DIRECT NUMERICAL SIMULATIONS OF REFLECTION-DRIVEN, REDUCED MAGNETOHYDRODYNAMIC TURBULENCE FROM THE SUN TO THE ALFVÉN CRITICAL POINT
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/776/i=2/a=124/pdf
Reference58 articles.
1. Large-amplitude Alfvén waves in the interplanetary medium, 2
2. Basic properties of magnetohydrodynamic turbulence in the inertial range
3. Polarization Intermittency and Its Influence on MHD Turbulence
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