Turbulent magnetic field amplification driven by cosmic ray pressure gradients

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.427, Iss.3, 2012-12, pp. : 2308-2313

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Non-Linear Amplification of a Magnetic Field Driven by Cosmic Ray Streaming

By Lucek S.G. Bell A.R.

Astrophysics and Space Science, Vol. 272, Iss. 1-3, 2000-01 ,pp. : 255-262

Springer Publishing Company

Access to resources Recommend Favorite

Various regimes of cosmic ray diffusion in turbulent magnetic fields

By Laval G.

Astrophysics and Space Science, Vol. 277, Iss. 1-2, 2001-01 ,pp. : 27-34

Springer Publishing Company

Access to resources Recommend Favorite

Cosmic-Ray Momentum Diffusion in Magnetosonic versus Alfvénic Turbulent Field

By Michalek G. Ostrowski M. Schlickeiser R.

Solar Physics, Vol. 184, Iss. 2, 1999-02 ,pp. : 339-352

Springer Publishing Company

Access to resources Recommend Favorite

Magnetic field amplification and X-ray emission in galaxy minor mergers

By Geng Annette Kotarba Hanna Bürzle Florian Dolag Klaus Stasyszyn Federico Beck Alexander Nielaba Peter

Monthly Notices of the Royal Astronomical Society, Vol. 419, Iss. 4, 2012-02 ,pp. : 3571-3589

Oxford University Press

Access to resources Recommend Favorite

Strong cosmic-ray scattering in an anisotropic random magnetic field

By Mel’nikov Yu. Toptygin I.

Astronomy Letters, Vol. 31, Iss. 3, 2005-03 ,pp. : 186-193

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite