Parallel and perpendicular cascades in solar wind turbulence

MHD-scale fluctuations in the velocity, magnetic, and density fields of the solar wind are routinely observed. The evolution of these fluctuations, as they are transported radially outwards by the solar wind, is believed to involve both wave and turbulence processes. The presence of an average magn...

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Bibliographic Details
Main Authors: S. Oughton, W. H. Matthaeus
Format: Article
Language:English
Published: Copernicus Publications 2005-01-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/12/299/2005/npg-12-299-2005.pdf