| タイトル | Current status of the dissipative thermal model for solar hard X-ray bursts |
| 著者（英） | Smith, D. F. |
| 著者所属（英） | Berkeley Research Associates, Inc. |
| 発行日 | 1985-01-01 |
| 言語 | eng |
| 内容記述 | The existing dissipative thermal models for hard X-ray bursts are briefly examined, and it is shown that the model with additional acceleration is the best candidate for explaining the whole hard X-ray burst. In both phases, but especially in the thermal phase, the plasma beta approaches unity, and two-dimensional modeling of the hydrodynamics is required. Following the accelerated electrons only, without taking into account the response of the bulk of the plasma, is inadequate. It is suggested that a useful approach might be a multifluid one using approximately 15 fluids with the possibility of transfer between fluids in one and two dimensions. It is concluded that, while the model is a promising one, many details remain to be worked out. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 85A48846 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/389590 |
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