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
The interpretation of hard X-ray polarization measurements in solar flares
✍ Scribed by John Leach; A. Gordon Emslie; Vahé Petrosian
- Publisher
- Springer
- Year
- 1985
- Tongue
- English
- Weight
- 396 KB
- Volume
- 96
- Category
- Article
- ISSN
- 0038-0938
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