𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Particle motions in coronal streamers and type III radio bursts

✍ Scribed by Dean F. Smith; G. W. Pneuman


Publisher
Springer
Year
1972
Tongue
English
Weight
821 KB
Volume
25
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


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

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.

Type III solar radio bursts observed at
✍ C. Mercier; H. Rosenberg πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 732 KB

Seventy-six type 1II solar radio bursts or burst groups occurring over 41 days in the period November 1968 to July 1971 were studied with high time and spatial resolution at 169 MHz and high time and spectral resolution between 160 and 320 MHz. The average height of the sources at 169 MHz was found