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dc.contributor.authorFalceta-Goncalves, D.
dc.contributor.authorKowal, G.
dc.contributor.authorFalgarone, E.
dc.contributor.authorChian, A. C. -L.
dc.date.accessioned2014-08-11T15:01:06Z
dc.date.available2014-08-11T15:01:06Z
dc.date.issued2014-05-16
dc.identifier.citationFalceta-Goncalves , D , Kowal , G , Falgarone , E & Chian , A C -L 2014 , ' Turbulence in the interstellar medium ' , Nonlinear processes in geophysics , vol. 21 , no. 3 , pp. 587-604 . https://doi.org/10.5194/npg-21-587-2014en
dc.identifier.issn1023-5809
dc.identifier.otherPURE: 139599612
dc.identifier.otherPURE UUID: 8e205de9-e8da-4110-8dbf-90ff0b3990f6
dc.identifier.otherWOS: 000338651000002
dc.identifier.otherScopus: 84901401435
dc.identifier.otherWOS: 000338651000002
dc.identifier.urihttp://hdl.handle.net/10023/5108
dc.descriptionD. Falceta-Gonçalves thanks the European Research Council (ADG-2011 ECOGAL) and Brazilian agencies CNPq (no. 300382/2008-1), CAPES (3400-13-1) and FAPESP (no. 2011/12909-8) for financial support. G. Kowal acknowledges support from FAPESP grant no. 2013/04073-2. A. C.-L. Chian thanks the European Commission for the award of a Marie Curie International Incoming Fellowship and CNPq for support.en
dc.description.abstractTurbulence 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.
dc.format.extent18
dc.language.isoeng
dc.relation.ispartofNonlinear processes in geophysicsen
dc.rights© Author(s) 2014. This work is distributed under the Creative Commons Attribution 3.0 License (https://creativecommons.org/licenses/by/3.0/).en
dc.subjectSmall-magellanic-clouden
dc.subjectGalactic molecular cloudsen
dc.subjectCompressible magnetohydrodynamic turbulenceen
dc.subjectMagnetic-field turbulenceen
dc.subjectPower spectrum analysisen
dc.subjectUniversal scaling lawsen
dc.subjectSolar-winden
dc.subjectMHD turbulenceen
dc.subjectStar-formationen
dc.subjectH2O masersen
dc.subjectQB Astronomyen
dc.subject.lccQBen
dc.titleTurbulence in the interstellar mediumen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.5194/npg-21-587-2014
dc.description.statusPeer revieweden
dc.identifier.urlhttp://www.nonlin-processes-geophys.net/21/587/2014/en


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