BaR-SPOrt: The instrument to be accommodated at Dome C
The BaR-SPOrt (Balloon-Borne Radiometers for Sky Polarization Observations) experiment, a program of the Agenzia Spaziale Italiana (ASI) co-funded by PNRA (Progetto Nazionale di Ricerca in Antartide) was originally designed as a payload for long duration balloons flights. The changing scenario, both...
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Format: | Conference Object |
Language: | English |
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E D P SCIENCES
2005
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Online Access: | http://hdl.handle.net/10281/38993 https://doi.org/10.1051/eas:2005040 |
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author | ZANNONI, MARIO BOELLA, GIULIANO FILIPPO SIRONI, GIORGIO GERVASI, MASSIMO Carretti, E Cortiglioni, S Macculi, C Ramponi, M Sbarra, C Ventura, G Monari, J Poloni, M Poppi, S Natale, V Nesti, R Baralis, M Peverini, O Tascone, R Virone, G Boscaleri, A De Bernardis, P Masi, S De Petris, M. |
author2 | Zannoni, M Carretti, E Cortiglioni, S Macculi, C Ramponi, M Sbarra, C Ventura, G Monari, J Poloni, M Poppi, S Natale, V Nesti, R Baralis, M Peverini, O Tascone, R Virone, G Boscaleri, A Boella, G Sironi, G Gervasi, M De Bernardis, P Masi, S De Petris, M |
author_facet | ZANNONI, MARIO BOELLA, GIULIANO FILIPPO SIRONI, GIORGIO GERVASI, MASSIMO Carretti, E Cortiglioni, S Macculi, C Ramponi, M Sbarra, C Ventura, G Monari, J Poloni, M Poppi, S Natale, V Nesti, R Baralis, M Peverini, O Tascone, R Virone, G Boscaleri, A De Bernardis, P Masi, S De Petris, M. |
author_sort | ZANNONI, MARIO |
collection | Università degli Studi di Milano-Bicocca: BOA (Bicocca Open Archive) |
description | The BaR-SPOrt (Balloon-Borne Radiometers for Sky Polarization Observations) experiment, a program of the Agenzia Spaziale Italiana (ASI) co-funded by PNRA (Progetto Nazionale di Ricerca in Antartide) was originally designed as a payload for long duration balloons flights. The changing scenario, both scientific and strategic, has led us to propose it for the starting winter campaign of at the Concordia Base. Here the instrument and the features making it suitable to operate at Dome-C are described. After the initial setup, BaR-SPOrt should not require any kind of routine intervention by a dedicated base staff. The experiment will just need electrical power (less than 2 kW) and a suitable accommodation on the field. It can be fully monitored and controlled, including the data acquisition, through its own telemetry/telecommand link using IRIDIUM modems. Both the receiver and the critical electronics are housed inside a temperature-controlled vacuum chamber, providing the properly stabilized environment. The cold part of the radiometer employs a closed loop mechanical cryo-cooler that provides temperatures < 70 +/- 0.1 K with low power consumption (< 200 W). |
format | Conference Object |
genre | Antartide |
genre_facet | Antartide |
id | ftunivmilanobic:oai:boa.unimib.it:10281/38993 |
institution | Open Polar |
language | English |
op_collection_id | ftunivmilanobic |
op_doi | https://doi.org/10.1051/eas:2005040 |
op_relation | info:eu-repo/semantics/altIdentifier/isbn/2-86883-835-9 info:eu-repo/semantics/altIdentifier/wos/WOS:000231723200039 ispartofseries:EAS PUBLICATIONS SERIES ispartofbook:Dome C: Astronomy and Astrophysics Meeting Dome C Astronomy and Astrophysics Meeting volume:14 firstpage:257 lastpage:262 numberofpages:6 journal:EAS PUBLICATIONS SERIES serie:EAS PUBLICATIONS SERIES http://hdl.handle.net/10281/38993 doi:10.1051/eas:2005040 |
publishDate | 2005 |
publisher | E D P SCIENCES |
record_format | openpolar |
