Time evolution of cosmic-ray modified MHD shocks

T. W. Jones, H. Kang

Research output: Contribution to conferencePaperpeer-review

Abstract

We present initial simulation results for the time evolution of CR modified plane parallel shocks in magnetohydrodynamical flows. The simulations utilize our new and very efficient ?Coarse Grained finite Momentum Volume? (CGMV) transport scheme [6]. The simulations aim to explore nonlinear feedback among the particles, the wave turbulence and the bulk flows. The calculations incorporate self-consistent treatment of the momentum-dependent CR diffusion convection equation and will soon be coupled with wave action equations for resonantly scattering Alfven and fast mode waves, also treated through the CGMV scheme. Recent advances in MHD turbulence theory require a broadened outlook on scattering processes in CR modified shocks.

Original languageEnglish (US)
Pages269-272
Number of pages4
StatePublished - Jan 1 2005
Event29th International Cosmic Ray Conference, ICRC 2005 - Pune, India
Duration: Aug 3 2005Aug 10 2005

Other

Other29th International Cosmic Ray Conference, ICRC 2005
CountryIndia
CityPune
Period8/3/058/10/05

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