Mexican Virtual Solar Observatory: Hydrodynamic simulations of the evolution of CMEs

Abstract

The Virtual Solar Observatory (VSO) concept contains software tools for searching, manipulating, and analyzing data from archives of solar data at many different observatories around the world (Hill 2000). The VSO not only provides fast and reliable access to existing solar data, but also represents a powerful and unique machinery to perform numerical simulations of a variety of different phenomena associated with solar activity. In this work we present the Numerical Model that the Mexican Virtual Solar Observatory (MVSO) uses to develop Remote Hydrodynamic Simulations to study the Evolution of Coronal Mass Ejection in the Interplanetary Medium.