Magnetoacoustic Wave Energy from Numerical Simulations of an Observed Sunspot Umbra
We aim at reproducing the height dependence of sunspot wave signatures obtained from spectropolarimetric observations through three-dimensional MHD numerical simulations. A magnetostatic sunspot model based on the properties of the observed sunspot is constructed and perturbed at the photosphere, introducing the fluctuations measured with the Si I
Felipe, T. et al.
Fecha de publicación:
7
2011