Stellar feedback drives the circulation of matter from the disk to the halo of galaxies. We
perform three-dimensional magnetohydrodynamic simulations of a vertical column of the …

We present a highly robust second order accurate scheme for the Euler equations and the
ideal MHD equations. The scheme is of predictor–corrector type, with a MUSCL scheme …

The ideal MHD equations are a central model in astrophysics, and their solution relies upon
stable numerical schemes. We present an implementation of a new method, which …

Adaptive immune receptor repertoires (AIRR) are key targets for biomedical research as they
record past and ongoing adaptive immune responses. The capacity of machine learning (…

We present a relaxation system for ideal magnetohydrodynamics (MHD) that is an extension
of the Suliciu relaxation system for the Euler equations of gas dynamics. From it one can …

In the first part of this work Bouchut et al. (J Comput Phys 108:7–41, 2007) we introduced an
approximate Riemann solver for one-dimensional ideal MHD derived from a relaxation …

To perform probabilistic tsunami hazard assessment for subduction zone earthquakes, it is
necessary to start with a catalog of possible future events along with the annual probability of …

The idea of this work is to compare a new positive and entropy stable approximate Riemann
solver by Francois Bouchut with a state-of the-art algorithm for astrophysical fluid dynamics. …

Wave propagation in idealized stellar atmospheres is modeled by the equations of ideal
MHD, together with the gravity source term. The waves are modeled as small perturbations of …

We design stable and high-order accurate finite volume schemes for the ideal MHD equations
in multi-dimensions. We obtain excellent numerical stability due to some new elements in …