modeling land surface fluxes and...
TRANSCRIPT
MODELING LAND SURFACE FLUXES AND MICROWAVE SIGNATURES OFGROWING VEGETATION
By
JOAQUIN J. CASANOVA
A THESIS PRESENTED TO THE GRADUATE SCHOOLOF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT
OF THE REQUIREMENTS FOR THE DEGREE OFMASTER OF ENGINEERING
UNIVERSITY OF FLORIDA
2007
1
ACKNOWLEDGMENTS
This research was supported by the NSF Earth Science Directorate (EAR-0337277)
and the NASA New Investigator Program (NASA-NIP-00050655). I would like to thank
Mr. Orlando Lanni and Mr. Larry Miller for providing engineering support during the
MicroWEXs and patiently tolerating my idiocy; Mr. Jim Boyer and his team at PSREU
for land and crop management; Dr. Roger De Roo at the University of Michigan for
radiometers and tech support; Mr. Kai-Jen Tien, Mr. Tzu-Yun Lin, Ms. Mi-Young Jang,
and Mr. Fei Yan for their help in data collection during the MicroWEXs; and to the
University of Florida High-Performance Computing Center for providing computational
resources and support that have contributed to the research results reported within this
thesis.
4
TABLE OF CONTENTS
page
ACKNOWLEDGMENTS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4
LIST OF TABLES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
LIST OF FIGURES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
ABSTRACT . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
CHAPTER
1 INTRODUCTION . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
1.1 Thesis Objectives . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 171.2 Thesis Format . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
2 MICROWAVE WATER AND ENERGY BALANCE EXPERIMENTS . . . . . 18
3 CALIBRATION OF A CROP GROWTH MODEL FOR SWEET CORN . . . . 25
3.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 253.2 CERES-Maize Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 253.3 Model Calibration . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27
3.3.1 Initialization . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 273.3.2 Inputs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 283.3.3 Methodology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28
3.4 Results and Discussion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 293.4.1 Crop Growth and Development . . . . . . . . . . . . . . . . . . . . 293.4.2 Evapotranspiration . . . . . . . . . . . . . . . . . . . . . . . . . . . 323.4.3 Soil Moisture and Temperature . . . . . . . . . . . . . . . . . . . . 34
3.5 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37
4 CALIBRATION OF AN SVAT MODEL AND COUPLING WITH A CROPMODEL FOR SWEET CORN . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
4.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 394.2 LSP Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
4.2.1 Energy and Moisture Transport at the Land Surface . . . . . . . . . 404.2.1.1 Energy Balance . . . . . . . . . . . . . . . . . . . . . . . . 404.2.1.2 Moisture Balance . . . . . . . . . . . . . . . . . . . . . . . 45
4.2.2 Soil Processes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 464.3 Coupling of LSP and DSSAT models . . . . . . . . . . . . . . . . . . . . . 474.4 Methodology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
4.4.1 Inputs and Initial Conditions . . . . . . . . . . . . . . . . . . . . . . 484.4.2 Calibration . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
4.5 Results and Discussion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51
5
4.5.1 Calibration . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 514.5.1.1 DSSAT . . . . . . . . . . . . . . . . . . . . . . . . . . . . 514.5.1.2 LSP . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51
4.5.2 Model Simulation . . . . . . . . . . . . . . . . . . . . . . . . . . . . 524.5.2.1 DSSAT . . . . . . . . . . . . . . . . . . . . . . . . . . . . 524.5.2.2 LSP-DSSAT Model . . . . . . . . . . . . . . . . . . . . . . 53
4.6 Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
5 CANOPY MICROWAVE MODEL . . . . . . . . . . . . . . . . . . . . . . . . . 82
5.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 825.2 Methodology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
5.2.1 Moisture Distribution Measurements . . . . . . . . . . . . . . . . . 825.2.2 Canopy Opacity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 835.2.3 Microwave Brightness Model . . . . . . . . . . . . . . . . . . . . . . 855.2.4 Model Comparison and Evaluation . . . . . . . . . . . . . . . . . . 87
5.3 Results and Discussion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 885.3.1 Moisture Distribution Function . . . . . . . . . . . . . . . . . . . . 885.3.2 Canopy Opacity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 895.3.3 Microwave Brightness . . . . . . . . . . . . . . . . . . . . . . . . . . 90
5.4 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94
6 CONCLUSION . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 96
6.1 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 966.2 Contributions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 976.3 Recommendations for Future Research . . . . . . . . . . . . . . . . . . . . 97
REFERENCES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99
BIOGRAPHICAL SKETCH . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105
6
LIST OF TABLES
Table page
3-1 Cultivar coefficient values in the calibrated CERES-Maize model. . . . . . . . . 29
3-2 Error statistics for crop growth and ET between CERES-Maize estimates andMicroWEX-2 field observations. . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
3-3 model performance statistics for soil moisture and temperature between CERES-Maizeestimates and MicroWEX-2 field observations. . . . . . . . . . . . . . . . . . . . 37
4-1 Values for soil properties in the LSP model. . . . . . . . . . . . . . . . . . . . . 49
4-2 Sampling ranges from [24] and calibrated values for parameters in the LSP model. 50
4-3 Comparison of LAI, dry biomass (kg/m2), and ET (mm) for stand-alone DSSATand coupled LSP-DSSAT simulations. . . . . . . . . . . . . . . . . . . . . . . . . 53
4-4 Comparison of surface fluxes (W/m2), for stand-alone LSP and coupled LSP-DSSATsimulations. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55
4-5 Comparison of volumetric soil moisture (m3/m3), for stand-alone LSP and coupledLSP-DSSAT simulations. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55
4-6 Comparison of soil temperature (K), for stand-alone LSP and coupled LSP-DSSATsimulations. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55
4-7 Measurement uncertaintities during MicroWEX-2. . . . . . . . . . . . . . . . . . 56
5-1 Values of the Coefficients in equations 5–6 and 5–7 . . . . . . . . . . . . . . . . 88
5-2 RMS differences between observed TB during MicroWEX-5 and those estimatedby the MB model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91
5-3 RMS differences between observed H-pol TB during MicroWEX-2 and those estimatedby the MB model. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94
7
LIST OF FIGURES
Figure page
1-1 Outline of the data assimilation scheme and the forward model. . . . . . . . . . 15
1-2 Contributions to microwave brightness TB from sky, soil, and canopy. . . . . . . 15
2-1 The University of Florida C-band Microwave Radiometer. . . . . . . . . . . . . 19
2-2 The University of Florida L-band Microwave Radiometer. . . . . . . . . . . . . . 19
2-3 The Eddy Covariance System. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20
2-4 The net radiometer used during the MicroWEXs. . . . . . . . . . . . . . . . . . 20
2-5 Map of the field site during MicroWEX-2. . . . . . . . . . . . . . . . . . . . . . 22
2-6 Map of the field site during MicroWEX-4. . . . . . . . . . . . . . . . . . . . . . 23
2-7 Map of the field site during MicroWEX-5. . . . . . . . . . . . . . . . . . . . . . 24
3-1 (a) Comparison of the CERES-Maize estimates and the observations of biomassduring MicroWEX-2, (b) scatter plot of estimated and observed biomass, (c)comparison of the CERES-Maize estimates and the observations of LAI duringMicroWEX-2, and (d) scatter plot of estimated and observed LAI. . . . . . . . . 31
3-2 Comparison of the latent heat flux estimates from CERES-Maize model usingfour methods with the observations during MicroWEX-2 by (a) daily heat fluxand (b) cumulative ET. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 33
3-3 Comparison of the CERES-Maize soil moisture estimates with MicroWEX-2observations at depths of (a) 0-5 cm, (b) 5-15 cm, (c) 15-30 cm, (d) 30-45 cm,(e) 45-60 cm, and (f) 60-90 cm. . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
3-4 Comparison of the CERES-Maize soil temperature estimates with MicroWEX-2observations at depths of (a) 0-5 cm, (b) 5-15 cm, (c) 15-30 cm, (d) 30-45 cm,(e) 45-60 cm, and (f) 60-90 cm. . . . . . . . . . . . . . . . . . . . . . . . . . . . 36
4-1 Surface resistance network to estimate sensible and latent heat fluxes in the LSPmodel. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
4-2 Algorithm for the coupling of the LSP and DSSAT models. . . . . . . . . . . . . 47
4-3 Pareto fronts from calibration of the stand-alone LSP model. The asterisk representsthe point on the Pareto front where the total seasonal RMSD for 2 cm VSM is0.04 m3/m3. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51
4-4 Comparison of estimations by the coupled LSP-DSSAT and stand-alone DSSATmodel simulation and those observed during MicroWEX-2: (a) dry biomass, (b)LAI, (c) 5 cm soil moisture, and (d) ET. . . . . . . . . . . . . . . . . . . . . . . 54
8
4-5 Comparison of net radiation, between DoY 78 to 105, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 56
4-6 Comparison of latent heat flux, between DoY 78 to 105, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 57
4-7 Comparison of sensible heat flux, between DoY 78 to 105, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 58
4-8 Comparison of soil heat flux, between DoY 78 to 105, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 59
4-9 Comparison of volumetric soil moisture estimated by the coupled LSP-DSSATand stand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 78 to 105: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60
4-10 Comparison of soil temperature estimated by the coupled LSP-DSSAT and stand-aloneLSP model simulation and those observed during MicroWEX-2, between DoY78 to 105: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and (f) 100 cm. . 61
4-11 Comparison of net radiation, between DoY 105 to 125, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 62
4-12 Comparison of latent heat flux, between DoY 105 to 125, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 63
4-13 Comparison of sensible heat flux, between DoY 105 to 125, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and those observedduring MicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . 64
4-14 Comparison of soil heat flux, between DoY 105 to 125, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 65
4-15 Comparison of volumetric soil moisture estimated by the coupled LSP-DSSATand stand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 105 to 125: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66
9
4-16 Comparison of soil temperature estimated by the coupled LSP-DSSAT and stand-aloneLSP model simulation and those observed during MicroWEX-2, between DoY105 to 125: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and (f) 100 cm. 67
4-17 Comparison of net radiation, between DoY 125 to 135, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 68
4-18 Comparison of latent heat flux, between DoY 125 to 135, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 69
4-19 Comparison of sensible heat flux, between DoY 125 to 135, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and those observedduring MicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . 70
4-20 Comparison of soil heat flux, between DoY 125 to 135, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 71
4-21 Comparison of volumetric soil moisture estimated by the coupled LSP-DSSATand stand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 125 to 135: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
4-22 Comparison of soil temperature estimated by the coupled LSP-DSSAT and stand-aloneLSP model simulation and those observed during MicroWEX-2, between DoY125 to 135: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and (f) 100 cm. 73
4-23 Comparison of net radiation, between DoY 135 to 154, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 74
