The stability of electron beams in the f
โ
K. G. McClements
๐
Article
๐
1987
๐
Springer
๐
English
โ 432 KB
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