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Turbulence in the interstellar medium

اضطراب في الوسط بين النجمي
descriptionPublicationkeyboard_double_arrow_right Article , Other literature type , Preprint 16 May 2014Embargo end date: 01 Jan 2014 France, France, France, Australia, France, United Kingdom, France, France Publisher:Copernicus GmbHJournal:Nonlinear Processes in Geophysics, volume 21, pages 587-604 (eissn: 1607-7946, Copyright policy )Funded by:EC | ECOGAL
Authors: Diego Falceta-Gonçalves; Diego Falceta-Gonçalves; Grzegorz Kowal; Abraham C.-L. Chian; Abraham C.-L. Chian; Abraham C.-L. Chian; E. Falgarone;

doi: 10.5194/npg-21-587-2014 , 10.48550/arxiv.1404.3691 , 10.60692/0k4b0-rww16 , 10.60692/1f6qz-7a079

arXiv: http://arxiv.org/abs/1404.3691

handle: 10023/5108 , 2440/94515

Turbulence in the interstellar medium

Abstract

Abstract. Turbulence is ubiquitous in the insterstellar medium and plays a major role in several processes such as the formation of dense structures and stars, the stability of molecular clouds, the amplification of magnetic fields, and the re-acceleration and diffusion of cosmic rays. Despite its importance, interstellar turbulence, like turbulence in general, is far from being fully understood. In this review we present the basics of turbulence physics, focusing on the statistics of its structure and energy cascade. We explore the physics of compressible and incompressible turbulent flows, as well as magnetised cases. The most relevant observational techniques that provide quantitative insights into interstellar turbulence are also presented. We also discuss the main difficulties in developing a three-dimensional view of interstellar turbulence from these observations. Finally, we briefly present what the main sources of turbulence in the interstellar medium could be.

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France, France, France, Australia, France, United Kingdom, France, France
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Keywords

Astronomy, Geophysics. Cosmic physics, Universal scaling laws, Stellar Astrophysics and Exoplanet Studies, Astrophysics, Power spectrum analysis, [PHYS] Physics [physics], Physics - Space Physics, Interstellar medium, QB Astronomy, QB, [PHYS]Physics [physics], Earth and Planetary Astrophysics (astro-ph.EP), Physics, Q, 520, MHD turbulence, Physical Sciences, Local Bubble, Science, QC1-999, Small-magellanic-cloud, FOS: Physical sciences, Molecular cloud, Mechanics, 530, 532, Solar-wind, Star Formation in Molecular Clouds and Protoplanetary Disks, Magnetohydrodynamic Turbulence, Compressible magnetohydrodynamic turbulence, Magnetic-field turbulence, H2O masers, Interstellar Medium, Solar Physics and Space Weather, QC801-809, Galactic molecular clouds, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Stars, Physics - Plasma Physics, Space Physics (physics.space-ph), Turbulence, Plasma Physics (physics.plasm-ph), Galaxy, Physics and Astronomy, Energy cascade, Astrophysics of Galaxies (astro-ph.GA), Star-formation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Astrophysics - Earth and Planetary Astrophysics

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
59
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