The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis
International audience The thermospheric atomic oxygen red line is among the brightest in the auroral spectrum. Previous observations in Longyearbyen, Svalbard, indicated that it may be intrinsically polarized, but a possible contamination by light pollution could not be ruled out. During the winter...
Published in: | Journal of Space Weather and Space Climate |
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Main Authors: | , , , , , , , , , |
Other Authors: | , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2013
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Subjects: | |
Online Access: | https://hal.science/hal-02382457 https://hal.science/hal-02382457/document https://hal.science/hal-02382457/file/swsc120007.pdf https://doi.org/10.1051/swsc/2012023 |
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openpolar |
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Open Polar |
collection |
Université de Paris: Portail HAL |
op_collection_id |
ftunivparis |
language |
English |
topic |
[SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
spellingShingle |
[SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] Lilensten, Jean Barthelemy, Mathieu Amblard, Pierre-Olivier Lamy, Hervé Wedlund, Cyril Simon Bommier, Véronique Moen, Joran Rothkaehl, Hanna Eymard, Julien Ribot, Jocelyn The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis |
topic_facet |
[SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
description |
International audience The thermospheric atomic oxygen red line is among the brightest in the auroral spectrum. Previous observations in Longyearbyen, Svalbard, indicated that it may be intrinsically polarized, but a possible contamination by light pollution could not be ruled out. During the winter 2010/2011, the polarization of the red line was measured for the first time at the Polish Hornsund polar base without contamination. Two methods of data analysis are presented to compute the degree of linear polarization (DoLP) and angle of linear polarization (AoLP): one is based on averaging and the other one on filtering. Results are compared and are in qualitative agreement. For solar zenith angles (SZA) larger than 108°(with no contribution from Rayleigh scattering), the DoLP ranges between 2 and 7%. The AoLP is more or less aligned with the direction of the magnetic field line, in agreement with the theoretical predictions of Bommier et al. (2010). However, the AoLP values range between ±20°around this direction, depending on the auro-ral conditions. Correlations between the polarization parameters and the red line intensity I were considered. The DoLP decreases when I increases, confirming a trend observed during the observations in Longyearbyen. However, for small values of I, DoLP varies within a large range of values, while for large values of I, DoLP is always small. The AoLP also varies with the red line intensity, slightly rotating around the magnetic field line. |
author2 |
Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ) Observatoire des Sciences de l'Univers de Grenoble (OSUG) Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS) GIPSA - Communication Information and Complex Systems (GIPSA-CICS) Département Images et Signal (GIPSA-DIS) Grenoble Images Parole Signal Automatique (GIPSA-lab) Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Grenoble Images Parole Signal Automatique (GIPSA-lab) Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS) Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB) Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA) Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS) Department of Physics Oslo Faculty of Mathematics and Natural Sciences Oslo University of Oslo (UiO)-University of Oslo (UiO) Space Research Centre of Polish Academy of Sciences (CBK) Polska Akademia Nauk = Polish Academy of Sciences = Académie polonaise des sciences (PAN) |
format |
Article in Journal/Newspaper |
author |
Lilensten, Jean Barthelemy, Mathieu Amblard, Pierre-Olivier Lamy, Hervé Wedlund, Cyril Simon Bommier, Véronique Moen, Joran Rothkaehl, Hanna Eymard, Julien Ribot, Jocelyn |
author_facet |
Lilensten, Jean Barthelemy, Mathieu Amblard, Pierre-Olivier Lamy, Hervé Wedlund, Cyril Simon Bommier, Véronique Moen, Joran Rothkaehl, Hanna Eymard, Julien Ribot, Jocelyn |
author_sort |
Lilensten, Jean |
title |
The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis |
title_short |
The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis |
title_full |
The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis |
title_fullStr |
The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis |
title_full_unstemmed |
The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis |
title_sort |
thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis |
publisher |
HAL CCSD |
