Abstract
Observations over the past 20 yrs or so are reviewed, with emphasis on recent high spatial resolution observations. The results lend support to earlier ideas on the propagation of type III electron streams through coronal regions of weak magnetic field strength but have not as yet settled the question whether the electrons propagate along the axes of coronal streamers. Several important burst properties appear to be significantly affected by ray scattering on small-scale size density irregularities in the corona.
Publisher
Cambridge University Press (CUP)
Cited by
24 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Index;Classical Kinetic Theory of Weakly Turbulent Nonlinear Plasma Processes;2019-10-31
2. One-Dimensional Normalized Equations;Classical Kinetic Theory of Weakly Turbulent Nonlinear Plasma Processes;2019-10-31
3. On Renormalized Kinetic Turbulence Theory;Classical Kinetic Theory of Weakly Turbulent Nonlinear Plasma Processes;2019-10-31
4. On Higher-Order Perturbative Expansion;Classical Kinetic Theory of Weakly Turbulent Nonlinear Plasma Processes;2019-10-31
5. Weak Turbulence Theory for Reactive Instabilities;Classical Kinetic Theory of Weakly Turbulent Nonlinear Plasma Processes;2019-10-31