| タイトル | Beam-return current systems in nonthermal solar flare models |
| 著者（英） | Larosa, T. N.; Emslie, A. Gordon |
| 著者所属（英） | Alabama Univ. |
| 発行日 | 1989-01-01 |
| 言語 | eng |
| 内容記述 | It is shown here that the generation of return current in large-scale astrophysical plasmas such as solar flares is quite different from the laboratory environment. Whereas in the laboratory the return current is established inductively and subsequently decays on a resistive timescale, the return current in a solar flare is established electrostatically and therefore does not decay. An explanation of the difference is given in terms of the characteristics of the laboratory circuit. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 89A51822 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/361616 |
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