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On Ion-cyclotron-resonance Heating of the Corona and Solar Wind : Volume 10, Issue 1/2 (30/11/-0001)

By Marsch, E.

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Book Id: WPLBN0004019526
Format Type: PDF Article :
File Size: Pages 12
Reproduction Date: 2015

Title: On Ion-cyclotron-resonance Heating of the Corona and Solar Wind : Volume 10, Issue 1/2 (30/11/-0001)  
Author: Marsch, E.
Volume: Vol. 10, Issue 1/2
Language: English
Subject: Science, Nonlinear, Processes
Collections: Periodicals: Journal and Magazine Collection, Copernicus GmbH
Publication Date:
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications


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Tu, C., Marsch, E., & Vocks, C. (-0001). On Ion-cyclotron-resonance Heating of the Corona and Solar Wind : Volume 10, Issue 1/2 (30/11/-0001). Retrieved from

Description: Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany. This paper concisely summarizes and critically reviews recent work by the authors on models of the heating of the solar corona by resonance of ions with high-frequency waves (up to the proton cyclotron frequency). The quasi-linear theory of pitch angle diffusion is presented in connection with relevant solar wind proton observations. Hybrid fluid-kinetic model equations, which include wave-particle interactions and collisions, are derived. Numerical solutions are discussed, representative of the inner corona and near-Sun solar wind. A semi-kinetic model for reduced velocity distributions is presented, yielding kinetic results for heavy ions in the solar corona. It is concluded that a self-consistent treatment of particle distributions and wave spectra is required, in order to adequately describe coronal physics and to obtain agreement with observations.

On ion-cyclotron-resonance heating of the corona and solar wind


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