Limits due to instrumental polarisation in CMB experiments at microwave wavelengths (Articolo in rivista)

Type
Label
  • Limits due to instrumental polarisation in CMB experiments at microwave wavelengths (Articolo in rivista) (literal)
Anno
  • 2001-01-01T00:00:00+01:00 (literal)
Alternative label
  • Carretti E., Tascone R., Cortiglioni S., Monari J., Orsini M. (2001)
    Limits due to instrumental polarisation in CMB experiments at microwave wavelengths
    in New astronomy (Gedrukt)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Carretti E., Tascone R., Cortiglioni S., Monari J., Orsini M. (literal)
Pagina inizio
  • 173 (literal)
Pagina fine
  • 187 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 6 (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#descrizioneSinteticaDelProdotto
  • Pubblicazione scientifica referata che descrive la generazione di errori sistematici in strumentazione radio. In particolare si concentra sul segnale polarizzato e riporta come esempi i casi di alcuni strumenti. Ne valuta infine gli impatti della misura della polarizzazione della CMB, argomento di punta della cosmologia attuale. Analisi degli errori strumentali per la misura di polarizzazione della CMB. (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • (1) IASF-CNR Bologna, Via Gobetti 101, 40129, Bologna, Italy (2) IEIIT-CNR Torino, C.so Duca degli Abruzzi 24, 10129, Torino, Italy (3) IRA-CNR Bologna, Via Gobetti 101, 40129, Bologna, Italy (literal)
Titolo
  • Limits due to instrumental polarisation in CMB experiments at microwave wavelengths (literal)
Abstract
  • An extended analysis of some instrumental polarisation sources has been done, as a consequence of the renewed interest in extremely sensitive polarisation measurements stimulated by Cosmic Microwave Background experiments. The case of correlation polarimeters, being them more suitable than other configurations, has been studied in detail and the algorithm has been derived to calculate their intrinsic sensitivity limit due to device characteristics as well as to the operating environment. The atmosphere emission, even though totally unpolarised, has been recognised to be the most important source of sensitivity degradation for ground based experiments. This happens through receiver component losses (mainly in the OMT), which generate instrumental polarisation in genuinely uncorrelated signals. The relevant result is that, also in best conditions (cfr. Antarctica), integration times longer than ~40 s are not allowed on ground without modulation techniques. Finally, basic rules to estimate the maximum modulation period for each instrumental configuration have been provided. (literal)
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