TERENZI, LUCALUCATERENZIMARIS, MicheleMicheleMARISZACCHEI, AndreaAndreaZACCHEIFRANCESCHI, ENRICOENRICOFRANCESCHIPearson, DavidDavidPearsonMORGANTE, GIANLUCAGIANLUCAMORGANTETAVAGNACCO, DanieleDanieleTAVAGNACCOCUTTAIA, FRANCESCOFRANCESCOCUTTAIAGREGORIO, AnnaAnnaGREGORIOMENNELLA, ANIELLOANIELLOMENNELLABATTAGLIA, Paola MariaPaola MariaBATTAGLIABersanelli, MarcoMarcoBersanelliDavis, RichardRichardDavisDE ROSA, Adriano GiuseppeAdriano GiuseppeDE ROSAFRAILIS, MarcoMarcoFRAILISFranceschet, CristianCristianFranceschetGALEOTTA, SamueleSamueleGALEOTTALeonardi, RodrigoRodrigoLeonardiLowe, StuartStuartLoweMandolesi, NAZZARENONAZZARENOMandolesiMeinhold,PeterMeinholdMendes, LuisLuisMendesPoutanen, TorstiTorstiPoutanenSANDRI, MAURAMAURASANDRITomasi, MaurizioMaurizioTomasiVALENZIANO, LucaLucaVALENZIANOVILLA, FabrizioFabrizioVILLAWilkinson,AltheaWilkinsonZonca, AndreaAndreaZonca2023-02-082023-02-082009http://hdl.handle.net/20.500.12386/33271The SCS PID will be used to characterise the radiometers front-end thermal susceptibility (THF). The temperature of the LFI focal plane (FPU) is changed over 4 values, each step having a duration > 3h, depending on the step. The temperature variations are of about 0.3 K each. The measured receivers output will be characterized as a function of FPU temperature variations.ELETTRONICOenResearch reportFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_17 Instrumentation – telescopes, detectors and techniques