Identification of slow magnetosonic wave trains and their evolution in 3-D compressible turbulence simulation

In solar wind, dissipation of slow-mode magnetosonic waves may play a significant role in heating the solar wind, and these modes contribute essentially to the solar wind compressible turbulence. Most previous identifications of slow waves utilized the characteristic negative correlation...

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Bibliographic Details

Published in:	Annales Geophysicae
Main Authors:	L. Zhang, L.-P. Yang, J.-S. He, C.-Y. Tu, L.-H. Wang, E. Marsch, X.-S. Feng
Format:	Article
Language:	English
Published:	Copernicus Publications 2015-01-01
Online Access:	https://www.ann-geophys.net/33/13/2015/angeo-33-13-2015.pdf