A new numerical code for hydrodynamical 3D simulations of supernova remnants
We develop a 3D hydrodynamical code written in C programming language to study the expansion of supernova remnants (SNRs) in the surrounding medium.It is based on the MUSCL-Hancock finite volume scheme with the HLLC Riemann solver.The code initiates the supernova remnant already in the Sedov phase and simulates hydrodynamics of the subsequent remna