4-24 Comparison of soil heat flux, between DoY 135 to 154, estimated by the coupledLSP-DSSAT and stand-alone DSSAT model simulation and those observed duringMicroWEX-2: (a) values and (b) residuals . . . . . . . . . . . . . . . . . . . . . 75
4-25 Comparison of volumetric soil moisture estimated by the coupled LSP-DSSATand stand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 135 to 154: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
4-26 Comparison of soil temperature estimated by the coupled LSP-DSSAT and stand-aloneLSP model simulation and those observed during MicroWEX-2, between DoY135 to 154: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and (f) 100 cm. 77
10
4-27 Comparison of fluxes estimated by the coupled LSP-DSSAT and stand-aloneLSP model simulation and those observed during MicroWEX-2: (a) net radiation,(b) latent heat flux, (c) sensible heat flux, and 2 cm soil heat flux. . . . . . . . . 78
4-28 Comparison of volumetric soil moisture estimated by the coupled LSP-DSSATand stand-alone LSP model simulation and those observed during MicroWEX-2:(a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and (f) 100 cm. . . . . . . . 79
4-29 Comparison of soil temperature estimated by the coupled LSP-DSSAT and stand-aloneLSP model simulation and those observed during MicroWEX-2: (a) 2 cm, (b) 4cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and (f) 100 cm. . . . . . . . . . . . . . . . . 80
5-1 Observations of total and ear wet biomass during (a) MicroWEX-4 in 2005 and(b) MicroWEX-5 in 2006. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83
5-2 Observations of canopy height during (a) MicroWEX-4 in 2005 and (b) MicroWEX-5in 2006. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84
5-3 Cloud densities measured during (a) MicroWEX-4 in 2005 and (b) MicroWEX-5in 2006. The symbols and the lines represent the measurements and the bestcurve-fits, respectively. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 85
5-4 Moisture mixing ratios measured during (a) MicroWEX-4 in 2005 and (b) MicroWEX-5in 2006. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 86
5-5 Comparison of τ calculated using the biophysical τ model (with and withoutthe gaussian term) and that using the Jackson model during (a) MicroWEX-4in 2005, and (b) MicroWEX-5 and 2006. . . . . . . . . . . . . . . . . . . . . . . 89
5-6 Comparison of the observed TB at H-pol during MW5 those simulated by theMB model using τ from the biophysical model and from the Jackson model duringlate-season MicroWEX-5. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90
5-7 Comparison of microwave brightness, estimated by the LSP-DSSAT-MB modelwith specular surface (a) and Wegmuller and Matzler (b), and C-band microwavebrightness observed during MicroWEX-2, before DoY 125. . . . . . . . . . . . . 92
5-8 Comparison of microwave brightness, estimated by the LSP-DSSAT-MB modelwith specular surface (a) and Wegmuller and Matzler (b), and C-band microwavebrightness observed during MicroWEX-2, after DoY 125. . . . . . . . . . . . . . 93
11
Abstract of Thesis Presented to the Graduate Schoolof the University of Florida in Partial Fulfillment of theRequirements for the Degree of Master of Engineering
MODELING LAND SURFACE FLUXES AND MICROWAVE SIGNATURES OFGROWING VEGETATION
By
Joaquin J. Casanova
December 2007
Chair: Jasmeet JudgeMajor: Agricultural and Biological Engineering
Soil moisture in the root zone is an important component of the global water and
energy balance, governing moisture and heat fluxes at the land surface and at the
vadose-saturated zone interface. Typically, soil moisture estimates are obtained using
Soil-Vegetation-Atmosphere Transfer (SVAT) models. However, two main challenges
remain in SVAT modeling. First, most models often oversimplify the coupling between
vegetation growth and surface fluxes, and second, model errors accumulate due to
uncertainty in parameters and forcings, and numerical computation. The ultimate goal
of this research is to improve estimates of root-zone soil moisture and ET by linking an
SVAT model with a crop growth model, and assimilating remotely-sensed observations
sensitive to soil moisture, such as microwave brightness (MB). Toward that goal, a coupled
SVAT-Crop model will be developed, calibrated, and linked to an MB model, to comprise
the forward model for data assimilation. The models will use observations from three
season-long field experiments monitoring growing sweet corn.
12
CHAPTER 1INTRODUCTION
Soil moisture in the root zone is an important component of the global water and
energy balance, governing moisture and heat fluxes at the land surface and at the
vadose-saturated zone interface. Typically, soil moisture estimates are obtained using
Soil-Vegetation-Atmosphere Transfer (SVAT) models. SVAT models simulate energy
and moisture transport in soil and vegetation and estimate the fluxes at the land surface
and in the root zone. Some widely-used SVAT models include the Common Land Model
(CLM) [10], the model developed by the National Centers for Environmental Prediction at
Oregon State University, Air Force, and Hydrologic Research Laboratory at the National
Weather Service (NOAH) [46], and the University of Michigan Microwave Geophysics
Group Land Surface Process (LSP) model [38]. However, two main challenges remain in
modeling energy and moisture fluxes using SVAT models.
First, most models often oversimplify the coupling between vegetation growth and
surface fluxes. The interactions between vegetation and the fluxes become increasingly
important as these fluxes affect plant growth and development. Vegetation canopies
impact latent and sensible heat fluxes, precipitation interception, and radiative transfer
at the land-atmosphere interface, affecting soil moisture and temperature profiles in the
vadose zone. These changing interactions during the growing season need to be included
in the SVAT models, in order to provide realistic estimates of the fluxes. Typically, SVAT
models employ observations or empirical functions for vegetation conditions to model
the effects of growing vegetation. For example, CLM uses vegetated grid spaces defined
by patches of “plant functional types,” with parameters for physiological and structural
properties associated with each type, and most of the vegetation parameters are empirical
to meet computational constraints [10]. NOAH simulates soil moisture and temperature
profiles with a sub-daily timestep, and with vegetation properties such as LAI, stomatal
resistance, and roughness length defined by vegetation type classes [46]. Such methods
13
ignore the interaction between surface fluxes and vegetation growth. Second, SVAT model
estimates of fluxes, soil moisture, and soil temperature diverge from observations due to
uncertainty in parameters, forcings, and initial conditions, and due to accumulated errors
from numerical computation.
SVAT models can be coupled with crop growth models to include dynamic interactions
between the vegetation growth and flux estimates. For example, [23] used a sub-daily
biochemical vegetation model with a land surface hydrology model. They modeled
canopy transpiration and its influence on soil moisture and carbon fluxes. [41] linked
daily process-based crop models for summer maize and winter wheat with an hourly
land surface flux model and a three-layer soil moisture model. Such coupling allows for
inclusion of vegetation effects without in situ observations or empirical growth functions.
Periodic in situ observations of vegetation could be incorporated in the coupled models to
reduce the divergence of model prediction from reality.
Remotely-sensed observations sensitive to soil moisture, such as low frequency (< 10
GHz) microwave brightness (TB) [15, 26, 43, 52] could also be incorporated periodically
to improve model flux estimates. To incorporate or assimilate microwave brightness,
the coupled SVAT-crop model has to be linked to a microwave emission model that
estimates microwave brightness using moisture and temperature profiles in soil and
vegetation estimated by the SVAT-Crop model as shown in Figure 1-1. Simple versions of
SVAT models linked with MB models include the Land Surface Process/Radiobrightness
(LSP/R) [30] and Simple Soil-Plant-Atmosphere Transfer - Remote Sensing (SiSPAT-RS)
[12] models.
The total TB of a terrain is dependent on sky TB, reflected by the soil (TB,sky),
thermal emission from the soil (TB,soil, and thermal emission from the vegetation canopy
(TB,canopy, all three components are shown in Figure 1-2). Since soil microwave emissions
(dependent on soil moisture and temperature profiles) are attenuated by transmission
14
Figure 1-1. Outline of the data assimilation scheme and the forward model.
Figure 1-2. Contributions to microwave brightness TB from sky, soil, and canopy.
15
through the canopy, a microwave transmission model for growing vegetation is an
important component of the MB model.
Microwave emission models for dynamic vegetation during the growing season require
accurate estimation of canopy emission and attenuation. Non-scattering attenuation is
described by canopy optical depth (τ) that primarily depends upon the distribution of
moisture in the canopy. Several methods have been investigated for determining canopy
optical depth. For example, Ulaby and Wilson[58] modeled τ of the wheat canopy as
a uniform cloud of wet biomass with leaves and stems treated separately. In addition,
polarization dependence was included for stem attenuation. Eom [21] developed a model
for τ applicable to row structured canopies such wheat or corn. The model accounts for
azimuthal anisotropy in τ by modeling the canopy as a random collection of dielectric
spheroids. This method matched well with observations but requires a computationally
intensive solution of the radiative transfer equation. Jackson and Schmugge [51], used
the results of many studies and developed an empirical model for τ . In their model, τ is
estimated as the product of a frequency-dependent constant b and water column density
(kg/m2) in the canopy. The Jackson model is flexible but has little physical basis, with
b often used as a fitting parameter in emission models or estimated empirically [61].
England and Galantowicz [19] developed a refractive model for estimating optical depth of
grass based upon vertical profiles of moisture content within the grass canopy.
In this thesis, an SVAT model, viz. the LSP model, is coupled with a widely-used and
well-tested crop growth model, the Decision Support System for Agrotechnology Transfer
Cropping System Model (DSSAT-CSM) [29]. The models are calibrated using obserations
from the Microwave Water and Energy Balance Experiment 2 (MicroWEX-2), one of three
season-long experiments monitoring growing sweet corn (MicroWEXs 2, 4, and 5). A
biophysically-based canopy transmission model is developed for growing sweet corn, using
data from MicroWEXs 4 and 5. This τ model is included in a simple MB model that is
linked with the LSP-DSSAT model.
16
1.1 Thesis Objectives
This thesis answers the following research questions:
1. What values for the six corn cultivar coefficients give the best DSSAT model
performance for both biomass and LAI for the MicroWEX-2 growing season?
(Chapter 3)
2. How do the model estimates for biomass and LAI compare with MicroWEX-2
observations? (Chapter 3)
3. What values of the twelve calibrated parameters give the best LSP model performance
for both latent heat flux and near surface soil moisture for the MicroWEX-2 growing
season? (Chapter 4)
4. How do the model estimates of soil moisture, temperature, and surface fluxes
compare with MicroWEX-2 observations? (Chapter 4)
5. What is the impact of coupling on both LSP and DSSAT model estimates of LAI,
biomass, soil moisture, temperature, and surface fluxes? (Chapter 4)
6. How does a physically-based τ model compare to Jackson’s widely-used empirical
model? (Chapter 5)
7. How do the brightness estimates predicted by the linked LSP-DSSAT-MB model
compare to observations during MicroWEX-2? (Chapter 5)
1.2 Thesis Format
The Chapter 2 of this thesis describes the field experiments, MicroWEXs 2, 4, and
5. In Chapter 3, the DSSAT model’s corn submodel, CERES-Maize, is calibrated for the
MicroWEX-2 growing season. In Chapter 4, the LSP model is calibrated and coupled
with DSSAT model. In Chapter 5, a canopy transmission model for growing sweet corn is
developed and tested in a simpled MB model, linked with the LSP-DSSAT model.
