“…We note that a significant number of flux-emergence simulations incorporated additional physics, such as convective motions, radiative heating and cooling, heat conduction, ambipolar diffusion, ion-neutral interactions, and non-equilibrium ionization (e.g., Leake and Arber, 2006;Stein and Nordlund, 2006;Cameron et al, 2007;Martínez-Sykora et al, 2008;Isobe et al, 2008;Cheung et al, 2010;Fang et al, 2010;Rempel and Cheung, 2014;Chen et al, 2017;Hansteen et al, 2017;Moreno-Insertis et al, 2018;Nóbrega-Siverio et al, 2018;Cheung et al, 2019;Toriumi and Hotta, 2019). These simulations are necessary for studying the thermodynamical aspects of phenomena related to flux emergence and the atmospheric response to the dynamic emergence of solar magnetic fields.…”