The Low Frequency Instrument (LFI) is one of the two instruments onboard the ESA Planck satellite. LFI will image the Cosmic Microwave Background anisotropies and the polarization status in four different bands, from 30 GHz to 100 GHz, with an array of 54 radiometers. The characteristics of the instrument are reported, underlining the ability of LFI to perform polarization measurements.
The low frequency instrument of the Planck mission / F. Villa, N. Mandolesi, M. Bersanelli, R. C. Butler, C. Burigana, A. Mennella, G. Morgante, M. Sandri, L. Valenziano - In: Astrophysical polarized backgrounds : workshop on astrophysical polarized backgrounds, Bologna, Italy 9-12 october 2001 / [a cura di] S. Cortiglioni, S. Cecchini, R. Sault, C. Sbarra. - Melville : American institute of physics, 2002. - ISBN 0-7354-0055-5. - pp. 144-149 (( convegno Workshop on astrophysical polarized backgrounds tenutosi a Bologna nel 2001 [10.1063/1.1471837].
The low frequency instrument of the Planck mission
F. VillaPrimo
;M. Bersanelli;A. Mennella;
2002
Abstract
The Low Frequency Instrument (LFI) is one of the two instruments onboard the ESA Planck satellite. LFI will image the Cosmic Microwave Background anisotropies and the polarization status in four different bands, from 30 GHz to 100 GHz, with an array of 54 radiometers. The characteristics of the instrument are reported, underlining the ability of LFI to perform polarization measurements.
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