Particle motions in coronal streamers and type III radio bursts
β 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.
π SIMILAR VOLUMES
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
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.
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