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Validating Satellite Land Surface Temperature Products for GOES-R and JPSS Missions
Yunyue Yu, Mitchell Goldberg, Ivan Csiszar NOAA/NESDIS Center for Satellite Applications and Research Presentation for IGARSS 2011
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Motivation -- LST validation needs
LST Products Derived from Different Sensors for Decades POES NOAA AVHRR (TIROS-N to NOAA-19) since 1978 ESA ATSR/AATSR since 1991 EOS MODIS since 1999 MetOp AVHRR since 2006 GOES US GOES/Imagers since 1975 Meteosat (MVIRI since 1995 and then) SEVIRI since 2004 Future LST products JPSS/NPP GOES-R LST Climate Data Record Just listed major LST sources, not include microwave sensors, LEO sensors. GOES generation: SMS – GOES 1 (1975) to 3 1st - GOES 4 to 7 2nd – GOES 8 to 12 3rd – GOES 13 to 15 4th – GOES R, S, T, U
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Motivation -- LST validation issues
LST Validation Difficulties In situ data limitation Measurement difficulty Cloud contamination effect particularly the partial or thin cloudy pixels Spatial and temporal variations Spot vs pixel difference Sub-pixel heterogeneity Accurate match-up process (different sampling rates and sampling timing) Others i.e. angle effect In situ data limitation Different spatial scales Different sampling rates and sample timing Sub-pixel cloud contamination Sub-pixel heterogeneity Limited samples of clear case Surface heterogeneity is shown in a 4km x 4km Google map (1km x 1km, in the center box) around the Bondville station area
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Approach -- Strategy Using Existing Ground Observation Data
Cost consideration Site representativeness and selection: characterization analysis Match-up Dataset Generation Stringent cloud filtering: additional measures Data pair quality control Site-to-pixel Model Development Synthetic pixel analysis using high resolution sensor data Proxy data testing Real satellite data evaluation Validation Methodology Direct comparisons Indirection comparisons
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Approach Synthetic pixel analysis using ASTER data— an integrated approach for site representativeness analysis and site-to-pixel model development Quantitatively characterize the sub-pixel heterogeneity and decide whether a ground site is adequately representative for the satellite pixel. The sub-pixels may be generated from pixels of a higher-resolution satellite. For pixel that is relatively homogeneous, analyze statistical relationship of the ground-site sub-pixel with the surrounding sub-pixels: {T(x,y) } ~ T(x0,y0) Establish relationship between the objective pixel and its sub-pixels (i.e., up-scaling model), e.g., Tpixel = T(x,y) + DT (time dependent?) T(x,y,t) T(x0,y0,t0) ASTER pixel The site pixel MODIS pixel Issues: 1) different t and t0 resulting different Ts. 2) the ground homogeneity maybe location/time dependent 3) the up-scaling model 4) the uncertainty of up-scaling estimation Solutions: 1) develop or use proper random statistic model for heterogeneity and interpolation analysis 2) develop or use proper up-scaling model to perform point-to-area estimation The Synthetic pixel/sub-pixel model
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Approach A Site Characterization Simulation Model – synthesizing VIIRS pixel using higher-resolution ASTER TIR pixels. ASTER scene (90m) pixel Each synthetic pixel has the target ground site enclosed, but the distance between the ground site and the center of synthetic pixel varies, which mimics the possible over-passing VIIRS swaths. Distance of every synthetic pixel center from the ground site is within the pixel size (~1Km). Different colors are used for the 9 synthetic pixels, and the center of each pixel is marked with a small numbered square of the same corresponding color. The numbers on the squares are the pixel IDs used in the relevant analysis. Colored squares: Ground site synthetic VIIRS pixels
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Approach Quantification of the difference between the Synthetic Pixel and Ground Measurement, that is, Evaluation: and with the model: Note that: Why Tc – Tg is systematic error? Sub-pixel heterogeneity Systematic bias between ASTER and ground measurements Tsat – satellite pixel LST Tg -- ground site LST Tc central sub-pixel LST
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Data Sets Data Acquisition
Inventory preparation of clear-sky ASTER scenes passing over 23 ground sites (SURFRAD and CRN) during Collection of the clear-sky ASTER data sets associated with six SURFRAD sites and two CRN sites. AST_04, AST_05, AST_08 and L1B (in total, about 2000 ASTER swath scenes). Collection of the six SURFRAD and the two CRN ground data. Collection of the two CRN ground data. Collection of MODIS LST product data (MOD11_L2). All the swaths passing over the SURFRAD sites in 2001 All the swaths corresponding to the ASTER scenes during Collection of the narrow-band emissivity data sets UW-Madison Baseline Fit Emissivity Database North American ASTER Land Surface Emissivity Database (NAALSED) Collection of NCEP reanalysis TPW datasets
