The low frequency instrument of the Planck mission

Details The low frequency instrument of the Planck mission The low frequency instrument of the Planck mission

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..609..144v&link_type=abstract

ASTROPHYSICAL POLARIZED BACKGROUNDS: Workshop on Astrophysical Polarized Backgrounds, held 9-12 October, 2001 in Bologna Italy.

Physics

6

Background Radiations, Radiation Mechanisms, Polarization, Spaceborne And Space Research Instruments, Apparatus, And Components, Radio, Microwave

Scientific paper

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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