spelling | ftunivmilanobic:oai:boa.unimib.it:10281/38993 2025-05-25T13:45:49+00:00 BaR-SPOrt: The instrument to be accommodated at Dome C ZANNONI, MARIO BOELLA, GIULIANO FILIPPO SIRONI, GIORGIO GERVASI, MASSIMO Carretti, E Cortiglioni, S Macculi, C Ramponi, M Sbarra, C Ventura, G Monari, J Poloni, M Poppi, S Natale, V Nesti, R Baralis, M Peverini, O Tascone, R Virone, G Boscaleri, A De Bernardis, P Masi, S De Petris, M. Zannoni, M Carretti, E Cortiglioni, S Macculi, C Ramponi, M Sbarra, C Ventura, G Monari, J Poloni, M Poppi, S Natale, V Nesti, R Baralis, M Peverini, O Tascone, R Virone, G Boscaleri, A Boella, G Sironi, G Gervasi, M De Bernardis, P Masi, S De Petris, M 2005 STAMPA http://hdl.handle.net/10281/38993 https://doi.org/10.1051/eas:2005040 eng eng E D P SCIENCES place:CEDEX A info:eu-repo/semantics/altIdentifier/isbn/2-86883-835-9 info:eu-repo/semantics/altIdentifier/wos/WOS:000231723200039 ispartofseries:EAS PUBLICATIONS SERIES ispartofbook:Dome C: Astronomy and Astrophysics Meeting Dome C Astronomy and Astrophysics Meeting volume:14 firstpage:257 lastpage:262 numberofpages:6 journal:EAS PUBLICATIONS SERIES serie:EAS PUBLICATIONS SERIES http://hdl.handle.net/10281/38993 doi:10.1051/eas:2005040 CMB Polarimetry Cosmology Instrumentation Settore PHYS-05/A - Astrofisica cosmologia e scienza dello spazio info:eu-repo/semantics/conferenceObject 2005 ftunivmilanobic https://doi.org/10.1051/eas:2005040 2025-04-28T01:57:19Z The BaR-SPOrt (Balloon-Borne Radiometers for Sky Polarization Observations) experiment, a program of the Agenzia Spaziale Italiana (ASI) co-funded by PNRA (Progetto Nazionale di Ricerca in Antartide) was originally designed as a payload for long duration balloons flights. The changing scenario, both scientific and strategic, has led us to propose it for the starting winter campaign of at the Concordia Base. Here the instrument and the features making it suitable to operate at Dome-C are described. After the initial setup, BaR-SPOrt should not require any kind of routine intervention by a dedicated base staff. The experiment will just need electrical power (less than 2 kW) and a suitable accommodation on the field. It can be fully monitored and controlled, including the data acquisition, through its own telemetry/telecommand link using IRIDIUM modems. Both the receiver and the critical electronics are housed inside a temperature-controlled vacuum chamber, providing the properly stabilized environment. The cold part of the radiometer employs a closed loop mechanical cryo-cooler that provides temperatures < 70 +/- 0.1 K with low power consumption (< 200 W). Conference Object Antartide Università degli Studi di Milano-Bicocca: BOA (Bicocca Open Archive) |
spellingShingle | CMB Polarimetry Cosmology Instrumentation Settore PHYS-05/A - Astrofisica cosmologia e scienza dello spazio ZANNONI, MARIO BOELLA, GIULIANO FILIPPO SIRONI, GIORGIO GERVASI, MASSIMO Carretti, E Cortiglioni, S Macculi, C Ramponi, M Sbarra, C Ventura, G Monari, J Poloni, M Poppi, S Natale, V Nesti, R Baralis, M Peverini, O Tascone, R Virone, G Boscaleri, A De Bernardis, P Masi, S De Petris, M. BaR-SPOrt: The instrument to be accommodated at Dome C |
title | BaR-SPOrt: The instrument to be accommodated at Dome C |
title_full | BaR-SPOrt: The instrument to be accommodated at Dome C |
title_fullStr | BaR-SPOrt: The instrument to be accommodated at Dome C |
title_full_unstemmed | BaR-SPOrt: The instrument to be accommodated at Dome C |
title_short | BaR-SPOrt: The instrument to be accommodated at Dome C |
title_sort | bar-sport: the instrument to be accommodated at dome c |
topic | CMB Polarimetry Cosmology Instrumentation Settore PHYS-05/A - Astrofisica cosmologia e scienza dello spazio |
topic_facet | CMB Polarimetry Cosmology Instrumentation Settore PHYS-05/A - Astrofisica cosmologia e scienza dello spazio |
url | http://hdl.handle.net/10281/38993 https://doi.org/10.1051/eas:2005040 |