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Clear Cases (additional cloud filter)
Data Sets Candidate Ground Sites and Database Dataset Used SURFRAD data ASTER Data Data period: ASTER data is courtesy by Shunlin Liang Satellite LST: MODIS LST, ASTER, and GOES LST Ground LST: Derived from SURFRAD site measurements Table: Matched ASTER Data Stations Clear Cases (ASTER cloud mask) Clear Cases (additional cloud filter) Desert Rock 63 46 Bondville, IL 115 51 PennState, PA 61 20 Boulder, CO 35 13 Fort Peck, MT 12 8 Should use my one (CRN sites are not used in the table, therefore not need to be shown)
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Data Sets Ground Site Broadband Emissivity
Regression based on the UW-Madison Baseline Fit Emissivity Database ( Seemann et al., 2008). Ground Site Broadband Emissivity Regression of Broadband emissivity from well-developed narrowband emissivity database: UW-Madison baseline Fit Emissivity Database a=0.2122, b=0.3859,c= (Wang, 2004) Jul. 2011
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Processing General Components of Validation Processing Ground Data
Satellite Data Match-up Datasets Time Match-up Geolocation Match-up Ground Data Mask Satellite Cloud Mask Manual Cloud Control Ground LST Estimation/Extraction Satellite LST Calculation/Extraction Synthetic Analysis and Correction Ground Data Ground Data Reader Satellite Data Reader Indirect Comparison Direct Comparison Statistical Analysis Outputs (Plots, Tables, etc.)
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Upwelling, Downwelling
Processing Sample Match-up Flow Chart Geolocation Match-up SURFRAD Data Satellite Time (< 5 mins) Time Series Smoothness Check (if available): Upwelling, Downwelling Irradiances Spatial Difference Test: BT -- 3X3 pix STDs, Visual deg Channel BT (Ts, T10mm), (T10mm, T3.9mm) (T10mm, T12mm) Matched Dataset Manual Tuning Cloud Mask Additional cloud filter Note: this flow chart is specifically for GOES Imager Similar procedure is/will be applied for the ASTER and MODIS/VIIRS data
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Processing Data Processing/Analysis Clear-sky cases analysis
Cloud and clear-sky climatology analysis (for site selection) ASTER Clear-sky swath selection from the ASTER inventory from the Warehouse Inventory Search Tool Ground broadband emissivity regression analysis SURFRAD LST estimation from PIR measurements Spatial and temporal match-up among ground sites, ASTER scenes and MODIS scenes Geolocation mapping of ASTER pixels as the sub-pixels of a MODIS pixel Quality-control and enhanced cloud filtering Processing of ASTER LST QC information Processing of ASTER emissivity QC information Processing MODIS cloud masks Processing of MODIS LST QC information Surface observations Statistical testing
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Processing Data Processing/Analysis (con’t)
Site representativeness analysis and site-to-pixel difference characterization Semi-variance analysis Synthetic analysis Site-to-pixel model testing Testing with all the MODIS Terra LST swaths passing over SUFRAD sites in 2001 Testing with the MODIS LST swaths corresponding with ASTER scenes during VIIRS LST case studies on NPP land LPEATE platform Development of VIIRS LST algorithm modules for flexible offline testing and algorithm improvement Visualization tools of the analysis and results disolay
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Results Additional cloud filtering is need for obtaining high quality satellite-ground match-up dataset Left: ATSER cloud free dataset. Right: possible cloud contamination. Cloud
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Results Comparison of the temperatures calculated from synthetic pixel average (top-right), center-pixel (bottom-left), and nearest pixel (bottom-right) with the ground site temperature. Note the different colors represent for the 9 different synthetic pixels shown previously. For this particular site the ground site location within the satellite pixel does not have significance impact to the validation process, simply because the land surface thermal emission at Desert Rock is fairly homogeneous. SURFRAD Station: Desert Rock
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Results Sample statistical analysis result on the Desert Rock site.
0.61 0.08 2.20 -1.74 2 -1.81 Mean Ts - Tc 0.76 -0.07 2.21 -1.88 Average 0.60 -0.16 2.37 -1.97 8 0.65 -0.26 2.40 -2.07 7 0.80 -0.34 2.30 -2.15 6 0.98 -0.24 2.18 -2.05 5 0.96 0.06 2.03 -1.75 4 0.92 0.20 1.99 -1.61 3 -0.01 2.26 -1.82 1 2.46 0.69 0.04 2.13 -1,78 STD STD` Tc-Ta Ts – Ta Case Site=Desert Rock, NV Impact of pixel location bias to the ground site The Ta and Ts difference is tested by comparing its spatial structure to the site geographic structure. It shows that such Ta and Ts difference matches the site geographic feature well, which implies that the synthetic pixel temperature calculation is reasonable. Ts: LST of SURFRAD site Ta: average LST over 13x13 ASTER pixels Tc: LST of ASTER pixel nearest to the site
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Results Sample statistical analysis result on the Bondville site.
