Evidence for rotational motions in the feet of a quiescent solar prominence
D. Orozco Su\'arez, A. Asensio Ramos, and J. Trujillo Bueno

TL;DR
This study provides spectroscopic evidence of apparent rotational plasma motions in the feet of a quiescent solar prominence, indicating swirling motions and counter-streaming flows, enhancing understanding of prominence dynamics.
Contribution
First spectroscopic detection of rotational motions in prominence feet using He I 1083.0 nm data, revealing complex plasma flows and counter-streaming phenomena.
Findings
Opposite Doppler shifts of ±6 km/s at prominence edges
Evidence of plasma rotating counterclockwise around the vertical axis
Presence of supersonic counter-streaming flows up to 20 km/s
Abstract
We present observational evidence of apparent plasma rotational motions in the feet of a solar prominence. Our study is based on spectroscopic observations taken in the He I 1083.0 nm multiplet with the Tenerife Infrared Polarimeter attached to the German Vacuum Tower Telescope. We recorded a time sequence of spectra with 34 s cadence placing the slit of the spectrograph almost parallel to the solar limb and crossing two feet of an intermediate size, quiescent hedgerow prominence. The data show opposite Doppler shifts, +/- 6 km/s, at the edges of the prominence feet. We argue that these shifts may be interpreted as prominence plasma rotating counterclockwise around the vertical axis to the solar surface as viewed from above. The evolution of the prominence seen in EUV images taken with the Solar Dynamic Observatory provided us clues to interpret the results as swirling motions.…
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