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The magnetospheric electron density nM and thermal energy EM above auroral arcs have been estimated by fitting the accelerated Maxwellian distribution function to the electron energy spectra observed by two Antarctic rockets and the Defense Meteorological Satellite Program (DMSP)  satellites. The fitting based on the adiabatic theory of auroral particle motions between the magnetosphere and the ionosphere. The theory also shows that the field-aligned current j∥is linearly proportional to the fieldaligned potential difference V∥. The proportional constant corresponds to the adiabatic conductivity K along  a magnetic field line. The main finding of this study is that the estimated magnetospheric electron density nM and the adiabatic conductivity K decrease with increasing V∥(obtained from the statistical study using the DMSP particle data). 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  1. B100 理学部/理学研究科
  2. B100d 学位論文
  3. 博士論文(理博・論理博)

A Study of Auroral Particles: Their Global Characteristics and Magnetosphere-Ionosphere Coupling Processes

http://hdl.handle.net/2237/6598
http://hdl.handle.net/2237/6598
91f87e7e-aaad-4beb-96fc-c43fe0e85886
名前 / ファイル ライセンス アクション
ot4638_abstr.pdf ot4638_abstr.pdf (307.9 kB)
ot4638.pdf ot4638.pdf (12.8 MB)
Item type 学位論文 / Thesis or Dissertation(1)
公開日 2006-06-22
タイトル
タイトル A Study of Auroral Particles: Their Global Characteristics and Magnetosphere-Ionosphere Coupling Processes
言語 en
その他のタイトル
その他のタイトル オーロラ粒子の研究: そのグローバルな特徴と磁気圏-電離圏結合過程
言語 ja
著者 Shiokawa, Kazuo

× Shiokawa, Kazuo

WEKO 12529

en Shiokawa, Kazuo

Search repository
塩川, 和夫

× 塩川, 和夫

WEKO 12530

ja 塩川, 和夫

Search repository
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
抄録
内容記述 Magnetosphere-ionosphere coupling processes associated with auroras have been studied on both the local and the global scale and on various magnetic activities and substorm phases. The magnetospheric electron density nM and thermal energy EM above auroral arcs have been estimated by fitting the accelerated Maxwellian distribution function to the electron energy spectra observed by two Antarctic rockets and the Defense Meteorological Satellite Program (DMSP) satellites. The fitting based on the adiabatic theory of auroral particle motions between the magnetosphere and the ionosphere. The theory also shows that the field-aligned current j∥is linearly proportional to the fieldaligned potential difference V∥. The proportional constant corresponds to the adiabatic conductivity K along a magnetic field line. The main finding of this study is that the estimated magnetospheric electron density nM and the adiabatic conductivity K decrease with increasing V∥(obtained from the statistical study using the DMSP particle data). This fact suggests that field-aligned potential differences are formed to maintain field-aligned currents in the magnetosphere-ionosphere coupling process. Several features of electron heating during field-aligned acceleration have been studied in detail using the rocket data and on a global scale using the DMSP data. The different structures of magnetospheric electron densities above quiet and active auroral arcs are found from the rocket observations. The DMSP observations suggest that the estimated electron density and thermal energy in the magnetosphere are very useful parameters for identifying the magnetospheric source region of precipitating particles. Another interesting result of the present study is that we have shown the global changes in the precipitating particle features associated with substorm phases. The Central Plasma Sheet (CPS) type electron precipitation region expands toward a higher latitude around midnight and toward a lower latitude around the postmidnight sector after the substorm occurs. Latitudinal dispersion of electron and ion energy is found near the lowest latitude of the particle precipitation region. The dispersion features can be explained by particle motions injected from the magnetotail associated with the substorm. Partial overlap events between the traditional Boundary Plasma Sheet (BPS) and CPS are found for all the nightside local times of 1800-0900 MLT in the recovery phase and only around the morning and evening sectors before the substorm onset. These overlap events suggest mixing of the source plasma of BPS and CPS at these times. A drastic increase in the field-aligned potential difference is observed in the eveningside BPS region after the substorm onset, while the potential difference for the overlap events are found to be slightly larger on the morning side. It is suggested that the mechanism by which the field-aligned potential difference is formed to maintain the field-aligned current can produce these different dawn-dusk asymmetries of potential difference. The magnetospheric electron density for the eveningside BPS region is found not to change greatly before and after and the substorm onset, suggesting that supply and loss of magnetospheric electrons in the evening sector are balanced during the substorm.
言語 en
内容記述タイプ Abstract
内容記述
内容記述 名古屋大学博士学位論文 学位の種類:博士(理学) (論文) 学位授与年月日:平成6年7月11日
言語 ja
内容記述タイプ Other
言語
言語 eng
資源タイプ
資源 http://purl.org/coar/resource_type/c_db06
タイプ doctoral thesis
書誌情報
発行日 1994-07-11
学位名
言語 ja
学位名 博士(理学)
学位授与機関
学位授与機関識別子Scheme kakenhi
学位授与機関識別子 13901
言語 ja
学位授与機関名 名古屋大学
言語 en
学位授与機関名 Nagoya University
学位授与年度
学位授与年度 1994
学位授与年月日
学位授与年月日 1994-07-11
学位授与番号
学位授与番号 乙第4638号
フォーマット
application/pdf
フォーマット
application/pdf
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/6598
識別子タイプ HDL
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