This work presents a new plasma cooling curve that is calculated using the SPEX package.
We compare our cooling rates to those in previous works, and implement the new cooling …

Following on from the companion volume Principles of Magnetohydrodynamics, this
textbook analyzes the applications of plasma physics to thermonuclear fusion and plasma …

Relativistic hydro and magnetohydrodynamics provide continuum fluid descriptions for gas
and plasma dynamics throughout the visible universe. We present an overview of state-of-the-…

In this paper, we present an update to the open source MPI-AMRVAC simulation toolkit where
we focus on solar and non-relativistic astrophysical magnetofluid dynamics. We highlight …

Aims. We re-examine the conditions required to steadily deviate an accretion flow from a
circumstellar disc into a magnetospheric funnel flow onto a slow rotating young forming star.…

We present numerical magnetohydrodynamic (MHD) simulations of a magnetized accretion
disk launching trans-Alfvénic jets. These simulations, performed in a 2.5-dimensional time-…

Context. Computational astrophysics nowadays routinely combines grid-adaptive capabilities
with modern shock-capturing, high resolution spatio-temporal integration schemes in …

In this paper, we give a detailed account of the first three-dimensional (3D) relativistic
magnetohydrodynamic simulations of pulsar wind nebulae, with parameters most suitable for the …

Obtainable computational efficiency is evaluated when using an Adaptive Mesh Refinement
(AMR) strategy in time accurate simulations governed by sets of conservation laws. For a …

We investigate the Kelvin–Helmholtz instability occurring at the interface of a shear-flow
configuration in 2D compressible magnetohydrodynamics (MHD). The linear growth and the …