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 from Slow Flares
โ Scribed by H. S. Hudson,D. E. McKenzie
- Book ID
- 126383984
- Publisher
- Terra Scientific Publishing Company, Tokyo
- Year
- 2001
- Tongue
- English
- Weight
- 262 KB
- Volume
- 53
- Category
- Article
- ISSN
- 1343-8832
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