In this paper we present a second order finite volume method for the resolu
tion of the bidimensional ideal MHD equations on adaptively refined triangu
lar meshes. Our numerical flux function is based on a multidimensional exte
nsion of the Roe scheme proposed by Cargo and Gallice for the 1D MHD system
. If the mesh is only composed of triangles, our scheme is proved to be wea
kly consistent with the condition del . B = 0. This property fails on a car
tesian grid. The efficiency of our refinement procedure is shown on 2D MHD
shock capturing simulations. Numerical results are compared in case of the
interaction of a supersonic plasma with a cylinder on the adapted grid and
several non-refined grids. We also present a mass loading simulation which
corresponds to a 2D version of the interaction between the solar wind and a
comet. (C) 1999 Academic Press.