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Energy Transfer across the Magnetospheric Boundary : A Computer Simulation of the Cross-field Heat Transfer in a Collisionless Plasma
https://jaxa.repo.nii.ac.jp/records/34574
https://jaxa.repo.nii.ac.jp/records/345746f9f39b2-edc8-490a-a719-c2f81b57073a
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
SA2404131.pdf (470.0 kB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||||||
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| 公開日 | 2015-03-26 | |||||||||
| タイトル | ||||||||||
| タイトル | Energy Transfer across the Magnetospheric Boundary : A Computer Simulation of the Cross-field Heat Transfer in a Collisionless Plasma | |||||||||
| 言語 | en | |||||||||
| 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 | |||||||||
| 著者 |
OBAYASHI, Tatsuzo
× OBAYASHI, Tatsuzo
× TSUDA, Takao
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| 著者所属（英） | ||||||||||
| en | ||||||||||
| Department of Electronics, Kyoto University | ||||||||||
| 出版者 | ||||||||||
| 出版者 | 東京大学宇宙航空研究所 | |||||||||
| 出版者（英） | ||||||||||
| 出版者 | Institute of Space and Aeronautical Science,University of Tokyo | |||||||||
| 書誌情報 |
en : ISAS report/Institute of Space and Aeronautical Science,University of Tokyo 巻 33, 号 11, p. 301-308, 発行日 1968-09 |
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| 抄録（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | A computer experiment has been made, simulating the condition of the earth's magnetospheric boundary where an appreciable flow of energy is entering to the magnetosphere from the high temperature domain of the solar wind. One dimensional sheet model being employed, the rate of heat energy flow is computed for the collisionless plasma in which the particles are transported across the static magnetic field. It is shown that the effective transfer rate of heat energy across the magnetic field can attain the value of 10^6 times as large as that estimated by the classical formulae of transport phenomena. An interpretation on the physical mechanism is suggested in terms of the wave-particle interactions in the collisionless regime. It is shown that magnetic turbulences generated at the magnetopause act to destroy the anisotropy of diffusion in such a manner the D_∥ and D_⊥ approach to an effective value D_*∿√<D_∥D_⊥>=υλ_⊥. | |||||||||
| ISSN | ||||||||||
| 収録物識別子タイプ | ISSN | |||||||||
| 収録物識別子 | 0372-1418 | |||||||||
| 書誌レコードID | ||||||||||
| 収録物識別子タイプ | NCID | |||||||||
| 収録物識別子 | AA00675986 | |||||||||
| 資料番号 | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | 資料番号: SA2404131000 | |||||||||