1.07 -0.05 2.05 -0.64 2 -0.59 Mean Ts - Tc 1.05 -0.09 2.08 -0.80 Average 0.97 -0.18 2.02 -0.77 8 0.95 -0.03 7 -0.001 2.12 -0.62 6 1.10 2.14 -0.60 5 1.15 2.10 -0.68 4 1.27 2.17 3 1.04 -0.14 2.01 -0.73 1 0.92 -0.07 2.04 -0.66 STD STD` Tc-Ta Ts – Ta Case Site=Bondville, IL Impact of pixel location bias to the ground site Jul. 2011
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Results Sample statistical analysis result on the Boulder site.
Site=Boulder, CO 0.91 -0.27 2.30 -1.03 2 -0.77 Mean Ts - Tc 0.72 -0.13 2.58 -0.90 Average 0.70 -0.25 2.70 -1.02 8 -0.10 2.80 -0.87 7 0.69 -0.00 2.75 6 0.61 2.64 -0.67 5 -0.03 2.54 -0.80 4 0.84 -0.14 2.27 -0.91 3 0.85 -0.38 2.61 -1.15 1 2.60 0.58 -0.07 2.62 -0.84 STD STD` Tc-Ta Ts – Ta Case Impact of pixel location bias to the ground site Jul. 2011
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Results Sample scatter plots show the linear relationship between satellite LST and ground LST. Tsat = A Tg + B + e
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Results 11/11/2018 Site-to-Pixel Statistical Relationship Site C σ
Desert Rock, NV 1.88 2.21 Boulder, CO 0.90 2.58 FortPeck, MT -0.15 2.62 Bondville,IL 0.68 2.08 PennState, PA -0.17 1.99 WolfPoint 34, MT 1.47 1.98 WolfPoint 29, MT 0.64 3.86 Oakley, KS 0.24 1.03 Mercury, NV 3.99 1.25 Site A B σ Desert Rock, NV 1.115 -33.66 1.73 Boulder, CO 1.138 -38.76 1.32 FortPeck, MT 1.089 -25.51 2.02 Bondville, IL 1.014 -3.29 2.01 PennState, PA 1.002 -0.66 1.97 WolfPoint 34, MT 0.768 65.99 WolfPoint 29, MT 0.593 114.48 3.23 Oakley, KS 1.374 1.33 Mercury, NV 1.044 -9.77 1.14 11/11/2018
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Results Site-to-Pixel Statistical Relationship – MODIS Proxy Site MODIS Pixel- SURFRAD Synthetic Pixel- SURFRAD Nearest Aster Pixel – Synthetic pixel Match-Up Pairs (SURFRAD, ASTER, MODIS) Mean StdDev Desert Rock, NV -0.44 1.84 2.09 1.69 0.04 0.44 34 Boulder,CO -0.49 2.08 1.49 2.90 -0.09 0.67 7 Fort Peck, MT 0.35 2.52 0.78 1.95 0.38 1.15 4 Bondville, IL -0.17 1.51 1.04 1.48 0.03 0.90 26 Penn State, PA -1.53 1.91 0.61 1.96 1.07 The standard deviation of the difference between real MODIS pixel LST and SURFRAD LST are consistent with the standard deviation of the difference between synthetic pixel and SURFRAD. The synthetic pixel LST is generally much warmer (about 1.5K) than SURFRAD LST, while MODIS LST is slightly cooler than SURFRAD LST. Implication: High resolution ASTER data be used for site representativeness analysis, but a further verification of ASTER LST quality seems essential for the parameter estimation of the site-to-pixel model (e.g., A,B,C) and the application of the model in real cases.
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Results –Summary Synthetic pixel analysis model is created for analyzing ground site temperature heterogeneous feature. ASTER data are used to generate synthetic VIIRS pixel data (LST) and compared to the SURFRAD site data LST of SURFRAD measurements may be used as good references for VIIRS/ABI LST cal/val if the measurements are of high-quality and the in-situ estimation of LST is accurate enough. Directional variations are small, so small geo-referencing (within 1Km) bias may not be an issue affecting VIIRS/ABI LST cal/val at the above SURFRAD sites. Application of the site-to-pixel model depends on the ASTER LST data quality. Directional variation of the potential sub-pixel heterogeneity is found to be consistent with the physical topographic features, even if it is small. The limited datasets doesn’t allow us to characterize the seasonal variation of heterogeneities, which is more desirable than a simple mean difference. More datasets are expected. And about 1K difference seems unavoidable in practice.
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Future Plan Analysis over time scales of interest, e.g., seasonal variation. Analysis over sites of different surface types Up/down-scaling models Emissivity uncertainties Test of the scaling model using real satellite data
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