The polarization of hard solar X-radiation (> l0 keV) is calculated on the assumption that electrons get a non-isotropic velocity distribution in the initial phase of a flare. The bremsstrahlung generated by nonthermal electrons spiralling around magnetic field lines with discrete pitch angles is co
Hard X rays of relativistic electrons accelerated in solar flares
โ Scribed by I. V. Kudryavtsev, Yu. E. Charikov
- Book ID
- 119882007
- Publisher
- SP MAIK Nauka/Interperiodica
- Year
- 2012
- Tongue
- English
- Weight
- 354 KB
- Volume
- 52
- Category
- Article
- ISSN
- 0016-7932
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