Title of article
On dissipative effects in solar prominences
Author/Authors
Ballai، I. نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2003
Pages
-16
From page
17
To page
0
Abstract
The present paper aims to discuss the possible dissipative mechanisms acting in a coronal prominence. These mechanism are discussed within the context of spatial damping of linear compressional waves. The obtained results show that the dominant mechanism is thermal radiation provided the supposition of optically thin prominence is valid. Damping due to thermal conduction is a viable attenuation mechanism provided the wavelength of the waves is short.
Keywords
Atmosphere , SUN , prominences , Magnetohydrodynamics , Evolution , numerical , magnetic fields
Journal title
Astronomy and Astrophysics
Serial Year
2003
Journal title
Astronomy and Astrophysics
Record number
78145
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