17
CHAPTER 2MICROWAVE WATER AND ENERGY BALANCE EXPERIMENTS
The MicroWEXs are a series of experiments conducted by the Center for Remote
Sensing at the University of Florida during growing seasons of corn and cotton [6, 8, 33,
37, 55, 67]. The objective of the experiments are to understand microwave signatures of
agricultural crops during different stages of growth. MicroWEX-2 was conducted during
the sweet corn growing season, from March 18 through June 2 in 2004 [33]. MicroWEX-4
was conducted during the sweet corn growing season, from March 10 through June 2 in
2005 [6]. MicroWEX-5 was conducted during the subsequent corn season from March 9
through May 26 in 2006 [8]. All experiments were conducted at the same 37,000 m2 site
in UF/IFAS Plant Science Research and Education Unit in Citra, FL (29.41 N, 82.18
W). The soils at the site are Lake Fine Sand with about 90 % sand and a bulk density of
1.55 g/cm3. Row spacing was 76 cm, with approximately eight plants per square meter.
Irrigation and fertigation were conducted via a linear move system.
Data collected during the MicroWEXs included soil moisture, temperature and
heat flux, latent and sensible heat flux, wind speed and direction, upwelling and
downwelling short and longwave radiation, precipitation, irrigation, water table depth,
and vertically and horizontally polarized microwave brightness at 6.7 GHz (λ = 4.47 cm),
every fifteen minutes using the tower-mounted University of Florida C-band Microwave
Radiometer (UFCMR, Figure 2-1). Additional horizontally polarized microwave brightness
observations at 1.4 GHz (λ = 21.4 cm) were conducted during MicroWEX-5 using the
UF L-Band Microwave Radiometer (UFLMR, Figure 2-2). The radiometer frequencies, at
6.7 GHz and at 1.4 GHz, correspond to the lowest frequency of the Advanced Scanning
Microwave Radiometer (AMSR-E) [22], and the frequency of the planned Soil Moisture
and Ocean Salinity (SMOS) mission [34], respectively.
The soil moisture, heat fluxes, and temperatures were observed at three locations
in the field. Soil moisture and soil temperature were observed at 2, 4, 8, 16, 32, 64,
18
Figure 2-1. The University of Florida C-band Microwave Radiometer.
Figure 2-2. The University of Florida L-band Microwave Radiometer.
19
Figure 2-3. The Eddy Covariance System.
Figure 2-4. The net radiometer used during the MicroWEXs.
and 120 cm (100 cm during MicroWEX-2) using Campbell Scientific Water Content
Reflectometers and Vitel Hydra- probes; and thermistors and thermocouples, respectively.
An Eddy Covariance System (Figure 2-3) measured wind speed, direction, and latent and
sensible heat fluxes. REBS CNR net radiometer (Figure 2-4)measured up- and down-
welling short- and long- wave radiation. Everest Interscience infrared sensor measured
thermal infrared temperature. Four tipping-bucket rain gauges logged precipitation at
four locations East and West of the footprint, and at the East and West sides of the field.
Water table depth was measured using Solinst Level Loggers in a monitoring well in each
quadrant.
In addition to continuously logged data, there were also weekly vegetation and
twice-weekly soil samplings (during MicroWEX-2 only). Vegetation sampling was
conducted in four areas, one in each quadrant of the field. Samples were selected by
placing a meter stick half-way between two plants and ending the sample at least 1 m
from the starting point and half-way between two plants. The actual row length of the
sample was noted. Stand density, leaf number, canopy height and width, wet and dry
20
weights of leaves, stems, and ears were measured. Two LAI measurements were taken
in each sampling area using the Licor LAI-2000 Canopy Analyzer. Vertical distribution
of moisture in the canopy was measured five times during MicroWEX-4 and three times
during MicroWEX-5 [7]. During soil sampling, soil moisture and temperatures were
observed in-row and in-furrow at depths of 2, 4, and 8 cm along eight transects at ten
to thirteen locations, using the Delta-T ThetaProbe soil moisture sensor and a digital
thermometer to quantify the spatial variability of the field. Vegetation and soil nitrogen
(as NH+4 and NO−
3 ) were measured in each of the four sampling areas. Root length density
was measured in the vadose zone at tasseling.
21
CHAPTER 3CALIBRATION OF A CROP GROWTH MODEL FOR SWEET CORN
3.1 Introduction
This chapter describes the calibration of a crop growth model for a growing season
of sweet corn in north-central Florida. There are two major corn growth models, EPIC
(Erosion Productivity Impact Calculator) [65] and CERES-Maize [28], that simulate
hydrology, nutrient cycling, growth, and development. CERES-Maize has the advantage
of being part of the well-known Decision Support System for Agrotechnology Transfer
Cropping System Model (DSSAT-CSM). DSSAT has been widely used for a number of
years, with validated models for over 15 crops. It also allows for simulations of multi-year
crop rotations [29].
3.2 CERES-Maize Model
The CERES-Maize model is a part of the crop growth submodule in DSSAT-CSM.
DSSAT-CSM is a modular crop simulation model with modules for soil, soil-plant-atmosphere,
crop development and growth, weather, management, etc. A simulation consists of several
stages: season and run initialization, rate calculation, integration, and output generation
[29]. The model determines total dry biomass using the radiation use efficiency method.
Total solar radiation is partitioned into photosynthetically active radiation (PAR), and
the fraction intercepted is calculated from LAI using Beer’s law [54]. The dry matter
accumulation rate is a product of radiation use efficiency and a conversion factor. Maize
growth and development is marked by eight events: germination, emergence, end of
juvenile phase, floral induction (tassel initiation), 75% silking, beginning grain fill,
maturity, and harvest. Transition from one developmental stage to the next is determined
by the growing degree days (GDD) with a base temperature of 8C. Vegetative growth
stops on 75% silking, when reproductive growth begins in the form of grain fill. Yield is
the grain fill value at harvest. Threshold GDD for each stage and grain fill parameters are
contained in a cultivar file.
25
The CERES-Maize model determines LAI by tracking the total number of leaves and
calculating a leaf area growth rate, so that the rate of increase of LAI is the product of
leaf area growth and current leaf number. Leaf growth is partly determined by the number
of degree days between successive leaf tip appearances, called the phyllochron interval. In
addition, a leaf senescence rate is calculated based on water stress.
The soil-plant-atmosphere module estimates ET at the land surface using either
the Ritchie-modified Priestley-Taylor (RPT) method [48] or the Penman-FAO (PFAO)
method [14]. The RPT method depends only on solar radiation and temperature, while
the PFAO method accounts for wind speed and relative humidity as well. Both methods
first determine a total potential ET, which is partitioned into potential soil evaporation
and potential plant transpiration. Potential soil evaporation is based on intercepted solar
radiation reaching the soil surface as a function of temperature, wind speed, radiation,
and humidity. Potential plant transpiration depends on the radiation intercepted by the
canopy and temperature, wind speed, and humidity. Actual evaporation and transpiration
are determined by the minimum of potential ET and the amount of available water. For
soil evaporation, surface soil water is the limiting factor, while for transpiration, root water
uptake is the limiting factor.
The soil is divided into nine layers, each with different constitutive properties.
Soil moisture is calculated using the bucket method [39]. When an upper soil layer is
above the drained upper limit, excess flows to the one below, in addition to computing
estimates for capillary rise. Runoff is calculated using the USDA Soil Conservation Service
runoff number method [53]. Infiltration is equal to excess precipitation after runoff. Soil
temperature is computed using a deep soil boundary condition and an air temperature
boundary condition. The air temperature (C) is calculated from the average of maximum
and minimum daily temperatures. Soil temperature (ST ) varies with soil layer (L) as [29]:
ST (L) = TAV G + (TAMP
2.0COS(ALX + ZD) +DT )eZD (3–1)
26
where DT is the difference between the average of the daily average temperatures
during the previous five days and the yearly average (C), ZD is depth (cm), TAMP is
amplitude of yearly temperature (C), and ALX is the difference in days from the current
day to the hottest day of the year.
3.3 Model Calibration
The CERES-Maize model was ported to the Linux OS and calibrated using data from
MicroWEX-2. This section describes the calibration procedure.
3.3.1 Initialization
CERES is the crop submodule for cereal crops, including maize. CERES-Maize uses
three files for determining growth and development characteristics: the species file, the
ecotype file, and the cultivar file. The species file contains defining characteristics of
corn, including root growth parameters, seed initial conditions, nitrogen and water stress
response coefficients, nitrogen uptake parameters, base and optimum temperatures for
grain fill and photosynthesis, and radiation and CO2 parameters governing photosynthesis.
The ecotype file specifies thermal time development, radiation use efficiency, and light
extinction coefficients for three main types of corn. The cultivar file specifies the cultivar
coefficients that describe the growth and development characteristics for different maize
cultivars. These are:
P1: degree days between emergence and end of juvenile stage.
P2: development delay for each hour increase in photoperiod past optimum
photoperiod.
P5: degree days from silking to maturity.
G2: maximum possible number of kernels per plant.
G3: kernel filling rate during the linear grain filling stage and under optimum
conditions (mg/day).
PHINT: phyllochron interval, i.e., the interval in thermal time (degree days) between
leaf tip appearances.
27
Soil properties such as hydraulic conductivity and texture were taken as the default
values for the soil type that most closely corresponds with our field site (Millhopper fine
sand) and that is included in the DSSAT soil properties file. The drained lower limit
of the top nine soil layers was set to the minimum soil moisture (0.05) observed during
MicroWEX-2. The initial soil moisture for all the layers was set equal to 0.2. The model
calibration was found to be insensitive to the choice of initial moisture conditions because
an irrigation event that occurred at planting reset the soil moisture profile of sandy soil.
3.3.2 Inputs
Most of the inputs for the model calibration were obtained from the MicroWEX-2
dataset. These included daily incoming solar radiation, precipitation, irrigation,
fertigation, and wind speed. Maximum and minimum daily temperature and relative
humidity were obtained from the micrometeorological dataset collected for the Agricultural
Field-Scale Irrigation Requirement Simulation (AFSIRS) study at a nearby site at the
PSREU [16].
3.3.3 Methodology
To calibrate the CERES-Maize model, a broad grid search was employed, followed by
simulated annealing in the area of the global minimum using the six cultivar coefficients.
Each coefficient was incrementally changed, so that a grid of possible combinations of
values was tested to minimize the differences between model estimates and observations
from biomass and LAI, the two most important canopy parameters required by the MB
model. The LAI observation on DoY 135 was excluded for calibration, due to its high
standard deviation (Figure 3-1a). The objective function (R) was computed as the sum of
square residuals, normalized by variance [54]:
R =SSRB
σ2B
+SSRLAI
σ2LAI
(3–2)
where SSRB is the sum of square residuals from total biomass, SSRLAI is the sum
of square residuals from LAI, and σ2B and σ2
LAI are the variances of biomass and LAI
28
Table 3-1. Cultivar coefficient values in the calibrated CERES-Maize model.
