The structure of the hydrodynamic plasma flow near the heliopause stagnation point

Belov, N.A. and Ruderman, M.S. (2010) The structure of the hydrodynamic plasma flow near the heliopause stagnation point. Monthly Notices of the Royal Astronomical Society , 401 (1). pp. 607-612. ISSN 0035-8711

Abstract

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Authors/Creators:
  • Belov, N.A.
  • Ruderman, M.S.
Copyright, Publisher and Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2009 The Authors. Journal compilation © 2009 RAS Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: hydrodynamics; plasmas; solar wind; Solar system: general
Dates:
  • Published: 1 January 2010
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: 06 Nov 2017 15:46
Last Modified: 06 Nov 2017 15:46
Published Version: https://doi.org/10.1111/j.1365-2966.2009.15683.x
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1111/j.1365-2966.2009.15683.x
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