Damping of visco-resistive Alfven waves in solar spicules

Interaction of Alfven waves with plasma inhomogeneity generates phase mixing which can cause the dissipation of Alfven waves. We investigated the dissipation of standing Alfven waves due to phase mixing at the presence of steady flow and sheared magnetic field in solar spicules. Moreover, the transi...

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Main Authors: Z Fazel, H Ebadi
Format: Article
Language:English
Published: Isfahan University of Technology 2014-12-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-665&slc_lang=en&sid=1
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author Z Fazel
H Ebadi
author_facet Z Fazel
H Ebadi
author_sort Z Fazel
collection DOAJ
description Interaction of Alfven waves with plasma inhomogeneity generates phase mixing which can cause the dissipation of Alfven waves. We investigated the dissipation of standing Alfven waves due to phase mixing at the presence of steady flow and sheared magnetic field in solar spicules. Moreover, the transition region between chromosphere and corona was considered. Our numerical simulation showed that the phase mixing and dissipation rate of Alfven waves are enhanced relative to viscosity and resistivity gradients. Comparison of the results of our models with and without these gradients illustrated a significant difference between them. In other words, with these assumptions, Alfven waves may transfer the photospheric energy to the corona during timescales corresponding to the observed lifetimes of spicules. It should be noted that the results of our numerical simulation were in good agreement with observational scaling law obtained by Kuridze et al. [1]
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spelling doaj.art-8049219ca360438c80667c2d8468e5aa2022-12-21T20:32:00ZengIsfahan University of TechnologyIranian Journal of Physics Research1682-69572014-12-011437378Damping of visco-resistive Alfven waves in solar spiculesZ Fazel0H Ebadi1 Astrophysics Section, Department of Physics, University of Tabriz, Tabriz, Iran Astrophysics Section, Department of Physics, University of Tabriz, Tabriz, Iran Interaction of Alfven waves with plasma inhomogeneity generates phase mixing which can cause the dissipation of Alfven waves. We investigated the dissipation of standing Alfven waves due to phase mixing at the presence of steady flow and sheared magnetic field in solar spicules. Moreover, the transition region between chromosphere and corona was considered. Our numerical simulation showed that the phase mixing and dissipation rate of Alfven waves are enhanced relative to viscosity and resistivity gradients. Comparison of the results of our models with and without these gradients illustrated a significant difference between them. In other words, with these assumptions, Alfven waves may transfer the photospheric energy to the corona during timescales corresponding to the observed lifetimes of spicules. It should be noted that the results of our numerical simulation were in good agreement with observational scaling law obtained by Kuridze et al. [1]http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-665&slc_lang=en&sid=1solar spicules Alfven waves damping transition region.
spellingShingle Z Fazel
H Ebadi
Damping of visco-resistive Alfven waves in solar spicules
Iranian Journal of Physics Research
solar spicules
Alfven waves
damping
transition region.
title Damping of visco-resistive Alfven waves in solar spicules
title_full Damping of visco-resistive Alfven waves in solar spicules
title_fullStr Damping of visco-resistive Alfven waves in solar spicules
title_full_unstemmed Damping of visco-resistive Alfven waves in solar spicules
title_short Damping of visco-resistive Alfven waves in solar spicules
title_sort damping of visco resistive alfven waves in solar spicules
topic solar spicules
Alfven waves
damping
transition region.
url http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-665&slc_lang=en&sid=1
work_keys_str_mv AT zfazel dampingofviscoresistivealfvenwavesinsolarspicules
AT hebadi dampingofviscoresistivealfvenwavesinsolarspicules