| タイトル | Shock-associated kilometric radio emission and solar metric type II bursts |
| 著者（英） | Kahler, S. W.; Cliver, E. W.; Cane, H. V. |
| 著者所属（英） | Emmanuel Coll.|NASA Goddard Space Flight Center|Air Force Geophysics Lab. |
| 発行日 | 1989-01-01 |
| 言語 | eng |
| 内容記述 | New criteria are used here to select and study the properties of shock-associated (SA) kilometric bursts. Nearly half of all intense metric type II bursts were temporally associated with 1980 kHz emission which was not attributable to metric type III bursts. A quarter of all intense type II bursts are not associated with any significant 1980 kHz emission and another quarter are accompanied by 1980 kHz emission presumed due to type II bursts. The SA bursts are generally not well correlated with microwave flux-density profiles but compare more closely with the most intense and structured parts of the profiles of metric type II bursts. These results imply that the SA emission is due primarily to energetic electrons accelerated at the associated shock. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 89A51826
AD-A212484 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/361614 |
