A small chromospheric jet is shown to be driven by a two-stage reconnection process: separating magnetic footpoints produce a cool jet, then converging footpoints stretch the current sheet, trigger a plasmoid, and generate a hot EUV jet.
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From Photospheric Footpoint Motion to Plasmoid Ejection: A Two-Stage Reconnection Process in a Small-scale Chromospheric Jet
A small chromospheric jet is shown to be driven by a two-stage reconnection process: separating magnetic footpoints produce a cool jet, then converging footpoints stretch the current sheet, trigger a plasmoid, and generate a hot EUV jet.