On the Origin of the Type II Spicules: Dynamic Three-dimensional MHD Simulations
Recent high temporal and spatial resolution observations of the chromosphere have forced the definition of a new type of spicule, "type II's," that are characterized by rising rapidly, having short lives, and by fading away at the end of their lifetimes. Here, we report on features found in realistic three-dimensional simulations of the outer solar
Martínez-Sykora, Juan et al.
Fecha de publicación:
7
2011