BaR-SPOrt: balloon-borne radiometers for sky polarization observations
BaR-SPOrt, funded by ASI (Italian Space Agency), is a 32 (90) GHz balloon-borne correlation polarimeter for direct measurements of the Q and U Stokes parameters, with an angular resolution of 0.6° (0.2°). Aim of the experiment is the detection of the polarized emission of the diffuse Galactic Backgr...
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Online Access: | http://hdl.handle.net/10281/3852 https://doi.org/10.1007/10857580_65 |
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ftunivmilanobic:oai:boa.unimib.it:10281/3852 2024-04-21T07:52:35+00:00 BaR-SPOrt: balloon-borne radiometers for sky polarization observations Sbarra, C Cortiglioni, S Bernardi, G Carretti, E Cecchini, S Macculi, C Ventura, G Baralis, M Peverini, O Tascone, R Tucci, M Natale, V Nesti, R Fabbri, R Monari, J Poppi, S Nicastro, L di Raffaele, R Boscaleri, A Pascale, E de Bernardis, P de Petris, M Masi, S Sazhin, MV Vinyajkin, EN BOELLA, GIULIANO FILIPPO BONOMETTO, SILVIO GERVASI, MASSIMO SIRONI, GIORGIO ZANNONI, MARIO Sbarra, C Cortiglioni, S Bernardi, G Carretti, E Cecchini, S Macculi, C Ventura, G Baralis, M Peverini, O Tascone, R Boella, G Bonometto, S Gervasi, M Sironi, G Tucci, M Zannoni, M Natale, V Nesti, R Fabbri, R Monari, J Poppi, S Nicastro, L di Raffaele, R Boscaleri, A Pascale, E de Bernardis, P de Petris, M Masi, S Sazhin, M Vinyajkin, E 2003 http://hdl.handle.net/10281/3852 https://doi.org/10.1007/10857580_65 eng eng Springer-Verlag country:DE info:eu-repo/semantics/altIdentifier/isbn/3-540-40179-2 info:eu-repo/semantics/altIdentifier/wos/WOS:000185215300065 ispartofseries:ESO ASTROPHYSICS SYMPOSIA ispartofbook:Astronomy, Cosmology and Fundamental Physics: Proceedings of the ESO/CERN/ESA Symposium Held in Garching, Germany, 4-7 March 2002 Symposium on Astronomy, Cosmology and Fundamental Physics 4-7 march volume:2003 firstpage:481 lastpage:482 numberofpages:2 serie:ESO ASTROPHYSICS SYMPOSIA http://hdl.handle.net/10281/3852 doi:10.1007/10857580_65 Astronomy Cosmology Astrophysic Cosmic Microwave Background Polarization FIS/05 - ASTRONOMIA E ASTROFISICA info:eu-repo/semantics/conferenceObject 2003 ftunivmilanobic https://doi.org/10.1007/10857580_65 2024-03-28T01:01:11Z BaR-SPOrt, funded by ASI (Italian Space Agency), is a 32 (90) GHz balloon-borne correlation polarimeter for direct measurements of the Q and U Stokes parameters, with an angular resolution of 0.6° (0.2°). Aim of the experiment is the detection of the polarized emission of the diffuse Galactic Background and the Cosmic Microwave Background (CMB). The most likely launch site is Antarctica (2 to 4-week flight). Kiruna (Sweden, 1-week flight) and Svalbard (Norway, > 1-week flight) are possible launch site to observe the Northern sky Conference Object Antarc* Antarctica Kiruna Svalbard Università degli Studi di Milano-Bicocca: BOA (Bicocca Open Archive) 481 482 |
institution |
Open Polar |
collection |
Università degli Studi di Milano-Bicocca: BOA (Bicocca Open Archive) |
op_collection_id |
ftunivmilanobic |
language |
English |
topic |
Astronomy Cosmology Astrophysic Cosmic Microwave Background Polarization FIS/05 - ASTRONOMIA E ASTROFISICA |
spellingShingle |
