1、Lunar observation plan based on SI-traceable demonstration instrument development,Feng JiangShanghai Institute of Technical Physics , Chinese Academy of Science,2017 Joint GSICS/IVOS Lunar Calibration Workshop,2017 Joint GSICS/IVOS Lunar Calibration Workshop,1.Lunar observation plan introduction,2.S
2、ensor calibration overview,3.Error budget analysis,4.On orbit calibration,Orbit parameters,Sun,Moon,Spectrometer,+Z,+X,+Y,0,-30,-60,-90,30,60,90,XOY plane,Cryogenic Absolute Radiometer,Key Laboratory of Optics Calibration and Characterization， Chinese Academy of Science,Spectral range: 0.2550m Absol
3、ute accuracy: 0.02%Power resolution: 0.01nW,Trap Detector,Spectral reponsivity,spatial non-uniformity,polarization sensitivity,linearity,instability,repeatability,laser power measurement,Standard detector,Absolue spectral response uncertainty of standard detector 632.8nm,Standard radiometer,Standard
4、 radiometer,Standard radiometer,Spectrometer calibration uncertainty,-Uncertainty of the standard radiometer-Stability and spatial uniformity of the light source-Wavelength calibration-Polarization sensitivity-Stray light-Detector linearity-Point spread function and line spread function-Thermal,Pre-
5、flight calibration,Spectrometer,Standard radiometer,Integrating Sphere,Tunable Laser,Polarization sensitivity,zigzag blazed grating,Depolarizer,Error Budget,Cryogenic Absolute radiometerUncertainty 0.02%,Si trap detector Uncertainty 0.15%,Standard Radiometer Uncertainty 0.5%,激光均匀光源 稳定性（Laser illuminated integrating sphere source）,Spectrometer (VISNIR)Uncertainty 1.24%,On orbit calibration,On orbit calibration,On orbit calibration,On orbit,Ground,attenuator,(Neutral density filter),Thank you !,
