Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
International audience Using data from the Planck satellite, we study the statistical properties of interstellar dust polarization at high Galactic latitudes around the south pole (b < −60°). Our aim is to advance the understanding of the magnetized interstellar medium (ISM), and to provide a mod...
Published in: | Astronomy & Astrophysics |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2016
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Online Access: | http://hal.in2p3.fr/in2p3-01420479 https://doi.org/10.1051/0004-6361/201628636 |
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ftunigrenoble:oai:HAL:in2p3-01420479v1 |
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openpolar |
institution |
Open Polar |
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Université Grenoble Alpes: HAL |
op_collection_id |
ftunigrenoble |
language |
English |
topic |
ISM: magnetic fields magnetohydrodynamics (MHD) polarization methods: data analysis dust extinction cosmic background radiation [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] |
spellingShingle |
ISM: magnetic fields magnetohydrodynamics (MHD) polarization methods: data analysis dust extinction cosmic background radiation [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] Collaboration, PLANCK Aghanim, N. Alves, M. Arzoumanian, D. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A. Barreiro, B. Bartolo, N. Basak, S. Benabed, K. Bernard, P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J. Borrill, J. Bouchet, F. Boulanger, F. Bracco, A. Bucher, M. Burigana, C. Calabrese, E. Cardoso, F. Chiang, C. Colombo, P. Combet, C. Comis, B. Couchot, F. Coulais, A. Crill, P. Curto, A. Cuttaia, F. Davis, J. De Bernardis, P. De Rosa, A. De Zotti, G. Delabrouille, J. Delouis, J. Di Valentino, E. Dickinson, C. Diego, J. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Efstathiou, G. Elsner, F. Enßlin, A. Eriksen, H. Falgarone, E. Fantaye, Y. Ferrière, K. Finelli, F. Frailis, M. Fraisse, A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, T. Gerbino, M. Ghosh, T. González-Nuevo, J. Górski, M. Gratton, Serge Gregorio, A. Gruppuso, A. Gudmundsson, J. Guillet, V. Hansen, F. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A. Jaffe, T. Jones, C. Keihänen, E. Keskitalo, R. Kisner, T. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lagache, Guilaine Lähteenmäki, A. Lamarre, J. Langer, M. Lasenby, A. Lattanzi, M. Le Jeune, M. Levrier, F. Liguori, M. Lilje, P. López-Caniego, M. Lubin, P. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Naselsky, P. Natoli, P. Neveu, J. Nørgaard-Nielsen, H. U. Oppermann, N. Oxborrow, A. Pagano, L. Paoletti, D. Partridge, B. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polenta, G. Rachen, P. Rebolo, R. Reinecke, M. Remazeilles, M. Renzi, A. Ristorcelli, I. Rocha, G. Rossetti, M. Roudier, G. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Soler, J. Suur-Uski, A. Tauber, A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Vansyngel, F. Van Tent, F. Vielva, P. Villa, Francesca Wandelt, B. D. Wehus, I. K. Zacchei, A. Zonca, A. Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap |
topic_facet |
ISM: magnetic fields magnetohydrodynamics (MHD) polarization methods: data analysis dust extinction cosmic background radiation [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] |
description |
International audience Using data from the Planck satellite, we study the statistical properties of interstellar dust polarization at high Galactic latitudes around the south pole (b < −60°). Our aim is to advance the understanding of the magnetized interstellar medium (ISM), and to provide a modelling framework of the polarized dust foreground for use in cosmic microwave background (CMB) component-separation procedures. We examine the Stokes I, Q, and U maps at 353 GHz, and particularly the statistical distribution of the polarization fraction (p) and angle (ψ), in order to characterize the ordered and turbulent components of the Galactic magnetic field (GMF) in the solar neighbourhood. The Q and U maps show patterns at large angular scales, which we relate