Stratospheric balloon experiments play a unique role in current Cosmic Microwave Background (CMB) studies. CMB research has entered a precision phase, harvesting the detailed properties of its anisotropy, polarization and spectrum, at incredible precision levels. These measurements, however, require careful monitoring and subtraction of local backgrounds, produced by the earth atmosphere and the interstellar medium. High frequencies (larger than 180 GHz) are crucial for the measurements of interstellar dust contamination, but are degraded by atmospheric emission and its fluctuations, even in the best (cold and dry) sites on earth. For this reason, new balloon-borne missions, exploiting long-duration and ultra-long duration stratospheric flights, are being developed in several laboratories worldwide. These experiments have the double purpose of qualifying instrumentation and validating methods to be used on satellite missions, and produce CMB science at a relatively fast pace, synergically to ground-based CMB observatories.

Balloon-borne Cosmic Microwave Background experiments / Masi, Silvia; Coppolecchia, A.; Battistelli, E.; de Bernardis, P.; Columbro, F.; D’Alessandro, G.; Lamagna, L.; Paiella, A.; Piacentini, F.; Presta, G.. - 209:(2019). (Intervento presentato al convegno RICAP18, 7th Roma International Conference on Astroparticle Physics tenutosi a Rome; Italy) [10.1051/epjconf/201920901046].

Balloon-borne Cosmic Microwave Background experiments

Silvia Masi;A. Coppolecchia;E. Battistelli;P. de Bernardis;F. Columbro;G. D’Alessandro;L. Lamagna;A. Paiella;F. Piacentini;G. Presta
2019

Abstract

Stratospheric balloon experiments play a unique role in current Cosmic Microwave Background (CMB) studies. CMB research has entered a precision phase, harvesting the detailed properties of its anisotropy, polarization and spectrum, at incredible precision levels. These measurements, however, require careful monitoring and subtraction of local backgrounds, produced by the earth atmosphere and the interstellar medium. High frequencies (larger than 180 GHz) are crucial for the measurements of interstellar dust contamination, but are degraded by atmospheric emission and its fluctuations, even in the best (cold and dry) sites on earth. For this reason, new balloon-borne missions, exploiting long-duration and ultra-long duration stratospheric flights, are being developed in several laboratories worldwide. These experiments have the double purpose of qualifying instrumentation and validating methods to be used on satellite missions, and produce CMB science at a relatively fast pace, synergically to ground-based CMB observatories.
2019
RICAP18, 7th Roma International Conference on Astroparticle Physics
balloon; cosmology; CMB
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Balloon-borne Cosmic Microwave Background experiments / Masi, Silvia; Coppolecchia, A.; Battistelli, E.; de Bernardis, P.; Columbro, F.; D’Alessandro, G.; Lamagna, L.; Paiella, A.; Piacentini, F.; Presta, G.. - 209:(2019). (Intervento presentato al convegno RICAP18, 7th Roma International Conference on Astroparticle Physics tenutosi a Rome; Italy) [10.1051/epjconf/201920901046].
File allegati a questo prodotto
File Dimensione Formato  
Masi_Balloon-borne_2019.pdf

accesso aperto

Tipologia: Versione editoriale (versione pubblicata con il layout dell'editore)
Licenza: Creative commons
Dimensione 1.94 MB
Formato Adobe PDF
1.94 MB Adobe PDF

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1344649
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? 7
social impact