Unveiling the magnetic nature of chromospheric vortices
Mariarita Murabito, Juie Shetye, Marco Stangalini, Erwin Verwichte,, Tony Arber, Ilaria Ermolli, Fabrizio Giorgi, Tom Goffrey

TL;DR
This study reveals that chromospheric vortices in the Sun are magnetic structures with observable rotational patterns, plasma flows, and possible magnetic connections, advancing understanding of solar atmospheric dynamics.
Contribution
First spectropolarimetric detection of magnetic chromospheric vortices, demonstrating their magnetic nature and potential magnetic connectivity in the solar atmosphere.
Findings
Chromospheric vortices are magnetic structures with significant circular polarization signals.
Plasma flows are observed around the vortex structures, indicating dynamic activity.
Simulations suggest magnetic connection and wave phenomena contribute to vortex behavior.
Abstract
Vortex structures in the Sun's chromosphere are believed to channel energy between different layers of the solar atmosphere. We investigate the nature and dynamics of two small-scale quiet-Sun rotating structures in the chromosphere. We analyse two chromospheric structures that show clear rotational patterns in spectropolarimetric observations taken with the Interferometric Bidimensional Spectrometer (IBIS) at the Ca II 8542 \AA~ line. We present the detection of spectropolarimetric signals that manifest the magnetic nature of rotating structures in the chromosphere. Our observations show two long-lived structures of plasma that each rotate clockwise inside a 10 arcsec~ quiet-Sun region. Their circular polarization signals are 5-10 times above the noise level. Line-of-sight Doppler velocity and horizontal velocity maps from the observations reveal clear plasma flows at and around…
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