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Remote Sensing ET Algorithm— Remote Evapotranspiration Calculation (RET)
Junming Wang,
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Build the Model ASTER Satellite from NASA
15 by 15 m visible and near-infrared radiance. Bands 1-3 30 by 30 m shortwave infrared radiance. Bands 4-9 90 by 90 m infrared radiance. Bands 10-14 Reflectance(Bands1-9) and temperature data can be requested as secondary processed data Availability: potentially 16 days upon request
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Reflectance (resolution 15 by 15 m)
Build the Model Band 3
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Temperature (resolution 90 by 90 m)
Build the Model
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Build the model Theory ETins = Rn - G - H R H ETins G n
Graph from Allen, et. al., (2002)
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General flowchart Build the Model Start
Satellite inputs: surface temperature and reflectance. Local weather inputs: solar radiation, humidity and wind speed Rn=f(Rs, reflectance) General flowchart NDVI=f(reflectance) G=f(NDVI, solar radiation, reflectance) H=f(NDVI, temperature, reflectance, solar radiation, wind speed) ETins=Rn-H-G Output daily ET End
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Rn Rn=Rns-Rnl = net radiation
Build the Model Rn=Rns-Rnl = net radiation Rns=(1-)Rs = net solar radiation is surface albedo, =0.484 i is the reflectance for ASTER data band I, averaged to 90m2 resolution. Rnl=f(RH,Ts) =net long wave radiation
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Empirical function G=Rn
Empirical function G=Rn*C NDVI from ASTER reflectance data of bands 3 and 2, Build the Model
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Sensible Heat Flux (H) H rah dT H = (r × cp × dT) / rah
Build the Model H = (r × cp × dT) / rah dT = the near surface temperature difference (K). rah = the aerodynamic resistance to heat transport (s/m). H rah z2 rah=ln(z2/z1)/(u*×k) u*= friction velocity dT Cp specific heat of air 75.4 J mol-1 C-1 z1 Graph from Allen, et. al., (2002)
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Selection of “Anchor Pixels” for dT calculation
Build the Model Selection of “Anchor Pixels” for dT calculation “wet” pixel: Ts Tair “dry” pixel: ET 0 Ts=303 K Ts=323 K
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Should be an alfalfa field, not cut and not stressed for water
Build the Model At the “wet” pixel: dTwet = Ts-Tair=0 Should be an alfalfa field, not cut and not stressed for water At the “dry” pixel: Hdry = Rn – G - ETdry where ETdry = 0 dTdry = Hdry× rah / ( × cp) Should be a bare soil field where evaporation is zero.
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dT regression Build the Model
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Sensible Heat Flux (H) Build the Model dT for each pixel is computed using the regression. H is calculated for each pixel after calculating rah for each pixel H = ( × cp × dT) / rah
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Calculate stability parameter for each pixel
Build the Model Start Calculate friction velocity (u*) at weather station and use to get wind speed at 200m Calculate H for each pixel Calculate stability parameter for each pixel Calculate roughness length( zom) for each pixel from NDVI Update H for each pixel based on stability parameter and iterate till change in H less than 10% Calculate friction velocity ( u*) for each pixel Calculate rah for each pixel Calculate Et from energy balance Calculate dT for each pixel from Ts End
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Et Calculation Obtain instant latent heat for each pixel
Build the Model Obtain instant latent heat for each pixel ETins = Rn - G - H Obtain instant reference latent heat for irrigated alfalfa field (ETrins) Obtain Daily reference ET calculated by FAO Penman-Monteith from weather station for alfalfa field (ETrdaily) Calculated ET daily for each pixel ETdaily=ETins/ ETrins×ETrdaily
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Validate the model Measurement sites
Build the Model Validate the model Measurement sites Pecan orchard Alfalfa field
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Validate the Model ET measurement Li Cor system
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ET map Validate the Model mm/day
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The pecan ET of simulation vs. observation.
Validate the Model The pecan ET of simulation vs. observation.
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Sensitivity analysis ET=Rn-G-H Sensitivity Analysis areas
Full vegetation area (6 points, NDVI=0.57) Half vegetation area (6 points, NDVI=0.31) Little vegetation area (6 points, NDVI=0.19)
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Sensitivity analysis Sensitivity Analysis Variables related to Rn Rs ( w/m2), ( ), Variables related to G C (G/Rn, ), Variables related to H rah (0-100 s/m ) Variables were changed over a typical rang for the selected six pixels
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dT regression Build the Model
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ET vs. dT dT is linearly related to Ts, H=f(dT, rah, u*, L, Zom)
Sensitivity analysis dT is linearly related to Ts, H=f(dT, rah, u*, L, Zom) The u* at the full vegetation is bigger than at he half and little vegetation areas, so the ET at the full vegetation area decrease faster than at the other areas.
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ET vs. dT ET is sensitive to dT which is calculated from Ts.
Sensitivity analysis ET vs. dT ET is sensitive to dT which is calculated from Ts. An error in your hot or cold spot dT calculation results in error in H and ET for intermediate points. Ts from satellite is not sensitive as an absolute number only as a relative number which may represent a 2% error in dT and ET If the algorithms in the model are to be changed, the dT calculation equation will be the key equation. It may not be linear
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ET vs. Rs Rns=(1-)Rs, Rn=Rns-Rnl
Sensitivity analysis
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ET vs. Rs ET is sensitive to Rs which determines Rn.
Sensitivity analysis ET vs. Rs ET is sensitive to Rs which determines Rn. Rs is from local weather stations and errors in this value can be as high as 5 to 10 % depending on the quality control for the climate network. An error of 10 % in Rs results in an ET error of 0.2 mm/day or a 3% error in ET
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ET vs. Albedo Rns=(1-)Rs, Rn=Rns-Rnl
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ET vs. Albedo ET is sensitive to albedo because it affects Rn value.
Sensitivity analysis ET vs. Albedo ET is sensitive to albedo because it affects Rn value. The albedo function is an empirical function that may not be applicable over conditions different from the experimental sites where the function was derived. The function is critical when vegetation cover exits and ET is occurring. For bare soil the function is not critical because this condition represents the dry point.
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ET vs. C (G/Rn) C is a polynomial function of NDVI
Sensitivity analysis
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Sensitivity analysis ET vs. C (G/Rn) ET is highly sensitive to C when there is full or half vegetation covered. But ET is not sensitive to C when there is little vegetation covered. If algorithm improvement is needed, the equation for C calculation is a key function.
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ET vs. rah rah=f(u*, z2, z1), H=f(dT, rah, u*, L, Zom)
Sensitivity analysis Z2: above canopy reference height, z1: close to canopy height
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When rah<40s/m, ET is sensitive to it.
Sensitivity analysis ET vs. rah When rah<40s/m, ET is sensitive to it. The rah calculation equation is a key equation for the algorithm and is a function of u* (friction velocity) which is a function of wind speed, roughness length and atmospheric stability which is also related to dT.
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Conclusion Most sensitive variables and equations
Input variables Rs, u from weather station Ts from satellite is not sensitive as an absolute number only as a relative number Intermediate variables (and their calculation equations) dT, albedo, C(G/Rn), and rah
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Thank You!
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