CONICET | Buscador de Institutos y Recursos Humanos

Our proximity to the Sun allows us to obtain high resolution images turning ourstar into a natural plasma laboratory. The reasons why the solar atmosphere is hotter than itssurface are still a mystery. Recent observations have revealed that there is a large number andvariety of oscillations in the solar atmosphere that lead to a new interest in the mechanismsof wave heating. One way to contribute to the understanding of coronal heating is to studythese waves and oscillations that propagate in the solar corona, since they are capable oftransporting energy and information. In this research we study the propagation of waves andcoronal oscillations under a numerical approach comparing with direct observations.