In this paper we discuss the linearity response of the Planck-LFI receivers, with particular reference to signal compression measured on the 30 and 44 GHz channels. In the article we discuss the various sources of compression and present a model that accurately describes data measured during tests performed with individual radiomeric chains. After discussing test results we present the best parameter set representing the receiver response and discuss the impact of non linearity on in-flight calibration, which is shown to be negligible.

The linearity response of the Planck-LFI flight model receivers / A. Mennella, F. Villa, L. Terenzi, F. Cuttaia, P. Battaglia, M. Bersanelli, R. C. Butler, O. D’Arcangelo, E. Artal, R. Davis, M. Frailis, C. Franceschet, S. Galeotta, A. Gregorio, N. Hughes, P. Jukkala, D. Kettle, V. H. Kilpiä, M. Laaninen, P. M. Lapolla, R. Leonardi, P. Leutenegger, S. Lowe, N. Mandolesi, M. Maris, P. Meinhold, L. Mendes, M. Miccolis, G. Morgante, N. Roddis, M. Sandri, R. Silvestri, L. Stringhetti, M. Tomasi, J. Tuovinen, L. Valenziano, A. Zacchei, J. Varis, A.Wilkinson, A. Zonca. - In: JOURNAL OF INSTRUMENTATION. - ISSN 1748-0221. - 4:[12](2009 Dec), pp. T12011.T12011.1-T12011.T12011.20.

The linearity response of the Planck-LFI flight model receivers

A. Mennella
Primo
;
M. Bersanelli;C. Franceschet;M. Tomasi;A. Zonca
Ultimo
2009

Abstract

In this paper we discuss the linearity response of the Planck-LFI receivers, with particular reference to signal compression measured on the 30 and 44 GHz channels. In the article we discuss the various sources of compression and present a model that accurately describes data measured during tests performed with individual radiomeric chains. After discussing test results we present the best parameter set representing the receiver response and discuss the impact of non linearity on in-flight calibration, which is shown to be negligible.
Instruments for CMB observations; Microwave radiometers; Space instrumentation; Systematic effects
Settore FIS/05 - Astronomia e Astrofisica
Settore FIS/01 - Fisica Sperimentale
dic-2009
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/150621
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