publishDate |
2013 |
url |
https://hal.science/hal-02382457 https://hal.science/hal-02382457/document https://hal.science/hal-02382457/file/swsc120007.pdf https://doi.org/10.1051/swsc/2012023 |
genre |
Hornsund Longyearbyen Svalbard |
genre_facet |
Hornsund Longyearbyen Svalbard |
op_source |
ISSN: 2115-7251 EISSN: 2115-7251 Journal of Space Weather and Space Climate https://hal.science/hal-02382457 Journal of Space Weather and Space Climate, 2013, 3, pp.A01. ⟨10.1051/swsc/2012023⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1051/swsc/2012023 hal-02382457 https://hal.science/hal-02382457 https://hal.science/hal-02382457/document https://hal.science/hal-02382457/file/swsc120007.pdf BIBCODE: 2013JSWSC.3A.01L doi:10.1051/swsc/2012023 |
op_rights |
http://creativecommons.org/licenses/by/ info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1051/swsc/2012023 |
container_title |
Journal of Space Weather and Space Climate |
container_volume |
3 |
container_start_page |
A01 |
_version_ |
1799481297785061376 |
spelling |
ftunivparis:oai:HAL:hal-02382457v1 2024-05-19T07:41:42+00:00 The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis Lilensten, Jean Barthelemy, Mathieu Amblard, Pierre-Olivier Lamy, Hervé Wedlund, Cyril Simon Bommier, Véronique Moen, Joran Rothkaehl, Hanna Eymard, Julien Ribot, Jocelyn Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ) Observatoire des Sciences de l'Univers de Grenoble (OSUG) Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS) GIPSA - Communication Information and Complex Systems (GIPSA-CICS) Département Images et Signal (GIPSA-DIS) Grenoble Images Parole Signal Automatique (GIPSA-lab) Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Grenoble Images Parole Signal Automatique (GIPSA-lab) Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Pierre Mendès France - Grenoble 2 (UPMF)-Université Stendhal - Grenoble 3-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS) Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB) Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA) Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS) Department of Physics Oslo Faculty of Mathematics and Natural Sciences Oslo University of Oslo (UiO)-University of Oslo (UiO) Space Research Centre of Polish Academy of Sciences (CBK) Polska Akademia Nauk = Polish Academy of Sciences = Académie polonaise des sciences (PAN) 2013 https://hal.science/hal-02382457 https://hal.science/hal-02382457/document https://hal.science/hal-02382457/file/swsc120007.pdf https://doi.org/10.1051/swsc/2012023 en eng HAL CCSD EDP sciences info:eu-repo/semantics/altIdentifier/doi/10.1051/swsc/2012023 hal-02382457 https://hal.science/hal-02382457 https://hal.science/hal-02382457/document https://hal.science/hal-02382457/file/swsc120007.pdf BIBCODE: 2013JSWSC.3A.01L doi:10.1051/swsc/2012023 http://creativecommons.org/licenses/by/ info:eu-repo/semantics/OpenAccess ISSN: 2115-7251 EISSN: 2115-7251 Journal of Space Weather and Space Climate https://hal.science/hal-02382457 Journal of Space Weather and Space Climate, 2013, 3, pp.A01. ⟨10.1051/swsc/2012023⟩ [SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2013 ftunivparis https://doi.org/10.1051/swsc/2012023 2024-04-23T03:42:26Z International audience The thermospheric atomic oxygen red line is among the brightest in the auroral spectrum. Previous observations in Longyearbyen, Svalbard, indicated that it may be intrinsically polarized, but a possible contamination by light pollution could not be ruled out. During the winter 2010/2011, the polarization of the red line was measured for the first time at the Polish Hornsund polar base without contamination. Two methods of data analysis are presented to compute the degree of linear polarization (DoLP) and angle of linear polarization (AoLP): one is based on averaging and the other one on filtering. Results are compared and are in qualitative agreement. For solar zenith angles (SZA) larger than 108°(with no contribution from Rayleigh scattering), the DoLP ranges between 2 and 7%. The AoLP is more or less aligned with the direction of the magnetic field line, in agreement with the theoretical predictions of Bommier et al. (2010). However, the AoLP values range between ±20°around this direction, depending on the auro-ral conditions. Correlations between the polarization parameters and the red line intensity I were considered. The DoLP decreases when I increases, confirming a trend observed during the observations in Longyearbyen. However, for small values of I, DoLP varies within a large range of values, while for large values of I, DoLP is always small. The AoLP also varies with the red line intensity, slightly rotating around the magnetic field line. Article in Journal/Newspaper Hornsund Longyearbyen Svalbard Université de Paris: Portail HAL Journal of Space Weather and Space Climate 3 A01 |