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Straylight analysis and minimization strategy in PLANCK low frequency instrument
2005
Optical Design and Engineering II
Planck is the space mission of the European Space Agency devoted to measure of the anisotropies of the cosmic microwave background (CMB), the relic radiation left by the big bang. The satellite will be launched in 2007 and it will carry state-of-the-art of microwave radiometers and bolometers arranged in two instruments, respectively the Low Frequency Instrument and the High Frequency Instrument, both coupled with a 1.5 m telescope and working in nine frequency channels between 30 and 857 GHz.
doi:10.1117/12.625188
fatcat:aqplizotofgdhihej5ya7dvtey