Compressibility Effect on the Rayleigh–Taylor Instability with Sheared Magnetic Fields

Ruderman, M.S. (2017) Compressibility Effect on the Rayleigh–Taylor Instability with Sheared Magnetic Fields. Solar Physics, 292. 47. ISSN 0038-0938

Abstract

Metadata

Authors/Creators:
  • Ruderman, M.S.
Copyright, Publisher and Additional Information: © 2017 Springer. This is an author produced version of a paper subsequently published in Solar Physics. Uploaded in accordance with the publisher's self-archiving policy. The final publication is available at Springer via http://dx.doi.org/10.1007/s11207-017-1073-8.
Keywords: Sun, corona; Magnetic fields; Magnetohydrodynamics; Stability
Dates:
  • Published: April 2017
  • Published (online): 22 March 2017
  • Accepted: 27 February 2017
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: 20 Apr 2017 08:44
Last Modified: 22 Mar 2018 01:38
Published Version: https://doi.org/10.1007/s11207-017-1073-8
Status: Published
Publisher: Springer Verlag
Refereed: Yes
Identification Number: https://doi.org/10.1007/s11207-017-1073-8

Share / Export

Statistics