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2013IAUS..294..325B
Astrophysical MHD turbulence: confluence of observations, simulations, and theory
Burkhart, Blakesley ( Astronomy Department, University of Wisconsin, Madison, 475 N. Charter St., WI 53711, USA ); Lazarian, Alex ( Astronomy Department, University of Wisconsin, Madison, 475 N. Charter St., WI 53711, USA ) show affiliations
Solar and Astrophysical Dynamos and Magnetic Activity, Proceedings of the International Astronomical Union, IAU Symposium, Volume 294, pp. 325-336
Published in Jul 2013
Magnetohydrodynamic (MHD) turbulence is a critical component of the current paradigms of star formation, dynamo theory, particle transport, magnetic reconnection and evolution of the ISM. In order to gain understanding of how MHD turbulence regulates processes in the Galaxy, a confluence of numerics, observations and theory must be imployed. In these proceedings we review recent progress that has been made on the connections between theoretical, numerical, and observational understanding of MHD turbulence as it applies to both the neutral and ionized interstellar medium.
Keywords:
Free Keywords: ISM: general; MHD (magnetohydrodynamics); Turbulence; ism general; mhd; turbulence
(c) 2013: Copyright © International Astronomical Union 2013
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