Coronal heating in coupled photosphere-chromosphere-coronal systems: turbulence and leakage
Coronal heating in coupled photosphere-chromosphere-coronal systems: turbulence and leakage
Context. Coronal loops act as resonant cavities for low-frequency fluctuations that are transmitted from the deeper layers of the solar atmosphere. These fluctuations are amplified in the corona and lead to the development of turbulence that in turn is able to dissipate the accumulated energy, thus heating the corona. However, …