The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes

Observations show that there are twisted magnetic flux tubes and plasma flow throughout the solar atmosphere. The main purpose of this work is to obtain the damping rate of sausage modes in the presence of magnetic twist and plasma flow. We obtain the dispersion relation for sausage modes in slow co...

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Main Authors: Mohammad Sadeghi, Karam Bahari, Kayoomars Karami
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acb536
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author Mohammad Sadeghi
Karam Bahari
Kayoomars Karami
author_facet Mohammad Sadeghi
Karam Bahari
Kayoomars Karami
author_sort Mohammad Sadeghi
collection DOAJ
description Observations show that there are twisted magnetic flux tubes and plasma flow throughout the solar atmosphere. The main purpose of this work is to obtain the damping rate of sausage modes in the presence of magnetic twist and plasma flow. We obtain the dispersion relation for sausage modes in slow continuity in an inhomogeneous layer under the conditions of magnetic pores, then we solve it numerically. For the selected density profile, the magnetic field, and the plasma flow as a function of radius across the inhomogeneous layer, we show that the effect of the twisted magnetic field on the resonance absorption at low speed of the plasma flow is greater than one at high speed.
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spelling doaj.art-aa251ae29b83464cb2b14e0133aa88122023-09-03T09:29:32ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-01944219410.3847/1538-4357/acb536The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux TubesMohammad Sadeghi0https://orcid.org/0000-0002-6409-7679Karam Bahari1https://orcid.org/0000-0002-4838-5646Kayoomars Karami2https://orcid.org/0000-0003-0008-0090Department of Physics, University of Kurdistan , Pasdaran Street, P.O. Box 66177-15175, Sanandaj, Iran; Centre for Mathematical Plasma Astrophysics (CmPA), KU Leuven, Celestijnenlaan 200B bus 2400, B-3001 Leuven, BelgiumPhysics Department, Faculty of Science, Razi University , Kermanshah, IranDepartment of Physics, University of Kurdistan , Pasdaran Street, P.O. Box 66177-15175, Sanandaj, IranObservations show that there are twisted magnetic flux tubes and plasma flow throughout the solar atmosphere. The main purpose of this work is to obtain the damping rate of sausage modes in the presence of magnetic twist and plasma flow. We obtain the dispersion relation for sausage modes in slow continuity in an inhomogeneous layer under the conditions of magnetic pores, then we solve it numerically. For the selected density profile, the magnetic field, and the plasma flow as a function of radius across the inhomogeneous layer, we show that the effect of the twisted magnetic field on the resonance absorption at low speed of the plasma flow is greater than one at high speed.https://doi.org/10.3847/1538-4357/acb536Solar physicsSolar photosphereSolar atmosphere
spellingShingle Mohammad Sadeghi
Karam Bahari
Kayoomars Karami
The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes
The Astrophysical Journal
Solar physics
Solar photosphere
Solar atmosphere
title The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes
title_full The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes
title_fullStr The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes
title_full_unstemmed The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes
title_short The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes
title_sort effect of flow and magnetic twist on resonant absorption of slow mhd waves in magnetic flux tubes
topic Solar physics
Solar photosphere
Solar atmosphere
url https://doi.org/10.3847/1538-4357/acb536
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