Damping of Linear Nonadiabatic MHD Waves in a Flowing Prominence Medium
Dublin Core
Title
Damping of Linear Nonadiabatic MHD Waves in a Flowing Prominence Medium
Description
We study the effect of shear flow on the time damping of linear nonadiabatic magnetoacoustic waves in a solar prominence. We consider a homogeneous, isothermal, and unbounded medium permeated by a uniform magnetic field. The adiabaticity is removed by including the optically thin radiative losses, thermal conduction, and heating term in energy equation. We present a local theory of MHD waves to obtain a dispersion relation. The dispersion relation is solved numerically to study the time damping of these waves. It is found that flow influences the damping time and damping per period of both the slow and fast waves significantly. Damping time and damping per period of slow waves are very much higher than the damping time and damping per period of fast waves.
Creator
Nagendra Kumar
Anil Kumar
Himanshu Sikka
Pradeep Kumar
Publisher
Advances in Astronomy
Date
2014
Rights
Copyright © 2014 Nagendra Kumar et al.
Language
en
Type
Research Article
Identifier
https://doi.org/10.1155/2014/541376
Collection
Citation
Nagendra Kumar et al., “Damping of Linear Nonadiabatic MHD Waves in a Flowing Prominence Medium,” Open Access Journal Archives, accessed January 19, 2022, https://oajour.info/items/show/897.