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Turbulence evolution in MHD plasmas

Published online by Cambridge University Press:  21 February 2013

MARTINA WISNIEWSKI,
RALF KISSMANN and
FELIX SPANIER
MARTINA WISNIEWSKI
Affiliation:
Lehrstuhl für Astronomie, Universität Würzburg, Emil-Fischer Str. 31, D-97074 Würzburg, Germany (fspanier@astro.uni-wuerzburg.de)
RALF KISSMANN
Affiliation:
Institut für Astro- und Teilchenphysik, Universität Innsbruck, Innsbruck, Austria
FELIX SPANIER
Affiliation:
Lehrstuhl für Astronomie, Universität Würzburg, Emil-Fischer Str. 31, D-97074 Würzburg, Germany (fspanier@astro.uni-wuerzburg.de)
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Abstract

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Turbulence in the interstellar medium has been an active field of research in the last decade. Numerical simulations are the tool of choice in most cases. However, while there are a number of simulations on the market, some questions have not been answered finally. In this paper, we examine the influence of compressible and incompressible driving on the evolution of turbulent spectra in a number of possible interstellar medium scenarios. We conclude that the driving has an influence not only on the ratio of compressible to incompressible component but also on the anisotropy of turbulence.

Information

Type
Papers
Information
Journal of Plasma Physics , Volume 79 , Issue 5 , October 2013, pp. 597 - 612
Copyright
Copyright © Cambridge University Press 2013 

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