Cal & VAL for Greenhouse Gases Observation Spectrometers

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Cal & VAL for Greenhouse Gases Observation Spectrometers Committee on Earth Observation Satellites Cal & VAL for Greenhouse Gases Observation Spectrometers Akihiko KUZE (Earth Observation Research Center Japan Aerospace Exploration Agency CEOS WGCV 43 São José dos Campos, SP, Brazil April 10-13, 2018

GHG Measurements from Space SCIAMACHY (2002 - 2012) GOSAT (2009 - ) OCO-2 (2014-) OCO-3 (2019-) GHGsat (2016-) TanSat (2016-) S5P TROPOMI (2017) FY-3D (2017-) FY-3G (2020-) GOSAT-2 (2018-) MERLIN (2020) GeoCARB MicroCarb (2020) ASCENDS (2021) CarbonSat (2022) 2

Background Both top-down satellite data and bottom-up emission inventories will be crucial to climate policy. The reliability of CHG remote sensing from space has to be demonstrated. Since 2002, GHG monitoring has started with space-borne high spectral resolution spectrometer (SCIAMACHY) and number of projects has rapidly-increased recently. The interpretation of the data from the near-future satellites with unique instrument designs from different space agencies. International Community, Long term and consistent data set. 3

4 Intercomparison between Instruments Challenges Pre-launch <Radiometric Standard: Lamp > Non-linearity correction for FTS High spectral resolution data with different type of spectrometers Radiance Spectra <Instrument: Grating, FTS..> (2) Topography, Observation geometry, aerosol scattering, instrument degradation (3) Validation of partial column density (vertical profile) GHG Column Density Selection spatio-temporal sampling Pattern from limited number of data and spatial resolution Wind speed and direction have large uncertainty Global and Regional Flux <Transport model> 4

5 Present Spectral radiance Intercomparison FTS vs. Grating Spectrometer FTS (GOSAT) vs FTS (S-HIS) Make similar instrument line shape (spectral resolution) by truncating the interferogram before I-FFT FTS (GOSAT) vs Grating (OCO-2) Comparison window channel only. Difficult to compare fine absorption structure. Needs comparison of retrieved parameters 5 Calibrated GOSAT and OCO-2 radiance spectra agrees within 5% for all bands (386 match up data).Katoka et al. (2017 MDPI, Remote Sensing) window channel for comparison

Long Term and Global Intercomparison Topography 2014/09~2016/05 XCO2 Level2 matchup Agreement: (ACOS-GOSAT B7.3 vsOCO-2 B7) < 0.18 ppm over Ocean < 0.57 ppm over Land (high gain) < 0.19 ppm over Land (desert) The time series of ∆ XCO2 from Sep. 2014 Kataoka et al. (2017) 6

Present Vicarious Calibration Almost all the geophysical parameters in radiative transfer have been measured Railroad valley, NV, USA, No topography, BRDF is still challenging item. from West 33.0deg 25deg from East 19deg 19.9deg High altitude TOA Spectral radiance Horizontal CO2  CH4 Vertical CO2  CH4 O3  Surface Thermal radiation Surface and Profile of Pressure, Temperature, Humidity Aerosol Optical Depth Surface CO2 CH4 CO O 3 Wind speed Surface Spectral Reflectance UV-SWIR BRDF  Variability 7 1

Why aerosol and BRDF matter in GHG observations Aerosol Scattering phase function and BRDF One of the largest uncertainty in retrieval Backward scattering is brighter but larger uncertainty. How to express BRDF? Kernel model is good but not perfect. Under estimated GHG Over estimated GHG High altitude thin cloud High altitude dust Multiple Scattering From west backward, from east forward MCD43B1.A2015177.h08v05.005.2015194084624.hdf MODIS band6 (1640 nm) In addition, high resolution spectrometer has generally larger footprint. It is difficult to measure the entire footprint on the ground. BRDF database is needed for vicarious calibration. Bright desert Dark Surface 8

Measured parameters for GHG CAL-VAL To be updated Candidates of CEOS sites for GHG Calibration Dunhuang, Namibia, Libya 9

Validation for background and enhancement for GHG Present: The Total Carbon Column Observing Network (TCCON)(Ground-based large FTS) is well characterized however number of sites is still limited. Recent improvements: portable FTS calibrated with TCCON . Needs for partial column of lower troposphere (LT) Larger enhancement from local emission source Remove influx in upper troposphere Recent algorithms provide partial column of LT Lower troposphere from absorption line shape (Kulawik et al.) Use both TIR and SWIR (Kikuchi et al.) Number of vertical profile data (especially coincident data) was limited. Recent progress: Airplane campaign (NASA ASCENDS/ABoVE, DLR-CNES CoMET etc.) Coutesy of R. Kawa AJAXA vertical profile vs. 4 GOSAT retrieval at RRV, NV 10

Long tem and consistent GHG dataset from different instruments and algorithms Column CO2 Retrieval intercomparison Seamless dataset Buchwitz et al., European Space Agency's (ESA) The Greenhouse Gas Climate Change Initiative (GHG-CCI) Common database for GHG observation instruments from space : Match up database of radiance spectra that include data quality, uncertainty, time, location of each instrument (GOSAT-OCO-2, GOSAT-AIRS, ……) Match-up point check tool http://www.eorc.jaxa.jp/GOSAT/GOSAT_Optimization/index.html 11

Common Standards and Data for Calibrations and Retrieval (updates from WGCV42)   Common standards and data Notes Calibration Prelaunch Cross-calibrated radiometers Viewing common radiometric standard Onboard Solar data Vicarious CEOS site (RRV etc.) Annual campaign Retrieval Algorithm Parameters Molecular spectroscopy A priori model (Aerosol) Input Calibrated spectra at 0.76, 1.6, 2.0μm Observation geometry and condition Level 1 Output Retrieved column amount GHG Simultaneously retrieved parameters (aerosol optical depth, Solar-induced plant chlorophyll fluorescence (SIF)) Level 2 Validation Ground Site High resolution spectrometer mobile spectrometer TCCON, mobile-FTS Vertical profile In situ measured data Airplane, Balloon Match up Land type and Ocean Viewing Common sites

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