Supra-arcade downflows in a quiescent filament eruption are at least three times wider than active-region counterparts but move at similar speeds, supporting a Rayleigh-Taylor instability origin.
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Supra-arcade downflows in an extensive fan associated with a giant quiescent solar filament eruption
Supra-arcade downflows in a quiescent filament eruption are at least three times wider than active-region counterparts but move at similar speeds, supporting a Rayleigh-Taylor instability origin.