Kinetic–MHD simulations of gyroresonance instability driven by CR pressure anisotropy
Author:
Affiliation:
1. DESY, Platanenallee 6, D-15738 Zeuthen, Germany
2. Institut für Physik und Astronomie, Universität Potsdam, D-14476 Potsdam-Golm, Germany
3. Taras Shevchenko National University of Kyiv, 64/13, Volodymyrska Street, 01601 Kyiv, Ukraine
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/476/2/2779/24422177/sty309.pdf
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3. Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
4. Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field
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