Hague, A. and Erdelyi, R. (2018) Buoyancy-driven magnetohydrodynamic waves in a partially ionized plasma. Astrophysical Journal, 866 (2). 114. ISSN 0004-637X
Abstract
A magnetohydrodynamic (MHD) fluid description is typically employed to study the magnetized plasma comprising the solaratmosphere.Thisapproachhas hadmanysuccessesinmodelingand explainingsolarphenomena.Mostoften, the plasma is assumed to be fully ionized. While this approach is justified in the higher atmosphere, i.e., the solar corona; the temperature in the lower solar atmosphere is such that a large proportion of the fluid may be electrically neutral. This begs the question: to what degree are the results derived from a fully ionized MHD description valid? In this article, we investigate the effect of partial ionization on buoyancy-driven MHD waves (the MHD analog of internal gravity waves) by applying a simplifiedtwo-fluid description. We show that previously derived results may be applied, when the fluid is weakly ionized, if the ion–neutral collision frequency is high. We derive dispersion relations for buoyancy-driven MHD waves, which include correction factors and damping rates due to ion–neutral collisions.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2018. The American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence (https://creativecommons.org/licenses/by/3.0/). Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. |
Keywords: | hydrodynamics; magnetohydrodynamics (MHD); Sun: atmosphere; Sun: oscillations; waves |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield) |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 07 Mar 2019 11:39 |
Last Modified: | 07 Mar 2019 11:39 |
Published Version: | https://doi.org/10.3847/1538-4357/aae25f |
Status: | Published |
Publisher: | American Astronomical Society; IOP Publishing |
Refereed: | Yes |
Identification Number: | 10.3847/1538-4357/aae25f |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:140803 |