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Radio signatures of Langmuir-Alfvén turbulence in the solar atmosphere

Published online by Cambridge University Press:  14 March 2005

A. C.-L. Chian ,
M. Goossens ,
R. A. Miranda ,
E. L. Rempel ,
O. Sirenko  and
Y. Voitenko
A. C.-L. Chian
Affiliation:
National Institute for Space Research (INPE) and World Institute for Space Environment Research (WISER), P.O. Box 515, São José dos Campos-SP 12227-010, Brazil
M. Goossens
Affiliation:
Centre for Plasma Astrophysics, K.U. Leuven, Celestijnenlaan 200B, 3001, Heverlee, Belgium
R. A. Miranda
Affiliation:
National Institute for Space Research (INPE) and World Institute for Space Environment Research (WISER), P.O. Box 515, São José dos Campos-SP 12227-010, Brazil Centro de Estudos del Cuaternario, Universidad de Magallanes, Punta Arenas, Chile
E. L. Rempel
Affiliation:
National Institute for Space Research (INPE) and World Institute for Space Environment Research (WISER), P.O. Box 515, São José dos Campos-SP 12227-010, Brazil
O. Sirenko
Affiliation:
Centre for Plasma Astrophysics, K.U. Leuven, Celestijnenlaan 200B, 3001, Heverlee, Belgium
Y. Voitenko
Affiliation:
Centre for Plasma Astrophysics, K.U. Leuven, Celestijnenlaan 200B, 3001, Heverlee, Belgium Main Astronomical Observatory, National Academy of Sciences of Ukraine, 03680 Kyiv, Ukraine
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Abstract

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Radio emissions from the solar active regions can be generated by nonlinear coupling of Langmuir waves with Alfvén waves. Multi-wavelength observations can be used to provide evidence for Langmuir-Alfvén turbulence in the solar atmosphere.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 95 - 96
Copyright
© 2004 International Astronomical Union