Cultivar Coefficient ValueP1 157.20P2 1.000P5 811.20G1 853.00G3 10.4PHINT 40.33
observations, respectively. The optimum combination of parameter values found by the
grid search was then used as the initial guess in a simulated annealing optimization
algorithm [2]. The root mean square difference (RMSD), relative root mean square
difference (RRMSD), and Willmott d -index [66] were calculated as for LAI and the
biomass of each component, leaves, stems, and grain:
RMSD = (Σ(Pi −Oi)
2
n)1/2 (3–3)
RRMSD =RMSD
O(3–4)
d = 1− Σ(Pi −Oi)2
Σ(|Pi − P |+ |Oi − O|)2(3–5)
where n is the number of observations, Pi and Oi are the predicted and observed
values, and P and O are the predicted and observed means. Table 3-1 shows the values of
the six cultivar coefficients that minimized R in Equation 3–2.
3.4 Results and Discussion
3.4.1 Crop Growth and Development
To evaluate the CERES-Maize model for crop growth and development, model
estimates are compared of emergence and silking dates, biomass, and LAI to the
observations during MicroWEX-2.
29
The modeled and observed emergence dates were on DoY 90 and DoY 86, respectively.
Modeled anthesis day (when 75% of the corn has silked) was DoY 139, while 75% silking
was observed by DoY 135. The model estimated realistic total dry biomass using the
parameters determined by the grid search, as shown in Figure 3-1. The RMSD for
biomass was 0.90 Mg/ha with a low RRMSD of 0.23 and a correspondingly high Willmott
d -index of 0.99, as shown in Table 3-2. Figure 3-1b shows a scatter plot of estimated
and observed total biomass. The biomass was increasingly underestimated by the model
as the season progressed, with the maximum difference of 1.41 Mg/ha at the end of the
season. The partitioning of the modeled biomass into leaf and stem biomass did not match
the observations (Figure 3-1a), as indicated by the high RMSD and RRMSD in Table
3-2. Partitioning of total biomass into stem biomass was underestimated by the model
during later vegetative stages of growth (DoY 127 to DoY 134). The partitioning into
leaf biomass was more realistic, with a slight overestimation during later growth stages
(DoY 132 to DoY 142). The model’s estimate of the beginning of grain fill at DoY 140
matched closely with the observed grain fill at DoY 139 (Figure 3-1a). The best fit for
LAI and total biomass did not produce the best fit for grain fill. In order to compensate
for the underestimated stem biomass, grain weight must be overestimated. The model
estimated realistic LAI, as seen in Figure 3-1, with a low RMSD and RRMSD of 0.22 and
0.13, respectively, and a high Willmott d -index of 0.99, as shown in Table 3-2. Figure 3-1d
shows the scatter plot of the model and observed LAI.
30
8090
100
110
120
130
140
150
024681012
Dry Biomass (Mg/ha)
(a)
Mic
roW
EX
−2
Tot
al
Mic
roW
EX
−2
Leaf
Mic
roW
EX
−2
Ste
m
Mic
roW
EX
−2
Gra
in
Mod
el T
otal
Mod
el L
eaf
Mod
el S
tem
Mod
el G
rain
02
46
810
12024681012
(b) Mic
roW
EX
−2
Bio
mas
s (M
g/ha
)
8090
100
110
120
130
140
150
0
0.51
1.52
2.53
3.54
4.5
DoY
200
4
LAI
(c)
Mic
roW
EX
−2
LAI ±
σ
Mod
el L
AI
01
23
40
0.51
1.52
2.53
3.54
4.5
Mic
roW
EX
−2
LAI
(d)
Fig
ure
3-1.
(a)
Com
par
ison
ofth
eC
ER
ES-M
aize
esti
mat
esan
dth
eob
serv
atio
ns
ofbio
mas
sduri
ng
Mic
roW
EX
-2,(b
)sc
atte
rplo
tof
esti
mat
edan
dob
serv
edbio
mas
s,(c
)co
mpar
ison
ofth
eC
ER
ES-M
aize
esti
mat
esan
dth
eob
serv
atio
ns
ofLA
Iduri
ng
Mic
roW
EX
-2,an
d(d
)sc
atte
rplo
tof
esti
mat
edan
dob
serv
edLA
I.
31
Table 3-2. Error statistics for crop growth and ET between CERES-Maize estimates andMicroWEX-2 field observations.
Parameter RMSD RRMSD Willmott dTotal biomass (Mg/ha) 0.91 0.23 0.99Stem biomass (Mg/ha) 0.97 0.52 0.90Leaf biomass (Mg/ha) 0.47 0.44 0.93Grain biomass (Mg/ha) 0.49 1.17 0.96LAI 0.22 0.13 0.99Latent heat flux (W/m2) 42.07 0.39 0.87
3.4.2 Evapotranspiration
To understand model estimates of energy and moisture fluxes at the land surface, the
modeled daily latent heat flux is compared with the observations during MicroWEX-2.
Four comparisons were conducted [50] using two methods (RPT and PFAO) to estimate
ET and two values (0.85 and 0.5) for the canopy light extinction coefficient (KCAN).
Figure 3-2 shows a comparison of the latent heat flux estimates using the four methods.
Even though the RMSD values were low (∼40 W/m2), the temporal distribution of
latent heat fluxes was not estimated realistically during the growing season (Figure
3-2a). The latent heat fluxes were underestimated in the early season and overestimated
(∼100 W/m2) during late season. The early season underestimation indicates low
evaporation rates from the modeled soil, and the late season overestimation indicates
higher transpiration rates in the modeled vegetation. The flux estimates were not
as sensitive to KCAN values as the previous studies had found under water-stressed
conditions [50]. In terms of cumulative ET, individual under- or overestimations by the
model effectively cancel each other, so that the fit for cumulative ET is better than for
daily values (Figure 3-2b).
32
8090
100
110
120
130
140
150
050100
150
200
Heat Flux (W/m2)
(a)
8090
100
110
120
130
140
150
50100
150
200
250
ET (mm)
DoY
200
4
(b)
Mic
roW
EX
−2
RP
T, K
CA
N =
.85
RP
T, K
CA
N =
.5
PF
AO
, KC
AN
= .8
5
PF
AO
, KC
AN
= .5
Fig
ure
3-2.
Com
par
ison
ofth
ela
tent
hea
tflux
esti
mat
esfr
omC
ER
ES-M
aize
model
usi
ng
four
met
hods
wit
hth
eob
serv
atio
ns
duri
ng
Mic
roW
EX
-2by
(a)
dai
lyhea
tflux
and
(b)
cum
ula
tive
ET
.
33
3.4.3 Soil Moisture and Temperature
To understand the model performance regarding moisture and energy transport
in soil, modeled daily soil moisture and temperature profiles are compared to the
observed average daily values during MicroWEX-2 (Figures 3-3, 3-4, and 3-3). To compare
observations at 2, 4, 8, 16, 32, 64, and 100 cm to model estimates of the top six layers,
the average of 2 and 4 cm observations are compared to estimates of 0-5 cm, 8 and 16
cm observations to estimates of 5-15 cm, 16 and 32 cm observations to estimates of 15-30
cm, average of 32 cm observations to estimates of 30-45 cm, 32 and 64 cm observations to
estimates of 45-60 cm, and 64 and 100 cm observations to estimates of 60-90 cm.
34
8010
012
014
00
0.050.
1
0.150.
2
0.25
0−5
cm
(a)
VSM (m3/m
3)
8090
100
110
120
130
140
150
0
0.050.
1
0.150.
2
0.25
5−15
cm
(b)
VSM (m3/m
3)
8090
100
110
120
130
140
150
0
0.050.
1
0.150.
2
0.25
15−
30 c
m
(c)
DoY
200
4
VSM (m3/m
3)
8090
100
110
120
130
140
150
0
0.050.
1
0.150.
2
0.25
30−
45 c
m
(d)
8090
100
110
120
130
140
150
0
0.050.
1
0.150.
2
0.25
45−
60 c
m
(e)
8090
100
110
120
130
140
150
0
0.050.
1
0.150.
2
0.25
60−
90 c
m
(f)
DoY
200
4
Mic
roW
EX
−2
(Dai
ly A
vera
ge)
Mod
el
Mic
roW
EX
−2
(15
min
)
Fig
ure
3-3.
Com
par
ison
ofth
eC
ER
ES-M
aize
soil
moi
sture
esti
mat
esw
ith
Mic
roW
EX
-2ob
serv
atio
ns
atdep
ths
of(a
)0-
5cm
,(b
)5-
15cm
,(c
)15
-30
cm,(d
)30
-45
cm,(e
)45
-60
cm,an
d(f
)60
-90
cm.
35
Fig
ure
3-4.
Com
par
ison
ofth
eC
ER
ES-M
aize
soil
tem
per
ature
esti
mat
esw
ith
Mic
roW
EX
-2ob
serv
atio
ns
atdep
ths
of(a
)0-
5cm
,(b
)5-
15cm
,(c
)15
-30
cm,(d
)30
-45
cm,(e
)45
-60
cm,an
d(f
)60
-90
cm.
36
Table 3-3. model performance statistics for soil moisture and temperature betweenCERES-Maize estimates and MicroWEX-2 field observations.
RMSDLayer Soil Moisture Soil Temperature (K)5-15 cm 0.0204 2.53415-30 cm 0.0344 1.42630-45 cm 0.0164 1.48545-60 cm 0.0117 2.77560-90 cm 0.0083 3.648
The CERES-Maize model simulates moisture at daily timesteps, while the hydrological
changes near the soil surface (0-5 cm) occur at much shorter timesteps, making it
challenging to compare model and observed near-surface soil moisture. In Figure 3-3a, the
daily moisture at 0-5 cm estimated by the CERES-Maize model is compared with daily
averages and 15 min observations of volumetric soil moisture (VSM) during MicroWEX-2.
Deeper soil layers matched the observed values fairly well, as suggested by their low
RMSD values in Table 3-3, except for a 2% underestimation during the entire growing
season for the 15-30 cm layer. This is within the experimental error of the observations
made by the TDR probes.
Overall, the model did not capture the changes in soil temperatures realistically
during the growing season. It estimated temperatures at depths of 15-45 cm fairly well,
as indicated by their low RMSD values in Table 3-3. The temperatures at deeper layers
were underestimated throughout the growing season, with increasing differences as the
season progressed. For the upper layers, the model did not capture the strong fluctuations
in temperature closer to the surface.
3.5 Summary
This chapter answers the first two research questions from Chapter 1.
Question 1:”What values for the six corn cultivar coefficients give the best
DSSAT model performance for both biomass and LAI for the MicroWEX-2
growing season?”
37
The calibrated cultivar coefficient values which give the best estimates for biomass
and LAI are given in Table 3-1.
Question 2:”How do the model estimates for biomass and LAI compare with
MicroWEX-2 observations?”
