Coronal mass ejections (CMEs) are eruptions into interplanetary
space of as much as a few billion tons of plasma and embedded
magnetic fields from the Sun's corona. In this work we present the
preliminary results of the software development for execute MHD remote
numerical simulations of the CME's through a web interface and store
the results into a database; this new astrophysical computational tool
are oriented to observational astronomers that need additional details
of the theoretical models in order to interpreted their data.