Spectrum of MHD turbulence: theory, modeling, observations

Details Spectrum of MHD turbulence: theory, modeling, observations Spectrum of MHD turbulence: theory, modeling, observations

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..dppki1001b&link_type=abstract

American Physical Society, 48th Annual Meeting of the Division of Plasma Physics, October 30-November 3, 2006, abstract #KI1.001

Physics

Plasma Physics

Scientific paper

Magnetohydrodynamic (MHD) turbulence plays an essential role in a variety of astrophysical systems, from intergalactic and interstellar media, to stars and planets. Despite more than 40 years of analytical, numerical and observational research, the MHD turbulent cascade is not completely understood. I will present a brief introduction to the theory, and discuss the new analytic and numerical results on the spectrum and structure of strong incompressible MHD turbulence. 1mm In collaboration with Fausto Cattaneo and Joanne Mason (U. Chicago)

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