The RMSD for biomass was 0.90 Mg/ha. The biomass was increasingly underestimated
by the model as the season progressed, with the maximum difference of 1.41 Mg/ha at the
end of the season. The model estimated realistic LAI with a low RMSD of 0.22.
38
CHAPTER 4CALIBRATION OF AN SVAT MODEL AND COUPLING WITH A CROP MODEL
FOR SWEET CORN
4.1 Introduction
This chapter describes the coupling of an SVAT model with a crop growth simulation
model to estimate land surface fluxes in growing vegetation and evaluate the performance
of the coupled model for estimating root-zone soil moisture and ET observations from
an extensive field experiment. Both categories of models benefit from two decades of
development and testing by their respective research communities. The SVAT model,
viz. Land Surface Process (LSP) model, simulates one-dimensional energy and moisture
transport as well as radiative, sensible and latent heat fluxes at the land surface. The
cropping system model, viz. the Decision Support System for Agrotechnology Transfer
(DSSAT), is a widely-used and tested modular suite of crop models that simulate crop
growth (biomass accumulation) and development (vegetative and reproductive growth
stages). Neither model is structurally changed and an interface is created to link the two
models. In the coupled LSP-DSSAT model, the DSSAT model provides the LSP model
with vegetation characteristics that influence heat, moisture, and radiation transfer at the
land surface and in the vadose zone and the LSP model provides the DSSAT model with
estimates of soil moisture and temperature profiles and evapotranspiration (ET).
4.2 LSP Model
The LSP model was originally developed by the Microwave Geophysics Group at
the University of Michigan [38]. The model simulates 1-d coupled energy and moisture
transport in soil and vegetation, and estimates energy and moisture fluxes at the land
surface and in the vadose zone. It is forced with micrometeorological parameters
such as air temperature, relative humidity, downwelling solar and longwave radiation,
irrigation/precipitation, and windspeed. The original version has been rigorously tested
[31] and extended to wheat stubble [30] and brome-grass [32], prairie wetlands in Florida
[64], and tundra in the Arctic [9] .
39
A new version of the LSP model was used with a modified radiation flux parameterization
at the land surface. Specifically, the shortwave radiative transfer was altered to a more
physically-based formulation, including both diffuse and direct radiation, and canopy
transmissivity described by Campbell and Norman [4]. The original version of the LSP
model followed a more empirically-based formulation by Verseghy et al. [62]. In addition,
the aerodymanic resistances and the surface vapor resistances were changed in the new
version to extend it to tall vegetation and to partially-vegetated terrain [24]. The original
version was developed for homogeneous land cover, such as bare soil or short grass. The
new version of the model also includes adaptive timesteps for computational efficiency and
to allow sudden changes or large fluxes in the sandy soils with high thermal and hydraulic
conductivities. The following section provides a detailed description of the modified LSP
model used in this study. Some fundamental governing equations are also included in the
section for completeness even though they remain unchanged from the original version.
4.2.1 Energy and Moisture Transport at the Land Surface
4.2.1.1 Energy Balance
Combining the radiation and heat flux boundary conditions, the net energy flux into
the canopy (Qnet,c) and soil (Qnet,s) (W/m2):
Qnet,c = Hsc +Rs,c +Rl,c −Hca − LEtr − LEev (4–1)
Qnet,s = −Hsc +Rs,s +Rl,s −Hsa − LEs (4–2)
where Hsc, Hca, and Hsa are the sensible heat fluxes between soil and canopy, canopy and
air, and soil and air, respectively; LEtr, LEev, and LEs are the latent heat fluxes from
transpiration, canopy evaporation, and soil evaporation, respectively; and Rs,c, Rs,s, Rl,c,
Rl,s, are the net solar radiation intercepted by the canopy, intercepted solar radiation by
the soil, net longwave radiation at the canopy, and net longwave at the soil, respectively.
Solar Radiation (Rs,c and Rs,s)
40
Downwelling solar radiation is partitioned between the soil and canopy by first
dividing total solar radiation into direct and diffuse components, as an empirical function
of clearness index and apparent solar time [1]. The direct fraction is either transmitted,
reflected, or absorbed. The net solar radiation absorbed by the canopy and soil are
Rs,c = [(1− fd)(1− τc,dir)(1− ρc,dir) + (fd)(1− τc,diff )(1− ρc,diff )]Rs,down (4–3)
Rs,s = (1− ρs)[(1− fd)(τc,dir)(1− ρc,dir) + (fd)(τc,diff )(1− ρc,diff )]Rs,down (4–4)
where fd is the diffuse fraction, τc,dir is the direct canopy transmissivity, τc,diff is the
diffuse canopy transmissivity, ρc,dir is the direct canopy reflectance, ρc,diff is the diffuse
canopy reflectance, ρs is the soil reflectance, and Rs,down is the downwelling solar radiation.
The direct canopy transmissivity is τc,dir, given by Campbell and Norman [4]:
τc,dir = e−K(x,Θ)√
1−σΩLAI (4–5)
where K(x,Θ) is the canopy extinction coefficient for canopy with an ellipsoidal leaf
angle distribution, σ is the reflectance of a single leaf, x is the leaf angle distribution
parameter, Θ is the solar zenith angle, LAI is the leaf area index of the canopy, and Ω is
the clumping factor which accounts for incomplete canopy cover.
The canopy reflectance is calculated as
ρc,dir =2K(x,Θ)
1 +K(x,Θ)
1−√1− σ
1 +√
1− σ(4–6)
The diffuse canopy transmissivity, τc,diff , is found by integrating τc,dir over all solar zenith
angles. Diffuse canopy reflectance ρc,diff is given by Goudriaan [24]:
ρc,diff =1−√1− σ
1 +√
1− σ(4–7)
Radiation transmitted by the canopy is either reflected or absorbed by the soil according
to the soil albedo, ρs, an empirical function of soil moisture, derived from MicroWEX-2
41
Figure 4-1. Surface resistance network to estimate sensible and latent heat fluxes in theLSP model.
bare-soil data:
ρs = 0.0854e[−max(θs−0.0532,0)2/0.0037] + 0.14650 (4–8)
where θs is the surface volumetric soil moisture (m3/m3).
Longwave Radiation (Rl,c and Rl,s)
The net longwave radiation abosrbed by the canopy (Rl,c) and soil (Rl,s) are given by
Kustas and Norman [35]:
Rl,c = (1− τl)Rl,down + (1− τl)εsσsbT4s − 2(1− τl)εcσsbT
4c (4–9)
Rl,s = (τl)Rl,down − εsσsbT4s + (1− τl)εcσsbT
4c (4–10)
where σsb is the Stefan-Boltzmann constant, Rl,down is the downwelling longwave radiation,
εs is the soil emissivity, εc is the canopy emissivity, and Ts and Tc are the soil and canopy
temperatures in Kelvin. τl is the longwave canopy transmissivity, the integral over the
hemisphere of direct transmissivity with σ as zero.
Sensible Heat Fluxes
Figure 4-1(a) shows the resistance network model used to estimate sensible heat flux
(H) at the surface.The sensible heat fluxes between the soil and air (Hsa), soil and canopy
42
(Hsc), and canopy and air (Hca), are calculated as:
Hsa = ρacpaTs − Ta
ras
fB (4–11)
Hsc = ρacpaTs − Tc
rsc + rbh
fV (4–12)
Hca = ρacpaTs − Tc
rac + rbh
fV (4–13)
where Ta, Ts,and Tc are the air, soil, and canopy temperatures (K), respectively, ρa is the
air density (kg/m3), cpa is the specific heat (J/kg K), fV and fB are the vegetation and
bare soil cover fractions, respectively.
The aerodynamic resistances ras (soil-air) and rac (canopy-air) are determined
assuming a log wind profile above the canopy or bare soil [24]:
ras =ln
(z
zob
)+ ΨH
ku∗(4–14)
rac =ln
(z−dzov
)+ ΨH
ku∗(4–15)
u∗ =ku(z)
ln(
z−dzo
)+ ΨM
(4–16)
where u∗ is the friction velocity, Ψ is the Businger-Dyer stability function [17], k is von
Karman’s constant (0.4), z is the measurement height, d is the vegetation displacement
height (taken as 0.63hc, hc is the plant canopy height), zov is the vegetation roughness
length (0.1hc), and zob is the bare soil roughness length.
For the aerodynamic resistance between the soil and the canopy, the log profile is not
valid due to momentum absorption by the canopy elements, so an exponential wind profile
in the canopy is used [24], with the under-canopy resistance, rsc, from Niu and Yang [42]:
rsc =hc
aKh
[ea(1−zob/hc) − ea(1−zov/hc)] (4–17)
43
where a and Kh are the canopy damping coefficient and the aerodynamic conductance for
heat at the top of the canopy [24], given by:
a =
√cdLAIhc
2lmiw(4–18)
where
lm = 23
√0.75w2
chc
πLAI(4–19)
Kh = ku∗(hc − d) (4–20)
where, lm is the canopy momentum length, iw is the wind intensity factor, cd is the drag
coefficient, and wc is canopy width. The leaf boundary layer resistances for heat transport,
rbh, is calculated as:
rbh =1
2(180)
√lwuc
(4–21)
uc = ku∗ln(hc − d
zov
)(4–22)
Latent Heat Flux
Latent heat flux is based upon the resistance network (see Figure 4-1(b)). Three
sources that contribute to the flux are: soil evaporation (LEs), canopy transpiration
(LEtr), and evaporation of intercepted precipitation (LEev).
LEs = λρa(qs − qa)
(fV
rs + rsc + rca
+fB
rs + ras
)(4–23)
LEtr = λρa(qc,sat − qa)
[fV (1− xl)
rac + rbv + rlv
](4–24)
LEev = λρa(qc,sat − qa)fV xl
rac + rbv
(4–25)
where qa, qs, and qc,sat are the specific humidities of the air, soil surface layer, and
saturated canopy, respectively, λ is the latent heat of vaporization of water, and xl is
the fraction of vegetation covered in intercepted precipitation, calculated by
xl =Wr
Wr,max
(4–26)
44
Wr,max = 0.2LAI (4–27)
where Wr,max is the maximum possible interception, and Wr is the intercepted moisture by
the canopy [62]. rbv is the leaf boundary layer moisture resistance. rlv and rs are surface
vapor transport resistances for the leaves and soil, repectively, where lw is leaf width. The
leaf resistance is based on canopy assimilation [24]:
rbv = 0.93rbh (4–28)
rlv =∆CCO2
1.66Fn
− .783rbh (4–29)
Fn = (1− eRs,cεphoto/Fm)(Fm − Fd) + Fd (4–30)
where ∆CCO2 is the concentration difference of CO2 between the leaf and air, in kg/m3,
εphoto is the photosynthetic efficiency, Fn is the net assimilation (kg CO2/m2s), Fd is the
base assimilation rate, determined by a Q10 relationship from parameter Fb, and Fm, the
maximum assimilation rate, is estimated as 10Fd.
