| タイトル | Hard x ray/microwave spectroscopy of solar flares |
| 本文（外部サイト） | http://hdl.handle.net/2060/19940009485 |
| 著者（英） | Gary, Dale E. |
| 著者所属（英） | California Inst. of Tech. |
| 発行日 | 1992-05-01 |
| 言語 | eng |
| 内容記述 | The joint study of hard x ray and microwave observations of solar flares is extremely important because the two complementary ways of viewing the accelerated electrons yield information that cannot be obtained using hard x rays or microwaves alone. The microwaves can provide spatial information lacking in the hard x rays, and the x ray data can give information on the energy distribution of electrons that remove ambiguities in the radio data. A prerequisite for combining the two data-sets, however, is to first understand which range of microwave frequencies correlate best with the hard x rays. This SMM Guest Investigator grant enabled us to combine multi-frequency OVRO data with calibrated hard x ray data to shed light on the relationship between the two emissions. In particular, the questions of which microwave frequencies correspond to which hard x ray energies, and what is the corresponding energy of the electrons that produce both types of emission are investigated. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 94N13958
NASA-CR-194399
NAS 1.26:194399 |
| 権利 | No Copyright |
|