to the mean orientation of the GMF towards Galactic coordinates (l0,b0) = (70° ± 5°,24° ± 5°). The histogram of the observed p values shows a wide dispersion up to 25%. The histogram of ψ has a standard deviation of 12° about the regular pattern expected from the ordered GMF. We build a phenomenological model that connects the distributions of p and ψ to a statistical description of the turbulent component of the GMF, assuming a uniform effective polarization fraction (p0) of dust emission. To compute the Stokes parameters, we approximate the integration along the line of sight (LOS) as a sum over a set of N independent polarization layers, in each of which the turbulent component of the GMF is obtained from Gaussian realizations of a power-law power spectrum. We are able to reproduce the observed p and ψ distributions using a p0 value of 26%, a ratio of 0.9 between the strengths of the turbulent and mean components of the GMF, and a small value of N. The mean value of p (inferred from the fit of the large-scale patterns in the Stokes maps) is 12 ± 1%. We relate the polarization layers to the density structure and to the correlation length of the GMF along the LOS. We emphasize the simplicity of our model (involving only a few parameters), which can be easily computed on the celestial sphere to produce simulated maps of dust polarization. Our work is an important step towards a model that can be used to assess the accuracy of component-separation methods in present and future CMB experiments designed to search the B mode CMB polarization from primordial gravity waves. |
author2 |
Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes 2016-2019 (UGA 2016-2019 ) Laboratoire de l'Accélérateur Linéaire (LAL) Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11) Laboratoire d'Astrophysique de Marseille (LAM) Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales Toulouse (CNES) PLANCK |
format |
Article in Journal/Newspaper |
author |
Collaboration, PLANCK Aghanim, N. Alves, M. Arzoumanian, D. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A. Barreiro, B. Bartolo, N. Basak, S. Benabed, K. Bernard, P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J. Borrill, J. Bouchet, F. Boulanger, F. Bracco, A. Bucher, M. Burigana, C. Calabrese, E. Cardoso, F. Chiang, C. Colombo, P. Combet, C. Comis, B. Couchot, F. Coulais, A. Crill, P. Curto, A. Cuttaia, F. Davis, J. De Bernardis, P. De Rosa, A. De Zotti, G. Delabrouille, J. Delouis, J. Di Valentino, E. Dickinson, C. Diego, J. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Efstathiou, G. Elsner, F. Enßlin, A. Eriksen, H. Falgarone, E. Fantaye, Y. Ferrière, K. Finelli, F. Frailis, M. Fraisse, A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, T. Gerbino, M. Ghosh, T. González-Nuevo, J. Górski, M. Gratton, Serge Gregorio, A. Gruppuso, A. Gudmundsson, J. Guillet, V. Hansen, F. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A. Jaffe, T. Jones, C. Keihänen, E. Keskitalo, R. Kisner, T. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lagache, Guilaine Lähteenmäki, A. Lamarre, J. Langer, M. Lasenby, A. Lattanzi, M. Le Jeune, M. Levrier, F. Liguori, M. Lilje, P. López-Caniego, M. Lubin, P. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Naselsky, P. Natoli, P. Neveu, J. Nørgaard-Nielsen, H. U. Oppermann, N. Oxborrow, A. Pagano, L. Paoletti, D. Partridge, B. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polenta, G. Rachen, P. Rebolo, R. Reinecke, M. Remazeilles, M. Renzi, A. Ristorcelli, I. Rocha, G. Rossetti, M. Roudier, G. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Soler, J. Suur-Uski, A. Tauber, A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Vansyngel, F. Van Tent, F. Vielva, P. Villa, Francesca Wandelt, B. D. Wehus, I. K. Zacchei, A. Zonca, A. |
author_facet |