Soil surface resistance is a linear function of surface moisture deficit [3],
rs = soila∆θ + soilb (4–31)
where moisture deficit (∆θ) is the difference between saturated moisture content and
actual moisture content.
4.2.1.2 Moisture Balance
The net infiltration of moisture at the soil surface (Inet,s) is given by:
Inet,s = PfB +D −R− Es (4–32)
where P is the precipitation, D is the canopy drainage from the canopy to the soil, R is
the runoff, and Es is the soil evaporation. D given by Wr −Wr,max. The rate of change in
moisture intercepted by the canopy is given by
45
dWr
dt= PfV −D − Eev (4–33)
4.2.2 Soil Processes
Heat and moisture transport in the soil is determined as the numerical solution to
[47]:
∂θ
∂t= −∇qm (4–34)
Cv,s∂T
∂t= −∇qh (4–35)
qm = ql + qv (4–36)
ql = −Dθ,l∇θ −DT,l∇T +K + S (4–37)
qv = −Dθ,v∇θ −DT,v∇T (4–38)
qh = −κ∇T + ρλqv + Cv,w(T − T0)qm (4–39)
where ql, qv, and qh are liquid, vapor, and heat fluxes, respectively; T and θ are temperature
and volumetric soil moisture, respectively. Dθ,l is the diffusivity of liquid under a moisture
gradient; DT,l is the diffusivity of liquid under a temperature gradient; Dθ,v is the
diffusivity of vapor under a moisture gradient; DT,v is the diffusivity of vapor under a
temperature gradient, from [47]; K is hydraulic conductivity, from [49]; κ is thermal
conductivity of soil from [11], S is a sink term (root water uptake), and Cv,s is the
volumetric heat capacity of soil. Cv,w, ρ, and λ are the heat capacity, density, and heat of
vaporization of water.
The soil profile is defined with layers of different constitutive properties, divided into
computational blocks, with the thickness of blocks increasing exponentially with depth.
The coupled heat and moisture transport equations are solved using a block-centered,
foward-time finite difference scheme. The upper boundary condition is a heat and moisture
flux determined by the meteorological forcings, while the lower boundary condition
assumes free flow of heat and moisture.
46
Figure 4-2. Algorithm for the coupling of the LSP and DSSAT models.
4.3 Coupling of LSP and DSSAT models
Both the LSP and the DSSAT models are forced with micrometeorological conditions
provided in each model’s required format. A flowchart of the model coupling is shown
in Figure 4-2. The soil moisture and temperature profiles are initialized in both models.
The LSP model simulates energy and moisture fluxes using an adaptive timestep. At the
last timestep of each day, the daily averages of ET, soil moisture and soil temperature
are calculated and passed on to the DSSAT model. The DSSAT uses these values in
calculating growth rates to obtain the crop variables such as biomass, LAI, etc. using a
daily timestep. The estimates of biomass, root-length densities, LAI, height, and width are
provided to the LSP model for flux estimation on the next day.
The main challenge in coupling an SVAT model such as the LSP and a crop model
such as the DSSAT arises from the difference in timestep and thickness of soil nodes
47
between the two models. The LSP model uses short timesteps (on the order of seconds)
and a user-defined number of nodes (35 in the top 1.8 m for this study). DSSAT uses
daily timesteps, with 9 nodes in the top 1.8 m. In the coupling, the LSP model essentially
replaces the soil and soil-plant-atmosphere modules of the DSSAT model. To account for
the timestep difference, the soil moisture and temperature profiles estimated by the LSP
model are averaged daily. The latent heat fluxes are accumulated daily and converted from
W/m2 to mm/day, treating soil and vegetation latent heat fluxes separately so that it can
match the DSSAT requirements. To account for the difference in thickness of soil nodes,
the daily averages of soil moisture and temperature profiles from the LSP were spatially
averaged to match the soil nodes in the DSSAT. In addition, the root length density for
the 9 DSSAT nodes are interpolated/extrapolated to match the LSP nodes. Because the
LSP model does not include nitrogen transport in canopy and soil, the DSSAT model
is run assuming there is no nitrogen stress. This is a reasonable assumption for heavily
fertigated soils, such as those during MicroWEX-2.
4.4 Methodology
In this study, the model simulations were conducted using two scenarios. First,
using a stand-alone LSP simulation forced with vegetation parameters observed during
MicroWEX-2 and second, using the coupled LSP-DSSAT model.
4.4.1 Inputs and Initial Conditions
Both the LSP and LSP-DSSAT models were run from planting on DoY 78, to
harvest on DoY 154, 2004. Micrometeorological forcings were obtained from observations
during MicroWEX-2, and from a nearby weather station, installed as part of the Florida
Automated Weather Network (FAWN). The precipitation/irrigation observations exhibited
most variability between the four raingauges (Figure 2-5). To obtain forcings for the model
simulations, we confirmed that raingauge data coincided with the observed soil moisture
increases. The data were scaled such that the daily accumulated observations from the
48
Table 4-1. Values for soil properties in the LSP model.
Parameter Description 0-1.7 m 1.7-2.7 mλ Pore-size index 0.27 0.05ψ0 Air entry pressure (m H2O) 0.076 0.019Ksat Saturated hydraulic conductivity (m/s) 2.06×10−4 8.93×10−5
θr Volumetric wilting point moisture (m3/m3) 0.0051 0.0040θsat Volumetric saturation moisture (m3/m3) 0.34 0.41φsa Volumetric sand fraction (m3/m3) 0.894 0.512φsi Volumetric silt fraction (m3/m3) 0.034 0.083φc Volumetric clay fraction (m3/m3) 0.071 0.405φo Volumetric organic fraction (m3/m3) 0.000 0.000φ Porosity 0.34 0.41
raingauges matched those observed independently at the same field site using collection
cans [16].
Initial conditions were not known during MicroWEX-2 because the sensor installation
was completed 7 days after planting. The first values observed by the soil moisture and
temperature sensors were used as the initial moisture and temperature values for the
simulations.
Soil physical properties were based on texture and retention curve measurements
taken from soil samples in the field at different depths, and are listed in Table 4-1.
4.4.2 Calibration
The DSSAT and the LSP models were calibrated separately for the entire growing
season. In the DSSAT model, six corn cultivar coefficients governing the growth and
development, as described in Chapter 3, were calibrated using Simulated Annealing to
minimize the root mean square difference (RMSD) between modeled and observed LAI
and biomass during MicroWEX-2.
In the LSP model, 12 parameters were calibrated using repeated Latin Hypercube
Sampling of the parameter space [40]. Four of these parameters were related to radiation
balance: leaf reflectance, σ, leaf angle distribution, x, soil emissivity, εs, and canopy
emissivity, εc. The remaining eight parameters were related to sensible and latent
heat fluxes: canopy base assimilation rate, Fb, photosynthetic efficiency, εphoto, bare
49
Table 4-2. Sampling ranges from [24] and calibrated values for parameters in the LSPmodel.
Parameter Description Sampling Range Calibrated valuezob Bare soil roughness length (m) 10−4 - 10−2 0.004x Leaf angle distribution parameter 10−2 - 2.0 0.819σ Leaf reflectance 10−2 - 0.5 0.474εc Canopy emissivity 0.95 - 0.995 0.973εs Soil emissivity 0.95 - 0.995 0.953cd Canopy drag coefficient 10−5 - 1.0 0.328iw Canopy wind intensity factor 10−3 - 102 67.90lw Leaf width (m) 10−3 - 10−1 0.0531Fb Base assimilation rate (kg CO2/m2s) -10−8 - -10−10 -8.20×10−9
εphoto Photosynthetic efficiency (kg CO2/J) 10−7 - 10−5 8.97×10−7
soila Slope parameter for rs (m2s/kg H2O) 0.0 - 5×103 3700.0soilb Intercept parameter for rs (m2s/kg H2O) 0.0 - -6×102 -531.0
soil aerodynamic roughness, zob, leaf width, lw, wind intensity factor, iw, canopy drag
coefficient, cd, and soil evaporation resistance parameters, soila and soilb. The calibration
of these parameters was conducted to minimize RMSDs between the modeled and
observed volumetric soil moisture (VSM) at 2 cm and latent heat flux (LE) for the
overall growing season. These two objectives were chosen because VSM is one of the most
important factors governing the moisture and energy fluxes, and in the calibration VSM
and LE were found to be competing objectives.
During the calibration, five thousand points were sampled in the form of twenty
250-point Latin Hypercube Samples within the ranges from Goudriaan [24], specified in
Table 4-2, using the University of Florida’s High-Performance Computing Center. These
sampled points were ordered by Pareto ranking and the set of points with the lowest
Pareto rank were considered as the optimal parameter set [25].
50
Figure 4-3. Pareto fronts from calibration of the stand-alone LSP model. The asteriskrepresents the point on the Pareto front where the total seasonal RMSD for 2cm VSM is 0.04 m3/m3.
4.5 Results and Discussion
4.5.1 Calibration
4.5.1.1 DSSAT
Table 3-1 provides the calibrated values of the six cultivar coefficients in the DSSAT
model. These values were used for simulations using both stand-alone DSSAT and coupled
LSP-DSSAT models.
4.5.1.2 LSP
The result of the multiobjective calibration was a Pareto front [25]. Figure 4-3
shows the Pareto fronts for the overall growing season with RMSDs between the model
51
estimates and observations of the two objectives, VSM at 2 cm and LE. Even though the
calibrated parameters were obtained for the whole growing season, the growing season was
divided into four periods to understand the differences in Pareto fronts during different
growth stages (Figure 4-3). These four stages include: almost bare soil (DoY 78-105),
intermediate vegetation cover (DoY 105-125), full vegetation cover (DoY 125-135),
and reproductive stage (DoY 135-154). A Pareto front could not be generated for the
reproductive stage due to lack of LE observations during this stage. In general, the
fronts show that the model performs best during the intermediate cover stage, with the
front closest to the origin, and worst during the almost bare soil stage, with the front
farthest from the origin. The worst performance during the bare soil stage is primarily
due to fewer observations (<2000) from MicroWEX-2 during this stage compared to the
>4000 observations during vegetated stages, resulting in calibrated parameters biased
towards minimizing differences during the vegetated stages. For the stand-alone LSP and
LSP-DSSAT simulations in this study, the Pareto front for the overall season in Figure
4-3 was used to choose the 12 parameter values corresponding to an RMSD in VSM at
2 cm of 0.04 m3/m3, noted by an asterisk in the Figure. This choice was based upon the
sensitivity of SVAT models to VSM for hydrometeorological applications [20, 34, 36]. With
the RMSD in VSM of 0.04 m3/m3, there is an expected RMSD in latent heat flux of about
45 W/m2 for the overall season and about 55, 40, and 50 W/m2 for the first three stages,
respectively (see Figure 4-3). Table 4-2 lists the calibrated parameter values used in the
LSP and LSP-DSSAT model simulations.
