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Nonlinear aspects of the solar coronal heating
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
CCLRC Rutherford-Appleton Labs, UK.
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
Linköping University, Department of Science and Technology, Visual Information Technology and Applications (VITA). Linköping University, The Institute of Technology.ORCID iD: 0000-0003-4055-0552
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2006 (English)In: Plasma Physics and Controlled Fusion, ISSN 0741-3335, E-ISSN 1361-6587, Vol. 48, no 12 B, B249-B255 p.Article in journal (Other academic) Published
Abstract [en]

The heating of the solar coronal plasma has remained one of the most important problems in solar physics. An explanation of the electron and ion heating rests on the identification of the energy source and appropriate physical mechanisms via which the energy can be channelled to the plasma particles. In this paper, we discuss two important nonlinear aspects of the electron and ion heating caused by finite amplitude obliquely propagating dispersive Alfvén (DA) waves and magnetic field-aligned circularly polarized electromagnetic ion-cyclotron Alfvén (EMICA) waves that may exist in the solar terrestrial environment. Specifically, DA waves may contribute to the solar coronal electron heating via Joule heating involving electron-wave interactions, and resonant ion EMICA wave interactions may contribute to differential ion heating in the solar corona.

Place, publisher, year, edition, pages
2006. Vol. 48, no 12 B, B249-B255 p.
Keyword [en]
plasma physics
National Category
Engineering and Technology
Identifiers
URN: urn:nbn:se:liu:diva-35703DOI: 10.1088/0741-3335/48/12B/S24Local ID: 28195OAI: oai:DiVA.org:liu-35703DiVA: diva2:256551
Available from: 2009-10-10 Created: 2009-10-10 Last updated: 2017-12-13

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Dieckmann, Mark EStenflo, Lennart

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