Astronomy Cosmology Astrophysic Cosmic Microwave Background Polarization FIS/05 - ASTRONOMIA E ASTROFISICA Sbarra, C Cortiglioni, S Bernardi, G Carretti, E Cecchini, S Macculi, C Ventura, G Baralis, M Peverini, O Tascone, R Tucci, M Natale, V Nesti, R Fabbri, R Monari, J Poppi, S Nicastro, L di Raffaele, R Boscaleri, A Pascale, E de Bernardis, P de Petris, M Masi, S Sazhin, MV Vinyajkin, EN BOELLA, GIULIANO FILIPPO BONOMETTO, SILVIO GERVASI, MASSIMO SIRONI, GIORGIO ZANNONI, MARIO BaR-SPOrt: balloon-borne radiometers for sky polarization observations |
topic_facet |
Astronomy Cosmology Astrophysic Cosmic Microwave Background Polarization FIS/05 - ASTRONOMIA E ASTROFISICA |
description |
BaR-SPOrt, funded by ASI (Italian Space Agency), is a 32 (90) GHz balloon-borne correlation polarimeter for direct measurements of the Q and U Stokes parameters, with an angular resolution of 0.6° (0.2°). Aim of the experiment is the detection of the polarized emission of the diffuse Galactic Background and the Cosmic Microwave Background (CMB). The most likely launch site is Antarctica (2 to 4-week flight). Kiruna (Sweden, 1-week flight) and Svalbard (Norway, > 1-week flight) are possible launch site to observe the Northern sky |
author2 |
Sbarra, C Cortiglioni, S Bernardi, G Carretti, E Cecchini, S Macculi, C Ventura, G Baralis, M Peverini, O Tascone, R Boella, G Bonometto, S Gervasi, M Sironi, G Tucci, M Zannoni, M Natale, V Nesti, R Fabbri, R Monari, J Poppi, S Nicastro, L di Raffaele, R Boscaleri, A Pascale, E de Bernardis, P de Petris, M Masi, S Sazhin, M Vinyajkin, E |
format |
Conference Object |
author |
Sbarra, C Cortiglioni, S Bernardi, G Carretti, E Cecchini, S Macculi, C Ventura, G Baralis, M Peverini, O Tascone, R Tucci, M Natale, V Nesti, R Fabbri, R Monari, J Poppi, S Nicastro, L di Raffaele, R Boscaleri, A Pascale, E de Bernardis, P de Petris, M Masi, S Sazhin, MV Vinyajkin, EN BOELLA, GIULIANO FILIPPO BONOMETTO, SILVIO GERVASI, MASSIMO SIRONI, GIORGIO ZANNONI, MARIO |
author_facet |
Sbarra, C Cortiglioni, S Bernardi, G Carretti, E Cecchini, S Macculi, C Ventura, G Baralis, M Peverini, O Tascone, R Tucci, M Natale, V Nesti, R Fabbri, R Monari, J Poppi, S Nicastro, L di Raffaele, R Boscaleri, A Pascale, E de Bernardis, P de Petris, M Masi, S Sazhin, MV Vinyajkin, EN BOELLA, GIULIANO FILIPPO BONOMETTO, SILVIO GERVASI, MASSIMO SIRONI, GIORGIO ZANNONI, MARIO |
author_sort |
Sbarra, C |
title |
BaR-SPOrt: balloon-borne radiometers for sky polarization observations |
title_short |
BaR-SPOrt: balloon-borne radiometers for sky polarization observations |
title_full |
BaR-SPOrt: balloon-borne radiometers for sky polarization observations |
title_fullStr |
BaR-SPOrt: balloon-borne radiometers for sky polarization observations |
title_full_unstemmed |
BaR-SPOrt: balloon-borne radiometers for sky polarization observations |
title_sort |
bar-sport: balloon-borne radiometers for sky polarization observations |
publisher |
Springer-Verlag |
publishDate |
2003 |
url |
http://hdl.handle.net/10281/3852 https://doi.org/10.1007/10857580_65 |
genre |
Antarc* Antarctica Kiruna Svalbard |
genre_facet |
Antarc* Antarctica Kiruna Svalbard |
op_relation |
info:eu-repo/semantics/altIdentifier/isbn/3-540-40179-2 info:eu-repo/semantics/altIdentifier/wos/WOS:000185215300065 ispartofseries:ESO ASTROPHYSICS SYMPOSIA ispartofbook:Astronomy, Cosmology and Fundamental Physics: Proceedings of the ESO/CERN/ESA Symposium Held in Garching, Germany, 4-7 March 2002 Symposium on Astronomy, Cosmology and Fundamental Physics 4-7 march volume:2003 firstpage:481 lastpage:482 numberofpages:2 serie:ESO ASTROPHYSICS SYMPOSIA http://hdl.handle.net/10281/3852 doi:10.1007/10857580_65 |
op_doi |
https://doi.org/10.1007/10857580_65 |
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