๐”– Bobbio Scriptorium
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Comments on the mechanism of type III bursts

โœ Scribed by Paul J. Kellogg


Publisher
Springer
Year
1976
Tongue
English
Weight
93 KB
Volume
46
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


On the theory of the type III burst exci
โœ Robert A. Smith; Melvyn L. Goldstein; Konstantinos Papadopoulos ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 662 KB

In situ satellite observations of type III burst exciters at 1 AU show that the beam does not evolve into a plateau in velocity space, contrary to the prediction quasilinear theory. The observations can be explained by a theory that includes mode coupling effects due to excitation of the parametric

The starting frequencies of type III bur
โœ J. McKim Malville ๐Ÿ“‚ Article ๐Ÿ“… 1967 ๐Ÿ› Springer ๐ŸŒ English โš– 393 KB

During the period 1960 to 1966 the monthly averages of the starting frequencies of type II[ bursts declined with the level of solar activity and reached a minimum near the minimum of the solar cycle in 1964. The electron densities corresponding to the observed starting frequencies are close to those

Time profile of type III bursts
โœ T. Takakura; Y. Naito; K. Ohki ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 423 KB
On the propagation of the electron strea
โœ D. B. Melrose ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 638 KB

The suggestion is explored that the two-stream instability has little effect on the propagation of the electron streams which generate type III bursts because the time required (tO for development of the instability is comparable with or greater than the time available (At) for growth of the waves.