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Spectropolarimetric fluctuations in a sunspot chromosphere

Stangalini, M; Baker, D; Valori, G; Jess, DB; Jafarzadeh, S; Murabito, M; To, ASH; ... MacBride, CD; + view all (2021) Spectropolarimetric fluctuations in a sunspot chromosphere. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences , 379 (2190) , Article 20200216. 10.1098/rsta.2020.0216. Green open access

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Abstract

The instrumental advances made in this new era of 4 m class solar telescopes with unmatched spectropolarimetric accuracy and sensitivity will enable the study of chromospheric magnetic fields and their dynamics with unprecedented detail. In this regard, spectropolarimetric diagnostics can provide invaluable insight into magneto-hydrodynamic (MHD) wave processes. MHD waves and, in particular, Alfvénic fluctuations associated with particular wave modes were recently recognized as important mechanisms not only for the heating of the outer layers of the Sun’s atmosphere and the acceleration of the solar wind, but also for the elemental abundance anomaly observed in the corona of the Sun and other Sun-like stars (also known as first ionization potential) effect. Here, we take advantage of state-of-the-art and unique spectropolarimetric Interferometric BIdimensional Spectrometer observations to investigate the relation between intensity and circular polarization (CP) fluctuations in a sunspot chromosphere. Our results show a clear link between the intensity and CP fluctuations in a patch which corresponds to a narrow range of magnetic field inclinations. This suggests the presence of Alfvénic perturbations in the sunspot. This article is part of the Theo Murphy meeting issue ‘High-resolution wave dynamics in the lower solar atmosphere’.

Type: Article
Title: Spectropolarimetric fluctuations in a sunspot chromosphere
Open access status: An open access version is available from UCL Discovery
DOI: 10.1098/rsta.2020.0216
Publisher version: https://doi.org/10.1098/rsta.2020.0216
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher's terms and conditions.
Keywords: solar MHD waves, chromospheric dynamics, solar spectropolarimetry
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10120382
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