Collaboration, PLANCK Aghanim, N. Alves, M. Arzoumanian, D. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A. Barreiro, B. Bartolo, N. Basak, S. Benabed, K. Bernard, P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J. Borrill, J. Bouchet, F. Boulanger, F. Bracco, A. Bucher, M. Burigana, C. Calabrese, E. Cardoso, F. Chiang, C. Colombo, P. Combet, C. Comis, B. Couchot, F. Coulais, A. Crill, P. Curto, A. Cuttaia, F. Davis, J. De Bernardis, P. De Rosa, A. De Zotti, G. Delabrouille, J. Delouis, J. Di Valentino, E. Dickinson, C. Diego, J. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Efstathiou, G. Elsner, F. Enßlin, A. Eriksen, H. Falgarone, E. Fantaye, Y. Ferrière, K. Finelli, F. Frailis, M. Fraisse, A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, T. Gerbino, M. Ghosh, T. González-Nuevo, J. Górski, M. Gratton, Serge Gregorio, A. Gruppuso, A. Gudmundsson, J. Guillet, V. Hansen, F. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A. Jaffe, T. Jones, C. Keihänen, E. Keskitalo, R. Kisner, T. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lagache, Guilaine Lähteenmäki, A. Lamarre, J. Langer, M. Lasenby, A. Lattanzi, M. Le Jeune, M. Levrier, F. Liguori, M. Lilje, P. López-Caniego, M. Lubin, P. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Naselsky, P. Natoli, P. Neveu, J. Nørgaard-Nielsen, H. U. Oppermann, N. Oxborrow, A. Pagano, L. Paoletti, D. Partridge, B. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polenta, G. Rachen, P. Rebolo, R. Reinecke, M. Remazeilles, M. Renzi, A. Ristorcelli, I. Rocha, G. Rossetti, M. Roudier, G. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Soler, J. Suur-Uski, A. Tauber, A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Vansyngel, F. Van Tent, F. Vielva, P. Villa, Francesca Wandelt, B. D. Wehus, I. K. Zacchei, A. Zonca, A. |
author_sort |
Collaboration, PLANCK |
title |
Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap |
title_short |
Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap |
title_full |
Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap |
title_fullStr |
Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap |
title_full_unstemmed |
Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap |
title_sort |
planck intermediate results. xliv. the structure of the galactic magnetic field from dust polarization maps of the southern galactic cap |
publisher |
HAL CCSD |
publishDate |
2016 |
url |
http://hal.in2p3.fr/in2p3-01420479 https://doi.org/10.1051/0004-6361/201628636 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
ISSN: 0004-6361 EISSN: 1432-0756 Astronomy and Astrophysics - A&A http://hal.in2p3.fr/in2p3-01420479 Astronomy and Astrophysics - A&A, EDP Sciences, 2016, 596, pp.A105. ⟨10.1051/0004-6361/201628636⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201628636 info:eu-repo/semantics/altIdentifier/arxiv/1604.01029 in2p3-01420479 http://hal.in2p3.fr/in2p3-01420479 doi:10.1051/0004-6361/201628636 ARXIV: 1604.01029 |
op_doi |
https://doi.org/10.1051/0004-6361/201628636 |
container_title |
Astronomy & Astrophysics |
container_volume |
596 |
container_start_page |
A105 |
_version_ |
1766202993466671104 |
spelling |
ftunigrenoble:oai:HAL:in2p3-01420479v1 2023-05-15T18:23:25+02:00 Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap Collaboration, PLANCK Aghanim, N. Alves, M. Arzoumanian, D. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A. Barreiro, B. Bartolo, N. Basak, S. Benabed, K. Bernard, P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J. Borrill, J. Bouchet, F. Boulanger, F. Bracco, A. Bucher, M. Burigana, C. Calabrese, E. Cardoso, F. Chiang, C. Colombo, P. Combet, C. Comis, B. Couchot, F. Coulais, A. Crill, P. Curto, A. Cuttaia, F. Davis, J. De Bernardis, P. De Rosa, A. De Zotti, G. Delabrouille, J. Delouis, J. Di Valentino, E. Dickinson, C. Diego, J. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Efstathiou, G. Elsner, F. Enßlin, A. Eriksen, H. Falgarone, E. Fantaye, Y. Ferrière, K. Finelli, F. Frailis, M. Fraisse, A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, T. Gerbino, M. Ghosh, T. González-Nuevo, J. Górski, M. Gratton, Serge Gregorio, A. Gruppuso, A. Gudmundsson, J. Guillet, V. Hansen, F. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A. Jaffe, T. Jones, C. Keihänen, E. Keskitalo, R. Kisner, T. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lagache, Guilaine Lähteenmäki, A. Lamarre, J. Langer, M. Lasenby, A. Lattanzi, M. Le Jeune, M. Levrier, F. Liguori, M. Lilje, P. López-Caniego, M. Lubin, P. