抄録(英)
内容記述タイプ Other
内容記述 The inner magnetosphere occupies a vast volume in space containing a relatively low-density mixture of hot and cold plasmas: the ring current, plasmasphere and radiation belt. Energy is transferred from the ring current to the cold plasmas through Coulomb collisions and wave-particle interactions, producing temperature enhancements in the plasmasphere. The plasma waves generated in the plasmasphere cause pitch-angle and energy diffusion of the energetic particles. The magnetic disturbances generated from the ring current alter the drift paths of radiation belt particles, causing radiation belt flux dropout during magnetic storm main phases. The ionosphere is filled with dense and cold plasmas in a 1000-km-thick shell above the Earth's surface at ~100km altitude. Despite the distinct differences in size, location and physical properties, the ionosphere and the inner magnetosphere are tightly connected to each other. The ionosphere is an important source of magnetospheric ions. Energy transported down from the inner magnetosphere to the ionosphere produces observable temperature enhancements and optical emissions in the ionosphere. The electric coupling between the ionosphere and magnetosphere explains features such as shielding field, non-linear response of the ring current to the plasma-sheet source, and the post-midnight enhancement of the storm-time ring current flux. Even though many signatures are well described from the perspective of magnetosphere-ionosphere coupling, there are still unanswered questions, for example, the precise roles of wave-particle interactions in ring current loss and plasmaspheric heating, the cause of rapid storm initial recovery, the source of O^+ enhancement at substorm expansion, and the causes of outer radiation belt enhancement during storm recovery. The unresolved questions can be answered through careful cross analysis of the observational data from the ongoing and future imaging and multi-point missions with simulation results of large-scale modeling.
雑誌書誌ID
収録物識別子タイプ NCID
収録物識別子 AA11397422
書誌情報 Advances in polar upper atmosphere research

巻 19, p. 106-134, 発行日 2005-08
出版者
出版者 National Institute of Polar Research
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