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Ion Cyclotron Instability and Electron Acceleration in Coronal Magnetic Flux Tubes

Published online by Cambridge University Press:  19 July 2016

Xu Min-jian ,
Li Ding-yi ,
Wang De-yu  and
Tsai Shih-tung
Xu Min-jian
Affiliation:
Association for Plasma Studied of China, Chinese Astronomical Society, Institute of Physics Academia Sinica, Beijing 100080, China
Li Ding-yi
Affiliation:
Association for Plasma Studied of China, Chinese Astronomical Society, Institute of Physics Academia Sinica, Beijing 100080, China
Wang De-yu
Affiliation:
Association for Plasma Studied of China, Chinese Astronomical Society, Institute of Physics Academia Sinica, Beijing 100080, China
Tsai Shih-tung
Affiliation:
Association for Plasma Studied of China, Chinese Astronomical Society, Institute of Physics Academia Sinica, Beijing 100080, China

Extract

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Part of the energy of low solar corona may be released and converted to plasma energy that may be the dominant source of solar flares. Recently, many physical mechanisms have been proposed to accelerate ions and electrons. In the magnetic mirror device of fusion research, ion cyclotron instability and the energetic ion losses have been discovered and the plasma becomes electron rich.

Type
VIII. Solar Flares
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 452 - 453
Copyright
Copyright © Kluwer 1990 

References

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