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Neutralization and stabilization of particle streams in the corona and type III radio bursts

✍ Scribed by Dean F. Smith


Publisher
Springer
Year
1972
Tongue
English
Weight
690 KB
Volume
23
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES


Comments on β€˜neutralization and stabiliz
✍ D. B. Melrose πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 269 KB

Electron streams which excite type III bursts experience a negligible energy loss in accelerating a return current. Furthermore the plasma oscillations generated as the return current turns on and off are too weak to be of significance as a source of the observed radiation.

A comparison of type III solar radio bur
✍ Larry G. Evans; Joseph Fainberg; R. G. Stone πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 330 KB

The required electron density to excite a type III solar burst can be predicted from different theories, using the low frequency radio observations of the RAE-1 satellite. Electron flux measurements by satellite in the vicinity of 1 AU then give an independent means of comparing these predicted exci

A type II solar radio burst observed in
✍ I. D. Palmer πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 375 KB

A type II solar radio burst, which was observed by the satellite IMP-6 and reported by Malitson et al. (1973a), is correlated with a type II burst recorded by ground-based instruments at Culgoora. Since no other important coronal activity (as measured by meter-wave observations) occurred in the 9 hr