4.5.2 Model Simulation
4.5.2.1 DSSAT
The DSSAT model provided realistic estimates of growth and development of sweet
corn. Both the stand-alone DSSAT and LSP-DSSAT models estimated the emergence date
on DoY 90, compared to DoY 86 observed during MicroWEX-2. Modeled anthesis day,
52
Table 4-3. Comparison of LAI, dry biomass (kg/m2), and ET (mm) for stand-aloneDSSAT and coupled LSP-DSSAT simulations.
Stand-Alone DSSAT Coupled LSP-DSSATRMSD MAD Bias RMSD MAD Bias
LAI (-) 0.38 0.26 0.06 0.43 0.39 0.29Total Biomass (kg/m2) 0.90 0.63 -0.59 0.52 0.40 0.05
ET (mm) 1.63 1.36 0.31 1.64 1.25 0.62
when 75% of the corn has silked, was DoY 139, while 75% silking was observed on DoY
135.
Figure 4-4 and Table 4-3 show the comparison of estimates of LAI and dry biomass
by the stand-alone DSSAT model, by the LSP-DSSAT model, and those observed
during MicroWEX-2. Estimates from both model simulations compared well with the
observations with RMSDs of <0.5 for LAI and <1.0 kg/m2 for dry biomass.
The estimates from the two models differed by <0.2 for LAI and <0.6 kg/m2 for
dry biomass, with the coupled LSP-DSSAT model estimating higher values than the
stand-alone DSSAT. These relatively small differences could be due to higher daily
averages of soil moisture in the LSP-DSSAT than those in the stand-alone DSSAT’s
bucket model, by > 0.02 m3/m3 (Figure 4-4(c)). The higher soil moisture values would
permit increased growth resulting in higher LAI and dry biomass in the coupled model.
The high moisture estimates also result in higher daily ET in the coupled model compared
to the DSSAT (Figure 4-4(d)). The LSP-DSSAT predicts <0.5 mm/day higher ET than
DSSAT alone, with the RMSD between the daily estimates of ET by the LSP-DSSAT and
observations of 1.69 mm.
4.5.2.2 LSP-DSSAT Model
The performance of the coupled LSP-DSSAT model was evaluated by comparing
its estimates of surface fluxes, soil moisture, and temperature profiles to those observed
during MicroWEX-2, and to those estimated by the stand-alone simulation of the LSP
model. These comparisons are discussed for the four growth stages and during the entire
growing season separately to provide detailed insight into modeled fluxes during different
53
80 90 100 110 120 130 140 1500
5
10
15D
ry B
iom
ass
(Mg/
ha)
DoY 2004
(a)
MicroWEX−2
DSSAT
LSP−DSSAT
80 90 100 110 120 130 140 1500
1
2
3
4
LAI
DoY 2004
(b)
80 90 100 110 120 130 140 1500
0.1
0.2
0.3
VS
M (
m3 /m
3 )
DoY 2004
(c)
80 90 100 110 120 130 140 1500
2
4
6
8
10
12
ET
(m
m)
DoY 2004
(d)
Figure 4-4. Comparison of estimations by the coupled LSP-DSSAT and stand-aloneDSSAT model simulation and those observed during MicroWEX-2: (a) drybiomass, (b) LAI, (c) 5 cm soil moisture, and (d) ET.
54
Table 4-4. Comparison of surface fluxes (W/m2), for stand-alone LSP and coupledLSP-DSSAT simulations.
Stand-Alone LSP Coupled LSP-DSSATFlux RMSD MAD Bias RMSD MAD Bias
Net Radiation 23.86 16.11 10.38 25.62 18.12 12.65Latent Heat Flux 46.34 32.03 14.96 50.69 35.28 18.84Sensible Heat Flux 34.48 24.07 15.69 37.19 24.79 14.88
Soil Heat Flux 47.68 26.24 -1.54 46.54 25.02 -1.83
Table 4-5. Comparison of volumetric soil moisture (m3/m3), for stand-alone LSP andcoupled LSP-DSSAT simulations.
Stand-Alone LSP Coupled LSP-DSSATDepth (cm) RMSD MAD Bias RMSD MAD Bias
2 0.047 0.044 0.044 0.046 0.043 0.0434 0.035 0.029 0.029 0.034 0.028 0.0288 0.036 0.030 0.028 0.036 0.030 0.02832 0.032 0.031 0.031 0.032 0.031 0.03064 0.062 0.061 0.061 0.062 0.061 0.061100 0.060 0.057 0.057 0.060 0.057 0.057
growing stages. The model simulations were conducted using calibrated parameter values
given in Table 4-2. This section discusses statistics for coupled LSP-DSSAT model
simulation, but Tables 4-4-4-6 provide detailed statistics for both the coupled LSP-DSSAT
and the stand-alone LSP model simulation.
Early Season - Almost Bare Soil
This period included the first 27 days of the growing season (DoY 78-105), when
it was “almost” bare soil with low vegetation. The canopy height was < 17 cm, LAI
was < 0.2, and vegetation cover was < 0.22. Figures 4-5(a) and (b) show the estimated
Table 4-6. Comparison of soil temperature (K), for stand-alone LSP and coupledLSP-DSSAT simulations.
Stand-Alone LSP Coupled LSP-DSSATDepth (cm) RMSD MAD Bias RMSD MAD Bias
2 2.80 2.22 1.90 2.43 1.91 1.374 2.88 2.21 1.73 2.56 2.00 1.218 2.60 2.03 1.73 2.27 1.77 1.2232 2.03 1.56 1.40 1.76 1.41 0.9364 1.70 1.24 1.09 1.45 1.15 0.67100 1.26 0.91 0.44 1.12 0.90 0.09
55
80 85 90 95 100 105−200
0
200
400
600
800
1000
Net
Rad
iatio
n (W
/m2 )
(a)MicroWEX−2 LSP LSP−DSSAT
80 85 90 95 100 105
−300
−200
−100
0
100
200
300
Net
Rad
iatio
n (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-5. Comparison of net radiation, between DoY 78 to 105, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
Table 4-7. Measurement uncertaintities during MicroWEX-2.
Sensor Uncertainty ReferenceRaingauge 12 mm/h [44]
TDR 0.025 VSM [5]Thermistor 0.1 K [45]
Soil heat flux 15 W/m2 [56]Net radiation 22 W/m2 [56]
Latent heat flux 17-36 W/m2 [56]Sensible heat flux 21 W/m2 [56]
56
80 85 90 95 100 105−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
80 85 90 95 100 105
−300
−200
−100
0
100
200
300
Res
idua
ls (
W/m
2 )
DoY 2004 (EST)
(b)
Figure 4-6. Comparison of latent heat flux, between DoY 78 to 105, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
and observed net radiation as well as residuals (LSP-DSSAT minus observed) during
this period, respectively. Overall, both the coupled and the stand alone models capture
the phases of the diurnal variation in net radiation. The RMSDs between the model
estimates and observations are similar for both models’ simulations (coupled LSP-DSSAT
and stand-alone LSP) at ∼32 W/m2. However, the peak daytime differences are as high
as 100 W/m2 on DoY 93, 95, 96, and 97. This corresponds to days when the model
estimates of VSM at 2 cm were higher than observed, with RMSD of 0.0374 m3/m3 and
bias of 0.036 m3/m3 (Figure 4-9). This overestimation in VSM, possibly due to improper
initial conditions and/or improper precipitation inputs (see Sections 4.4.1 and 4.5.2.2),
would lead to lower estimates of soil albedo using Equation 4–8. The overestimation also
results in higher LE estimates (Figures 4-6(a) and (b)) due to underestimated soil surface
57
80 85 90 95 100 105−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
80 85 90 95 100 105
−300
−200
−100
0
100
200
300
Hea
t Flu
x (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-7. Comparison of sensible heat flux, between DoY 78 to 105, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
resistance using Equation 4–31. In both the coupled and the standalone models, LE is
overestimated with RMSDs of ∼54 W/m2 and biases of ∼18 W/m2. These RMSDs are
higher than the sensor uncertainty of 17-36 W/m2 (Table 4-7) but are comparable with
those expected from Figure 4-3 using the Pareto front from the early season (see Section
4.5.1.2).
Both the coupled and stand-alone models estimate similar sensible heat fluxes, with
RMSDs of ∼40 W/m2 and biases of ∼16 W/m2 (Figure 4-7). These RMSDs are lower
than those obtained for LE. For the days when LE is positively biased (e.g. DoY 97, 98,
101, 102, and 103), the sensible heat flux is biased negatively, and vice versa. The overall
RMSD for sensible heat fluxes could be due to slightly lower aerodynamic resistance
and/or due to overestimation of soil temperature in both the models (Figure 4-10). The
58
80 85 90 95 100 105−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
80 85 90 95 100 105
−300
−200
−100
0
100
200
300
Hea
t Flu
x (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-8. Comparison of soil heat flux, between DoY 78 to 105, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
RMSDs between the models and observations for soil temperature are <2.22 K. This
positive bias (<1.7 K) in soil temperature in the beginning of the simulation could be due
to improper initial conditions (see Section 4.4.1).
The estimated soil heat flux (Figure 4-8) is overestimated during the day and
underestimated at night. The net effect of which is 2 cm soil heat flux is slightly
underestimated with RMSDs of ∼48 W/m2 and biases of ∼-3 W/m2, because the
magnitude of the latent and sensible heat flux biases exceeds that of the net radiation
overestimation.
Mid-Season - Intermediate Vegetation Cover
This period included the next 20 days of the growing season, when the vegetation is
partially covering the terrain (DoY 105-125). The canopy height was 17-73 cm, LAI was
59
80 85 90 95 100 1050.05
0.1
0.15
0.2(a)
VS
M (
m3 /m
3 )
80 85 90 95 100 1050.05
0.1
0.15
0.2(b)
VS
M (
m3 /m
3 )
80 85 90 95 100 1050.05
0.1
0.15
0.2(c)
VS
M (
m3 /m
3 )
80 85 90 95 100 1050.05
0.1
0.15
0.2(d)
VS
M (
m3 /m
3 )
80 85 90 95 100 1050.05
0.1
0.15
0.2(e)
VS
M (
m3 /m
3 )
80 85 90 95 100 1050.05
0.1
0.15
0.2(f)
DoY 2004 (EST)
VS
M (
m3 /m
3 )
MicroWEX−2 LSP LSP−DSSAT
Figure 4-9. Comparison of volumetric soil moisture estimated by the coupled LSP-DSSATand stand-alone LSP model simulation and those observed duringMicroWEX-2, between DoY 78 to 105: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32cm, (e) 64 cm, and (f) 100 cm.
60
80 85 90 95 100 105
280
300
320
(a)Tem
p. (
K)
80 85 90 95 100 105
280
300
320
(b)Tem
p. (
K)
80 85 90 95 100 105
280
300
320
(c)Tem
p. (
K)
80 85 90 95 100 105
280
300
320
(d)Tem
p. (
K)
80 85 90 95 100 105
280
300
320
(e)Tem
p. (
K)
80 85 90 95 100 105
280
300
320
DoY 2004 (EST)
Tem
p. (
K)
(f)
MicroWEX−2 LSP LSP−DSSAT
Figure 4-10. Comparison of soil temperature estimated by the coupled LSP-DSSAT andstand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 78 to 105: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm.
