High order explicit Runge-Kutta pairs for ephemerides of the solar system and the Moon.
Note sur l'article précédent
Numerical simulations in astrophysics: Supernovae explosions, magnetorotational model and neutrino emission.
Sur la construction graphique de la courbe d'ombre ou de pénombre pendant la durée d'une éclipse de soleil
Sur la parallaxe du soleil déduite des observations méridiennes de Mars en 1862
Time-dependent numerical modeling of large-scale astrophysical processes: from relatively smooth flows to explosive events with extremely large discontinuities and high Mach numbers
We calculate self-consistent time-dependent models of astrophysical processes. We have developed two types of our own (magneto) hydrodynamic codes, either the operator-split, finite volume Eulerian code on a staggered grid for smooth hydrodynamic flows, or the finite volume unsplit code based on the Roe's method for explosive events with extremely large discontinuities and highly supersonic outbursts. Both the types of the codes use the second order Navier-Stokes viscosity to realistically model...