Abstract
A model is presented using the electron cyclotron maser instability driven by a loss-cone distribution (taking account of the relativistic effects for electron cyclotron frequency and electron velocity as well as Landau damping and cyclotron damping) to excite the UFFS (Ultra-Fast Fine Structures) of microwave bursts and adopting a nonlinear density wave as a trigger mechanism to explain the millisecond time structure of the UFFS.
Proceedings of the Workshop on Radio Continua during Solar Flares, held at Duino (Trieste), Italy, 27–31 May, 1985.
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© 1986 D. Reidel Publishing Company
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Zhao, RY., Shi, JK. (1986). A Model of Ultra-Fast Fine Structures of Microwave Bursts. In: Benz, A.O. (eds) Radio Continua During Solar Flares. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4710-8_15
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DOI: https://doi.org/10.1007/978-94-009-4710-8_15
Publisher Name: Springer, Dordrecht
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