The Role Of Torsional Alfvén Waves in Coronal Heating

In the context of coronal heating, among the zoo of magnetohydrodynamic (MHD) waves that exist in the solar atmosphere, Alfven waves receive special attention. Indeed, these waves constitute an attractive heating agent due to their ability to carry over the many different layers of the solar atmosph...

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Vydáno v:	The Astrophysical journal Ročník 712; číslo 1; s. 494 - 510
Hlavní autoři:	Antolin, P, Shibata, K
Médium:	Journal Article
Jazyk:	angličtina
Vydáno:	Bristol IOP Publishing 20.03.2010 IOP
Témata:	ABSORPTION ALFVEN WAVES Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ATMOSPHERES Earth, ocean, space ELECTROMAGNETIC RADIATION Exact sciences and technology FLUID MECHANICS HEATING HYDRODYNAMICS HYDROMAGNETIC WAVES MAGNETIC FIELDS MAGNETIC FLUX MAGNETOHYDRODYNAMICS MAIN SEQUENCE STARS MECHANICS MODE CONVERSION MONOCHROMATIC RADIATION PHOTOSPHERE PLASMA HEATING POLARIMETERS RADIATIONS SATELLITES SHOCK HEATING SOLAR ATMOSPHERE SOLAR CORONA SORPTION SPECTRA STARS STELLAR ATMOSPHERES STELLAR CORONAE SUN TELESCOPES Collapse Energetics Alfven waves Sun: flares waves Solar corona Magnetic flux Plasma Magnetohydrodynamics Mixing Critical value MHD waves Flux tubes Sun: corona Resonant absorption Sun Noise spectrum Shock heating Hinode satellite White noise Solar atmosphere Models Magnetic fields magnetohydrodynamics (MHD)
ISSN:	0004-637X, 1538-4357
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