The structure and statistics of interstellar turbulence

The structure and statistics of interstellar turbulence

We explore the structure and statistics of multiphase, magnetized ISM turbulence in the local Milky Way by means of driven periodic box numerical MHD simulations. Using the higher order-accurate piecewise-parabolic method on a local stencil (PPML), we carry out a small parameter survey varying the m...

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Bibliographic Details
Main Authors: A G Kritsuk, S D Ustyugov, M L Norman
Format: Article
Language:English
Published: IOP Publishing 2017-01-01
Series:New Journal of Physics
Subjects:
MHD turbulence
interstellar turbulence
interstellar clouds
star formation
47.27.–i
47.27.E–
Online Access:https://doi.org/10.1088/1367-2630/aa7156

Internet

https://doi.org/10.1088/1367-2630/aa7156

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