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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Main Authors: 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.
Other Authors: Zannoni, M, Boella, G, Sironi, G, Gervasi, M, De Petris, M
Format: Conference Object
Language:English
Published: E D P SCIENCES 2005
Subjects:
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