Titlebook: Magnetic Fields in Diffuse Media; Alexander Lazarian,Elisabete M. de Gouveia Dal Pin Book 2015 Springer-Verlag Berlin Heidelberg 2015 astr

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https://doi.org/10.1007/978-3-662-44625-6astrophysical diffuse media; astrophysical magnetic fields; interstellar medium properties; magnetic tu

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0067-0057 medium and for star formation. Written by a group of leading experts the book represents an excellent overview of the field. Nonspecialists will find sufficient background to enter the field and be able to appreciate the state of the art.978-3-662-50722-3978-3-662-44625-6Series ISSN 0067-0057 Series E-ISSN 2214-7985

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Interstellar Grain Alignment: Observational Statusas having been empirically confirmed, the first two have failed some critical observational tests, whereas the latter has recently been given specific observational support and must now be viewed as the leading candidate.

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Synchrotron Radiation and Faraday Rotationtudy of Faraday rotation in particular, rapid development is taking place in techniques to confidently recover the physical conditions of the magnetoionized medium in the Milky Way and extragalactic objects.

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Kinetic Turbulenceence. Key questions about the nature of kinetic turbulence that drive current research efforts are identified. A comprehensive model of the kinetic turbulent cascade is presented, with a detailed discussion of each component of the model and a review of supporting and conflicting theoretical, numerical, and observational evidence.

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Interstellar Polarization and Magnetic Turbulencence in the magnetic field is necessarily an indirect process. In this chapter we explore several techniques and results for using polarimetry to explore the turbulent component of the magnetic field in the Galaxy.

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