Nonthermal electrons responsible for solar radio and X-ray emissions
โ Scribed by Guang-Li Huang; Zhi-Hai Qin
- Publisher
- Elsevier Science
- Year
- 1998
- Tongue
- English
- Weight
- 744 KB
- Volume
- 3
- Category
- Article
- ISSN
- 1384-1076
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Observations of impulsive solar flare X-rays > 10 keV made with the OGO-5 satellite are compared with ground based measurements of type III solar radio bursts in 10-580 MHz range. It is shown that the times of maxima of these two emissions, when detectable, agree within ~ 18 s. This maximum time dif
Properties of electron acceleration in flares, especially the density structure in the acceleration region, are deduced from a correlation study between decimetric type III, spike, and hard X-ray (HXR) bursts. The high association rate found (71%) strongly suggests that spikes also originate from en
X-ray emission from seventeen X-ray flares was analyzed to obtain electron temperatures and emission measures associated with the source region in the solar corona. The source region was assumed to be isothermal with a Maxwellian electron velocity distribution. Flares which were characterized by a