The role of cooling induced by mixing in the mass and energy cycles of the solar atmosphere
In many astrophysical systems, mixing between cool and hot temperature gas/plasma through Kelvin-Helmholtz-instability-driven turbulence leads to the formation of an intermediate temperature phase with increased radiative losses that drive efficient cooling. The solar atmosphere is a potential site for this process to occur with interaction between
Hillier, Andrew et al.
Fecha de publicación:
4
2023