Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line

Magnetic fields in turbulent, convective high-β plasma naturally develop highly tangled and complex topologies - the solar photosphere being the paradigmatic example. These fields are mostly undetectable by standard diagnostic techniques with finite spatio-temporal resolution due to cancellations of...

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Published in:The Astrophysical Journal
Main Authors: Zeuner, Franziska, Manso Sainz, Rafael, Feller, Alex, van Noort, Michiel, Solanki, Sami K., Iglesias, Francisco Andres, Reardon, Kevin, Martínez Pillet, Valentín
Format: Article in Journal/Newspaper
Language:English
Published: IOP Publishing
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Online Access:http://hdl.handle.net/11336/174484
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spelling ftconicet:oai:ri.conicet.gov.ar:11336/174484 2023-10-09T21:55:47+02:00 Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line Zeuner, Franziska Manso Sainz, Rafael Feller, Alex van Noort, Michiel Solanki, Sami K. Iglesias, Francisco Andres Reardon, Kevin Martínez Pillet, Valentín application/pdf http://hdl.handle.net/11336/174484 eng eng IOP Publishing info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/ab86b8 info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/ab86b8 http://hdl.handle.net/11336/174484 Zeuner, Franziska; Manso Sainz, Rafael; Feller, Alex; van Noort, Michiel; Solanki, Sami K.; et al.; Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line; IOP Publishing; Astrophysical Journal Letters; 893; 2; 4-2020; 1-8 2041-8213 CONICET Digital CONICET info:eu-repo/semantics/restrictedAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ Spectropolarimetry Quiet sun Solar magnetic fields https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion ftconicet https://doi.org/10.3847/2041-8213/ab86b8 2023-09-24T20:34:19Z Magnetic fields in turbulent, convective high-β plasma naturally develop highly tangled and complex topologies - the solar photosphere being the paradigmatic example. These fields are mostly undetectable by standard diagnostic techniques with finite spatio-temporal resolution due to cancellations of Zeeman polarization signals. Observations of resonance scattering polarization have been considered to overcome these problems. But up to now, observations of scattering polarization lack the necessary combination of high sensitivity and high spatial resolution in order to directly infer the turbulent magnetic structure at the resolution limit of solar telescopes. Here, we report the detection of clear spatial structuring of scattering polarization in a magnetically quiet solar region at disk center in the Sr i 4607 Å spectral line on granular scales, confirming theoretical expectations. We find that the linear polarization presents a strong spatial correlation with the local quadrupole of the radiation field. The result indicates that polarization survives the dynamic and turbulent magnetic environment of the middle photosphere and is thereby usable for spatially resolved Hanle observations. This is an important step toward the long-sought goal of directly observing turbulent solar magnetic fields at the resolution limit and investigating their spatial structure. Fil: Zeuner, Franziska. Universität Göttingen; Alemania Fil: Manso Sainz, Rafael. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Feller, Alex. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: van Noort, Michiel. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Solanki, Sami K. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Iglesias, Francisco Andres. Universidad Tecnológica Nacional. Facultad Regional de Mendoza; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina Fil: Reardon, Kevin. National Solar Observatory; ... Article in Journal/Newspaper sami CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas) Argentina The Astrophysical Journal 893 2 L44
institution Open Polar
collection CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas)
op_collection_id ftconicet
language English
topic Spectropolarimetry
Quiet sun
Solar magnetic fields
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
spellingShingle Spectropolarimetry
Quiet sun
Solar magnetic fields
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
Zeuner, Franziska
Manso Sainz, Rafael
Feller, Alex
van Noort, Michiel
Solanki, Sami K.
Iglesias, Francisco Andres
Reardon, Kevin
Martínez Pillet, Valentín
Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line
topic_facet Spectropolarimetry
Quiet sun
Solar magnetic fields
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
description Magnetic fields in turbulent, convective high-β plasma naturally develop highly tangled and complex topologies - the solar photosphere being the paradigmatic example. These fields are mostly undetectable by standard diagnostic techniques with finite spatio-temporal resolution due to cancellations of Zeeman polarization signals. Observations of resonance scattering polarization have been considered to overcome these problems. But up to now, observations of scattering polarization lack the necessary combination of high sensitivity and high spatial resolution in order to directly infer the turbulent magnetic structure at the resolution limit of solar telescopes. Here, we report the detection of clear spatial structuring of scattering polarization in a magnetically quiet solar region at disk center in the Sr i 4607 Å spectral line on granular scales, confirming theoretical expectations. We find that the linear polarization presents a strong spatial correlation with the local quadrupole of the radiation field. The result indicates that polarization survives the dynamic and turbulent magnetic environment of the middle photosphere and is thereby usable for spatially resolved Hanle observations. This is an important step toward the long-sought goal of directly observing turbulent solar magnetic fields at the resolution limit and investigating their spatial structure. Fil: Zeuner, Franziska. Universität Göttingen; Alemania Fil: Manso Sainz, Rafael. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Feller, Alex. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: van Noort, Michiel. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Solanki, Sami K. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Iglesias, Francisco Andres. Universidad Tecnológica Nacional. Facultad Regional de Mendoza; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina Fil: Reardon, Kevin. National Solar Observatory; ...
format Article in Journal/Newspaper
author Zeuner, Franziska
Manso Sainz, Rafael
Feller, Alex
van Noort, Michiel
Solanki, Sami K.
Iglesias, Francisco Andres
Reardon, Kevin
Martínez Pillet, Valentín
author_facet Zeuner, Franziska
Manso Sainz, Rafael
Feller, Alex
van Noort, Michiel
Solanki, Sami K.
Iglesias, Francisco Andres
Reardon, Kevin
Martínez Pillet, Valentín
author_sort Zeuner, Franziska
title Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line
title_short Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line
title_full Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line
title_fullStr Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line
title_full_unstemmed Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line
title_sort solar disk center shows scattering polarization in the sr i 4607 å line
publisher IOP Publishing
url http://hdl.handle.net/11336/174484
geographic Argentina
geographic_facet Argentina
genre sami
genre_facet sami
op_relation info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2041-8213/ab86b8
info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/ab86b8
http://hdl.handle.net/11336/174484
Zeuner, Franziska; Manso Sainz, Rafael; Feller, Alex; van Noort, Michiel; Solanki, Sami K.; et al.; Solar Disk Center Shows Scattering Polarization in the Sr i 4607 Å Line; IOP Publishing; Astrophysical Journal Letters; 893; 2; 4-2020; 1-8
2041-8213
CONICET Digital
CONICET
op_rights info:eu-repo/semantics/restrictedAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
op_doi https://doi.org/10.3847/2041-8213/ab86b8
container_title The Astrophysical Journal
container_volume 893
container_issue 2
container_start_page L44
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