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Reflection of Alfvén Waves and Heating in Solar Coronal Holes
1991Using a simple model coronal hole, we estimate the short-period period limit for the reflection of Alfven waves in solar coronal holes. Waves with periods longer than this limit are strongly reflected and blocked from escaping into the solar wind; waves with periods appreciably shorter than this limit suffer little reflection and freely escape into the
Ronald L. Moore +3 more
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Solar global coronal wave front velocity estimation
PHYSICS OF SPACE : Proceedings of the 53-st All-Russian with international participation student scientific conferenceGlobal coronal waves are one of the manifestations of solar activity. They are generated as a result of impulsive energy releases such as solar flares, coronal mass ejections, and jets. The nature of global waves is not completely clear. Estimations of the wave parameters are needed.
D. D. Kuziy, E. G. Kupriyanova
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Slow-Mode Magnetoacoustic Waves in Coronal Loops
Space Science Reviews, 2021Abhishek Srivastava +2 more
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Magnetohydrodynamic waves and coronal seismology: an overview of recent results
Philosophical Transactions Series A, Mathematical, Physical, and Engineering Sciences, 2012V M Nakariakov, Ineke de Moortel
exaly
The Temporal Evolution of Linear Fast and Alfvén MHD Waves in Solar Coronal Arcades
Thirty Years of Astronomical Discovery With UKIRT, 2010José Luis Ballester +2 more
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