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Coronal Heating and the Solar Wind Acceleration

Published online by Cambridge University Press:  13 May 2016

T. Hirayama
T. Hirayama*
Affiliation:
Meisei Univ., Ome-shi, Tokyo 198-8655, Japan

Abstract

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We propose a coronal heating theory based on the magnetic twisting, which inevitably produces charge imbalance. The resulting electric field creates supra-thermal electron beams. Beams are then thermalized by classical collisions. The dissipation rate is enough to heat the corona and to accelerate the solar wind.

Type
Session V: Coronal Heating and Solar Wind Acceleration
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 495 - 497
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Hirayama, T. 2000, submitted to PASJ (referred as Paper I)”.Google Scholar
Withbroe, G. 1988, Apj, 325, 442.Google Scholar