Energy distribution and substructure formation in astrophysical MHD simulations
During substructure formation in magnetized astrophysical plasma, dissipation of magnetic
energy facilitated by magnetic reconnection affects the system dynamics by heating and …
energy facilitated by magnetic reconnection affects the system dynamics by heating and …
Estimating the rate of field line braiding in the solar corona by photospheric flows
S Candelaresi, DI Pontin, AR Yeates… - The Astrophysical …, 2018 - iopscience.iop.org
In this paper, we seek to understand the timescale in which the photospheric motions on the
Sun braid coronal magnetic field lines. This is a crucial ingredient for determining the …
Sun braid coronal magnetic field lines. This is a crucial ingredient for determining the …