| タイトル | The three-dimensional structure of the solar corona |
| 著者（英） | Epple, A.; Inhester, B.; Zidowitz, S. |
| 著者所属（英） | Max-Planck-Inst. fuer Aeronomie |
| 発行日 | 1995-06-30 |
| 言語 | eng |
| 内容記述 | Due to the rotation of the sun the solar corona can be observed under different directions at different times. Using methods of computer tomography the three-dimensional structure of the emissivity of the solar corona can be reconstructed. We discuss the feasibility of this method for stationary and for non-stationary corona and also for incomplete and finite resolution data. As example we present reconstructions based on YOHKOH-images, and we compare the results with ground-based optical corona observations. Structures are interpreted in terms of the solar magnetic field topology. |
| NASA分類 | Solar Physics |
| レポートNO | 96N24774 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/304977 |
