The conditions required for the stability of a steady-state electron beam propagating in the solar corona are determined using the quasi-linear theory. The growth rate for electron plasma waves in a magnetized plasma is evaluated, with the electron distribution function being given by an analytic so
Electron beams and associated rapid fluctuations in solar flares
โ Scribed by C. S. Li; Q. J. Fu; H. W. Li
- Publisher
- Springer
- Year
- 1991
- Tongue
- English
- Weight
- 753 KB
- Volume
- 131
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The generation of energetic electrons is always associated with the solar flares which occur within the sunspot groups that are highly active in emitting type I noise storms. The number of the solar flares which are associated with the distinct electron events observed at the earth tends to increase
We show that protons can be accelerated to several GeV in ~I0 s by Alfven turbulence whose energy density is greater than a few erg/cmS. We also show that electrons can be accelerated to tens of MeV on similar time scales by whistler and Alfven turbulence.