A rising cool column as signature for helical flux emergence and formation of prominence and coronal cavity
Takenori J. Okamoto, Saku Tsuneta, and Thomas E. Berger

TL;DR
This study observes a rising cool plasma column associated with a coronal cavity, interpreting it as evidence of helical flux emergence and reconnection, which influences prominence formation and coronal dynamics.
Contribution
It provides the first detailed observation linking a rising cool column to helical flux emergence and reconnection processes in the solar corona.
Findings
A cool plasma column rises at 2 km/s with fine structures moving up to 20 km/s.
The coronal cavity moves upward at about 5 km/s during the event.
The observations support the emergence of a helical flux rope causing prominence and cavity dynamics.
Abstract
Continuous observations were performed of a quiescent prominence with the Solar Optical Telescope (SOT) on board the /emph{Hinode} satellite on 2006 December 23--24. A peculiar slowly-rising column of K plasma develops from the lower atmosphere during the observations. The apparent ascent speed of the column is 2 km s, while the fine structures of the column exhibit much faster motion of up to 20 km s. The column eventually becomes a faint low-lying prominence. Associated with the appearance of the column, an overlying coronal cavity seen in the X-ray and EUV moves upward at 5 km s. We discuss the relationship between these episodes, and suggest that they are due to the emergence of a helical flux rope that undergoes reconnection with lower coronal fields, possibly carrying material into the coronal cavity. Under the assumption of the emerging…
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