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Turbulent magnetic field amplification driven by cosmic ray pressure gradients

Published:2012-11-20 Issue:3 Volume:427 Page:2308-2313
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Drury L. O'C.¹,Downes T. P.

Affiliation:

1. School of Cosmic Physics; Dublin Institute for Advanced Studies; 31 Fitzwilliam Place; Dublin 2; Ireland

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/427/3/2308/3845577/427-3-2308.pdf

Reference27 articles.

1. X-ray synchrotron emission from supernova remnants

2. Thermal and Nonthermal X‐Rays from the Large Magellanic Cloud Superbubble 30 Doradus C

3. A Spatial and Spectral Study of Nonthermal Filaments in Historical Supernova Remnants: Observational Results withChandra

4. Acoustic instability driven by cosmic-ray streaming

5. Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays

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1. Magnetic Structures and Turbulence in SN 1006 Revealed with Imaging X-Ray Polarimetry;The Astrophysical Journal;2023-10-27

2. Reacceleration of Galactic Cosmic Rays beyond the Knee at the Termination Shock of a Cosmic-Ray-driven Galactic Wind;The Astrophysical Journal;2023-08-01

3. Lagrangian statistics of a shock-driven turbulent dynamo in decaying turbulence;Monthly Notices of the Royal Astronomical Society;2023-02-20

4. Study of the GeV to TeV morphology of the γ Cygni SNR (G 78.2+2.1) with MAGIC and Fermi-LAT;Astronomy & Astrophysics;2023-01-30

5. Turbulent Magnetic Field Amplification by the Interaction of a Shock Wave and Inhomogeneous Medium;The Astrophysical Journal;2022-12-01

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