We describe a simple but effective iterative procedure specifically designed to destripe Q and U Stokes parameter data as those collected by the SPOrt experiment onboard the International Space Station (ISS). The method is general enough to be useful for other experiments, both in polarization and total intensity. The only requirement for the algorithm to work properly is that the receiver knee frequency must be lower than the signal modulation frequency, corresponding in our case to the ISS orbit period. Detailed performances of the technique are presented in the context of the SPOrt experiment, both in terms of added rms noise and residual correlated noise

Sbarra, C., Carretti, E., Cortiglioni, S., Zannoni, M., Fabbri, R., Macculi, C., et al. (2003). An iterative destriping technique for diffuse background polarization data. ASTRONOMY & ASTROPHYSICS, 401(3), 1215-1222 [10.1051/0004-6361:20030200].

An iterative destriping technique for diffuse background polarization data

ZANNONI, MARIO;
2003

Abstract

We describe a simple but effective iterative procedure specifically designed to destripe Q and U Stokes parameter data as those collected by the SPOrt experiment onboard the International Space Station (ISS). The method is general enough to be useful for other experiments, both in polarization and total intensity. The only requirement for the algorithm to work properly is that the receiver knee frequency must be lower than the signal modulation frequency, corresponding in our case to the ISS orbit period. Detailed performances of the technique are presented in the context of the SPOrt experiment, both in terms of added rms noise and residual correlated noise
Articolo in rivista - Articolo scientifico
cosmic microwave background, polarization, cosmology: observations, methods: data analysis, methods: numerical
English
2003
401
3
1215
1222
none
Sbarra, C., Carretti, E., Cortiglioni, S., Zannoni, M., Fabbri, R., Macculi, C., et al. (2003). An iterative destriping technique for diffuse background polarization data. ASTRONOMY & ASTROPHYSICS, 401(3), 1215-1222 [10.1051/0004-6361:20030200].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/3781
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