Energy loss of solar p modes due to the excitation of magnetic sausage tube waves: importance of coupling the upper atmosphere

Gascoyne, A., Jain, R. orcid.org/0000-0002-0080-5445 and Hindman, B.W. (2014) Energy loss of solar p modes due to the excitation of magnetic sausage tube waves: importance of coupling the upper atmosphere. Astrophysical Journal, 789 (2). 109. ISSN 0004-637X

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2014. The American Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: magnetohydrodynamics (MHD); Sun: chromosphere; Sun: helioseismology; Sun: magnetic fields; Sun: oscillations; waves
Dates:
  • Published: 19 June 2014
  • Accepted: 22 May 2014
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: 22 Apr 2016 11:11
Last Modified: 22 Apr 2016 11:26
Published Version: https://dx.doi.org/10.1088/0004-637X/789/2/109
Status: Published
Publisher: American Astronomical Society
Refereed: Yes
Identification Number: https://doi.org/10.1088/0004-637X/789/2/109
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