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Evolution of Magnetic Fields in Supernova Remnants
K. M. Schure, J. Vink, A. Achterberg +1
Supernova remnants (SNR) are now widely believed to be a source of cosmic rays (CRs) up to an energy of 1 PeV. The magnetic fields required to accelerate CRs to sufficiently high e…
Linear wave propagation in relativistic magnetohydrodynamics
R. Keppens, Z. Meliani
The properties of linear Alfvén, slow, and fast magnetoacoustic waves for uniform plasmas in relativistic magnetohydrodynamics (MHD) are discussed, augmenting the well-known expres…
A multidimensional grid-adaptive relativistic magnetofluid code
B. van der Holst, R. Keppens, Z. Meliani
A robust second order, shock-capturing numerical scheme for multi-dimensional special relativistic magnetohydrodynamics on computational domains with adaptive mesh refinement is pr…
Extragalactic jets with helical magnetic fields: relativistic MHD simulations
R. Keppens, Z. Meliani, B. van der Holst +1
Extragalactic jets are inferred to harbor dynamically important, organized magnetic fields which presumably aid in the collimation of the relativistic jet flows. We here explore by…