Magnetic Fields in Diffuse Media

Author:   Alexander Lazarian ,  Elisabete M. de Gouveia Dal Pino ,  Claudio Melioli
Publisher:   Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
Edition:   Softcover reprint of the original 1st ed. 2015
Volume:   407
ISBN:  

9783662507223


Pages:   623
Publication Date:   23 August 2016
Format:   Paperback
Availability:   Manufactured on demand   Availability explained
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Magnetic Fields in Diffuse Media


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Author:   Alexander Lazarian ,  Elisabete M. de Gouveia Dal Pino ,  Claudio Melioli
Publisher:   Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
Imprint:   Springer-Verlag Berlin and Heidelberg GmbH & Co. K
Edition:   Softcover reprint of the original 1st ed. 2015
Volume:   407
Dimensions:   Width: 15.50cm , Height: 3.30cm , Length: 23.50cm
Weight:   9.591kg
ISBN:  

9783662507223


ISBN 10:   3662507226
Pages:   623
Publication Date:   23 August 2016
Audience:   Professional and scholarly ,  Professional & Vocational
Format:   Paperback
Publisher's Status:   Active
Availability:   Manufactured on demand   Availability explained
We will order this item for you from a manufactured on demand supplier.

Table of Contents

Future Observations of Cosmic Magnetic Fields with LOFAR, SKA and its precursors.- Magnetic fields with the Atacama Large Millimeter/submillimeter Array.- Synchrotron radiation and Faraday rotation.- Interstellar Grain Alignment – Observational Status.- Magnetic Field Measurement with Ground State Alignment.- Kinetic Turbulence.- Interstellar Polarization and Magnetic Turbulence.- MHD Turbulence and its Implications.- The intermittency of ISM turbulence : what do the observations tell us?.- Ambipolar Diffusion.- Magnetic Reconnection in Astrophysical Environments.- Interstellar MHD Turbulence and Star Formation.- Observations of Magnetic Fields in Molecular Clouds—Testing Star Formation Theory.- Magnetic Fields in Star Formation.- Particle Acceleration by Magnetic Reconnection.- Cosmic Ray transport in turbulent magnetic field.- Magnetic Fields in the Milky Way.- Magnetic fields in galaxies.- Simulations of galactic dynamos.- Cosmic rays in galaxy clusters and their interaction with magnetic fields.- Turbulence in the intracluster medium.

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