On magnetic field amplification and particle acceleration near non-relativistic astrophysical shocks: particles in MHD cells simulations-Reference-Cited by-同舟云学术

On magnetic field amplification and particle acceleration near non-relativistic astrophysical shocks: particles in MHD cells simulations

Published:2017-09-27 Issue:3 Volume:473 Page:3394-3409
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

van Marle Allard Jan¹,Casse Fabien¹,Marcowith Alexandre²

Affiliation:

1. Laboratoire AstroParticle and Cosmologie (APC), Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10 rue Alice Domon et Leonie Duquet, F-75205 Paris Cedex 13, France

2. Laboratoire Univers et Particules de Montpellier (LUPM) Université Montpellier, CNRS/IN2P3, CC72, place Eugène Bataillon, F-34095 Montpellier Cedex 5, France

Funder

Labex

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/473/3/3394/21750596/stx2509.pdf

Reference29 articles.

1. MAGNETOHYDRODYNAMIC-PARTICLE-IN-CELL METHOD FOR COUPLING COSMIC RAYS WITH A THERMAL PLASMA: APPLICATION TO NON-RELATIVISTIC SHOCKS

2. A Staggered Mesh Algorithm Using High Order Godunov Fluxes to Ensure Solenoidal Magnetic Fields in Magnetohydrodynamic Simulations

3. The acceleration of cosmic rays in shock fronts - I