3D RMHD simulations with MURaM and RH1.5D radiative synthesis show plasmoid-mediated turbulent reconnection in small-scale events can produce coexisting hot and cool plasma that explains UV bursts connected with Ellerman bombs.
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Three dimensional magnetic reconnection mediated with plasmoids and the resulted multi-thermal emissions in the cool atmosphere of the Sun
3D RMHD simulations with MURaM and RH1.5D radiative synthesis show plasmoid-mediated turbulent reconnection in small-scale events can produce coexisting hot and cool plasma that explains UV bursts connected with Ellerman bombs.