Solar Flares pp 300-349 | Cite as
Flare Models
Chapter
Abstract
First of all, let us summarize the basic properties of flares which we learned in Chapters II through V, and which an ideal flare theory should explain.
Keywords
Current Sheet Magnetic Field Line Radio Burst Neutral Line Acceleration Process
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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Copyright information
© D. Reidel Publishing Company, Dordrecht, Holland 1976