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...
Published in: | The Astrophysical Journal |
---|---|
Main Authors: | , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
IOP Publishing
|
Subjects: | |
Online Access: | http://hdl.handle.net/11336/174484 |
id |
ftconicet:oai:ri.conicet.gov.ar:11336/174484 |
---|---|
record_format |
openpolar |
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 |
_version_ |
1779319859961659392 |