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Naselsky, P. Natoli, P. Neveu, J. Nørgaard-Nielsen, H. U. Oppermann, N. Oxborrow, A. Pagano, L. Paoletti, D. Partridge, B. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polenta, G. Rachen, P. Rebolo, R. Reinecke, M. Remazeilles, M. Renzi, A. Ristorcelli, I. Rocha, G. Rossetti, M. Roudier, G. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Soler, J. Suur-Uski, A. Tauber, A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Vansyngel, F. Van Tent, F. Vielva, P. Villa, Francesca Wandelt, B. D. Wehus, I. K. Zacchei, A. Zonca, A. Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes 2016-2019 (UGA 2016-2019 ) Laboratoire de l'Accélérateur Linéaire (LAL) Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11) Laboratoire d'Astrophysique de Marseille (LAM) Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales Toulouse (CNES) PLANCK 2016-04-04 http://hal.in2p3.fr/in2p3-01420479 https://doi.org/10.1051/0004-6361/201628636 en eng HAL CCSD EDP Sciences info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201628636 info:eu-repo/semantics/altIdentifier/arxiv/1604.01029 in2p3-01420479 http://hal.in2p3.fr/in2p3-01420479 doi:10.1051/0004-6361/201628636 ARXIV: 1604.01029 ISSN: 0004-6361 EISSN: 1432-0756 Astronomy and Astrophysics - A&A http://hal.in2p3.fr/in2p3-01420479 Astronomy and Astrophysics - A&A, EDP Sciences, 2016, 596, pp.A105. ⟨10.1051/0004-6361/201628636⟩ ISM: magnetic fields magnetohydrodynamics (MHD) polarization methods: data analysis dust extinction cosmic background radiation [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] info:eu-repo/semantics/article Journal articles 2016 ftunigrenoble https://doi.org/10.1051/0004-6361/201628636 2022-02-08T23:36:42Z International audience Using data from the Planck satellite, we study the statistical properties of interstellar dust polarization at high Galactic latitudes around the south pole (b < −60°). Our aim is to advance the understanding of the magnetized interstellar medium (ISM), and to provide a modelling framework of the polarized dust foreground for use in cosmic microwave background (CMB) component-separation procedures. We examine the Stokes I, Q, and U maps at 353 GHz, and particularly the statistical distribution of the polarization fraction (p) and angle (ψ), in order to characterize the ordered and turbulent components of the Galactic magnetic field (GMF) in the solar neighbourhood. The Q and U maps show patterns at large angular scales, which we relate to the mean orientation of the GMF towards Galactic coordinates (l0,b0) = (70° ± 5°,24° ± 5°). The histogram of the observed p values shows a wide dispersion up to 25%. The histogram of ψ has a standard deviation of 12° about the regular pattern expected from the ordered GMF. We build a phenomenological model that connects the distributions of p and ψ to a statistical description of the turbulent component of the GMF, assuming a uniform effective polarization fraction (p0) of dust emission. To compute the Stokes parameters, we approximate the integration along the line of sight (LOS) as a sum over a set of N independent polarization layers, in each of which the turbulent component of the GMF is obtained from Gaussian realizations of a power-law power spectrum. We are able to reproduce the observed p and ψ distributions using a p0 value of 26%, a ratio of 0.9 between the strengths of the turbulent and mean components of the GMF, and a small value of N. The mean value of p (inferred from the fit of the large-scale patterns in the Stokes maps) is 12 ± 1%. We relate the polarization layers to the density structure and to the correlation length of the GMF along the LOS. We emphasize the simplicity of our model (involving only a few parameters), which can be easily computed on the celestial sphere to produce simulated maps of dust polarization. Our work is an important step towards a model that can be used to assess the accuracy of component-separation methods in present and future CMB experiments designed to search the B mode CMB polarization from primordial gravity waves. Article in Journal/Newspaper South pole Université Grenoble Alpes: HAL South Pole Astronomy & Astrophysics 596 A105 |