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Nonlinear Damping of Fast Waves and Plasma Heating in the Solar Corona

Published online by Cambridge University Press:  13 May 2016

Y. Voitenko
Affiliation:
Centre for Plasma Astrophysics, K. U. Leuven, Celestijnenlaan 200B, 3001 Heverlee, Belgium 2Main Astronomical Observatory, Golosiiv, 03680 Kyiv-127, Ukraine
M. Goossens
Affiliation:
Centre for Plasma Astrophysics, K. U. Leuven, Celestijnenlaan 200B, 3001 Heverlee, Belgium

Abstract

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A nonlinear mechanism for the damping of fast magnetoacoustic wave in the solar corona is studied. It is shown that the nonlinear coupling of finite-amplitude fast waves to small-scale Alfven waves can be much faster than damping mechanisms involving classic transport coefficients.

Type
Session V: Coronal Heating and Solar Wind Acceleration
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Aschwanden, M. J., Fletcher, L., Schrijver, C. J., & Alexander, D. 1999, ApJ 520, 880.Google Scholar
Berger, T. E., De Pontieu, B., Schrijver, C. J., & Title, A. M. 1999, ApJ 519, L97.Google Scholar
De Groof, A., Tirry, W. J., & Goossens, M. 1998, A&A 335, 329.Google Scholar
De Groof, A. & Goossens, M. 2000, A&A 356, 724.Google Scholar
Doyle, J.G., Banerjee, D., & Perez, M. E 1998, Solar Phys. 181, 91.Google Scholar
Hollweg, J. V. 1999, J. Geophys. Res. 76, 14811.Google Scholar
Koutchmy, S., Zugzda, Y. D., & Locans, V. 1983, A&A 120, 185.Google Scholar
Nakariakov, V. N., Ofman, L., DeLuca, E. E., Roberts, B., & Davila, J. M. 1999, Science 285, 862.Google Scholar
Tirry, W. J. & Berghmans, D. 1997, A&A 325, 329.Google Scholar
Voitenko, Yu. M. & Goossens, M. 2000a, A&A 357, 1073.Google Scholar
Voitenko, Yu. M. & Goossens, M. 2000b, A&A 357, 1086.Google Scholar