## Abstract Different regimes of an whistler instability yield divers elements of fine structures: millisecond pulsations or different stripes in emission and absorption, moreover zebraβstripes can convers into fiber bursts and inversely.
Whistlers in the solar corona and their relevance to fine structures of type IV radio emission
β Scribed by G. P. Chernov
- Publisher
- Springer
- Year
- 1990
- Tongue
- English
- Weight
- 602 KB
- Volume
- 130
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
The longitudinal waves (Bernstein modes and plasma waves near the hybrid frequency) in a mixture of equilibrium coronal plasma and a small group of energetic electrons are investigated. The energetic electrons have a nonequilibrium momentum distribution inherent in trapped particles. The frequency d
The results of investigation of the cyclotron wave instability in the corona for Bernstein modes and plasma waves in a hybrid band have been used to interpret zebra-pattern phenomena. Two models of the generation region of parallel drifting bands are considered: the model of the point source localiz