61
105 110 115 120 125−200
0
200
400
600
800
1000
Net
Rad
iatio
n (W
/m2 )
(a)MicroWEX−2 LSP LSP−DSSAT
105 110 115 120 125
−300
−200
−100
0
100
200
300
Net
Rad
iatio
n (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-11. Comparison of net radiation, between DoY 105 to 125, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
0.2-1.82, and fractional vegetation cover was 0.22-1.00. Overall, the model performance
is better during this growth stage compared to the previous stage, as expected from the
Pareto fronts (Figure 4-3 and Section 4.5.1.2).
As the vegetation cover increased during this period, the residuals in net radiation
decrease significantly, indicating the decreasing influence of soil albedo on radiation
balance. The daytime residuals decrease from ∼80 W/m2 before DoY 115 to <30 W/m2
after DoY 115 (Figure 4-11). Due to the improved net radiation estimates (RMSD ∼27
W/m2), and the decreasing influence of soil surface resistance, RMSDs in LE are lower
during this stage than during the bare soil stage (compare Figures 4-6 and 4-12) even
though VSM remains overestimated by similar amounts (compare Figures 4-9 and 4-15).
62
105 110 115 120 125−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
105 110 115 120 125
−300
−200
−100
0
100
200
300
Res
idua
ls (
W/m
2 )
DoY 2004 (EST)
(b)
Figure 4-12. Comparison of latent heat flux, between DoY 105 to 125, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
The RMSD of ∼40 W/m2 correspond to those expected from the Pareto front in Figure
4-3.
Similarly low RMSDs and biases are found in sensible heat flux, soil heat flux, and
soil temperature. Sensible heat flux is overestimated, but matches more closely with
observations during this stage than during the bare soil stage (Figure 4-13), with RMSDs
of ∼30 W/m2 and biases of ∼12 W/m2. Soil heat flux remains overestimated during
the day and underestimated at night, similar to the previous stage (Figures 4-14(a) and
(b)). Overall, the 2 cm soil heat flux is underestimated with RMSD of ∼39 W/m2 and
biases of ∼-6 W/m2 and . This is reflected in the soil temperature (Figure 4-16) as a lower
overestimation (RMSD < 1.67 K and bias < 0.67 K) than in the previous stage for the
63
105 110 115 120 125−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
105 110 115 120 125
−300
−200
−100
0
100
200
300
Hea
t Flu
x (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-13. Comparison of sensible heat flux, between DoY 105 to 125, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
stand-alone LSP, and an underestimation (RMSD < 1.47 K and a negative bias > -0.91
K) in the case of the LSP-DSSAT model.
Late Season - Vegetative Stage
This period included the next ten days of the growing season, when the corn was
in the vegetative growth stage and at full vegetation cover (DoY 125-135). The canopy
height was 73-162 cm, LAI was 1.82-2.49, and vegetation cover was 1.00.
In the previous stage, as vegetation cover increased, residuals for net radiation
decreased. Because of full vegetation cover during this stage, net radiation (Figure 4-17)
matches very closely with observations, with RMSDs of ∼16 W/m2 and biases of ∼8
W/m2, less than the estimated sensor uncertainty (Table 4-7). LE is overestimated with
RMSD of ∼49 W/m2 and bias of ∼16 W/m2 (Figure 4-18). The RMSD of ∼49 W/m2
64
105 110 115 120 125−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
105 110 115 120 125
−300
−200
−100
0
100
200
300
Hea
t Flu
x (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-14. Comparison of soil heat flux, between DoY 105 to 125, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
correspond to the RMSD expected from the Pareto front in Figure 4-3. Though the net
radiation matches well, it is still biased high, which would permit lower leaf surface vapor
resistance by Equations 4–29 and 4–30, resulting in overestimated LE from increased
canopy transpiration. Overestimated VSM, shown in Figure 4-21, (RMSD 0.0492 m3/m3
and positive bias 0.0472 m3/m3) could also lead to overestimation of LE by increasing soil
evaporation.
Sensible heat flux (Figure 4-19) is overestimated with RMSDs of ∼43 W/m2 biases of
∼22 W/m2. This overestimation could be due to overestimated vegetation aerodynamic
roughness length.
The 2 cm soil heat flux (Figure 4-20) is slightly overestimated with RMSD of ∼44
W/m2 and bias of ∼0.70 W/m2. Since during full cover, the net flux going into the soil
65
105 110 115 120 1250.05
0.1
0.15
0.2(a)
VS
M (
m3 /m
3 )
105 110 115 120 1250.05
0.1
0.15
0.2(b)
VS
M (
m3 /m
3 )
105 110 115 120 1250.05
0.1
0.15
0.2(c)
VS
M (
m3 /m
3 )
105 110 115 120 1250.05
0.1
0.15
0.2(d)
VS
M (
m3 /m
3 )
105 110 115 120 1250.05
0.1
0.15
0.2(e)
VS
M (
m3 /m
3 )
105 110 115 120 1250.05
0.1
0.15
0.2(f)
DoY 2004 (EST)
VS
M (
m3 /m
3 )
MicroWEX−2 LSP LSP−DSSAT
Figure 4-15. Comparison of volumetric soil moisture estimated by the coupledLSP-DSSAT and stand-alone LSP model simulation and those observedduring MicroWEX-2, between DoY 105 to 125: (a) 2 cm, (b) 4 cm, (c) 8 cm,(d) 32 cm, (e) 64 cm, and (f) 100 cm.
66
105 110 115 120 125
280
300
320
(a)Tem
p. (
K)
105 110 115 120 125
280
300
320
(b)Tem
p. (
K)
105 110 115 120 125
280
300
320
(c)Tem
p. (
K)
105 110 115 120 125
280
300
320
(d)Tem
p. (
K)
105 110 115 120 125
280
300
320
(e)Tem
p. (
K)
105 110 115 120 125
280
300
320
DoY 2004 (EST)
Tem
p. (
K)
(f)
MicroWEX−2 LSP LSP−DSSAT
Figure 4-16. Comparison of soil temperature estimated by the coupled LSP-DSSAT andstand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 105 to 125: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm.
67
125 126 127 128 129 130 131 132 133 134 135−200
0
200
400
600
800
1000
Net
Rad
iatio
n (W
/m2 )
(a)MicroWEX−2 LSP LSP−DSSAT
125 126 127 128 129 130 131 132 133 134 135
−300
−200
−100
0
100
200
300
Net
Rad
iatio
n (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-17. Comparison of net radiation, between DoY 125 to 135, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
is dominated by the flux between the soil and the canopy, the overestimation of soil heat
flux indicates that soil-canopy flux is underestimated. This overestimation in soil heat flux
leads to overestimation in soil temperature (Figure 4-22), moreso than during intermediate
vegetation cover, with a positive bias < 2.68 K and RMSD < 3.32 K.
Reproductive Stage
The last 19 days of the growing season, DoY 135 - 154, comprised the reproductive
stage, beginning with silk formation. During this period, the canopy height was 162-200
cm, LAI was 2.49-2.75, and vegetation cover was 1.00. The biomass growth during this
stage was primarily due to ear growth.
68
125 126 127 128 129 130 131 132 133 134 135−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
125 126 127 128 129 130 131 132 133 134 135
−300
−200
−100
0
100
200
300
Res
idua
ls (
W/m
2 )
DoY 2004 (EST)
(b)
Figure 4-18. Comparison of latent heat flux, between DoY 125 to 135, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
Similar to the previous stage, net radiation (Figure 4-23) matches very closely with
observations, with RMSDs of ∼17 W/m2 and biases of ∼2.6 W/m2. The LE and H
comparison could not be presented due to missing observations during this period.
The 2 cm soil heat flux (Figures 4-24) is slightly overestimated with RMSDs of ∼55
W/m2 and biases of ∼2.3 W/m2, for similar reasons as during the non-reproductive
full cover period. The overestimation in soil heat flux leads to overestimation in soil
temperature (Figure 4-26), with RMSD < 3.39 K and a positive bias < 3.39 K.
VSM (Figure 4-25) is overestimated with RMSD 0.0632 m3/m3 and a positive bias
0.0623. The overestimation could be due to incorrect precipitation inputs, or accumulated
moisture because of underestimated hydraulic conductivity in the bottom clay layer.
Growing Season - Planting to Harvest
69
125 126 127 128 129 130 131 132 133 134 135−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
125 126 127 128 129 130 131 132 133 134 135
−300
−200
−100
0
100
200
300
Hea
t Flu
x (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-19. Comparison of sensible heat flux, between DoY 125 to 135, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
The coupled LSP-DSSAT model estimates radiation, fluxes, and soil moisture and
temperature profiles that are very similar to those estimated by the stand-alone LSP
model with observed vegetation parameters for the growing season, as shown in Figures
4-27-4-29 and Tables 4-4-4-6. The RMSDs for the fluxes from the LSP-DSSAT model
are slightly higher (by ∼3 W/m2) than those from the LSP model, primarily because
modeled canopy characteristics used in the LSP-DSSAT model rather than observations.
For instance, LSP-DSSAT overestimates LAI by 0.29, compared to the stand-alone DSSAT
which overestimates by 0.06 (Figure 4-4(c)), increasing canopy interception and net
radiation.
Overall, both the LSP and LSP-DSSAT models capture the diurnal variations and
phases for net radiation (Figure 4-27(a)) throughout the growing season. The RMSDs
70
125 126 127 128 129 130 131 132 133 134 135−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
125 126 127 128 129 130 131 132 133 134 135
−300
−200
−100
0
100
200
300
Hea
t Flu
x (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-20. Comparison of soil heat flux, between DoY 125 to 135, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
between the LSP-DSSAT and observed net radiation are ∼ 24 W/m2. These differences
are close to the sensor uncertainty of 22 W/m2 in Table 4-7. The biases are ∼ 17 W/m2
indicate an overestimation. LE RMSDs of ∼48 W/m2 are what can be expected from
the Pareto front in Figure 4-3. Sudden increases in LE on DoY 93, 109, 119, and 127,
as shown in Figure 4-27(b), are due to high evaporation after rainfall or irrigation. The
RMSDs of ∼ 36 W/m2 for sensible heat flux (Figure 4-27(c)) are lower than those for LE.
The model overestimates the diurnal amplitude for 2 cm soil heat flux (Figure 4-27(d)),
which has LSP-DSSAT RMSDs of ∼ 47 W/m2, due to daytime overestimation of net
radiation and nighttime overestimation of latent and sensible heat fluxes.
The RMSD for VSM at 2 cm (Figure 4-28 and Table 4-5) is similar to our choice
of 0.04 m3/m3 on the overall season Pareto front (Figure 4-3). For both the LSP and
71
125 126 127 128 129 130 131 132 133 134 1350.05
0.1
0.15
0.2(a)
VS
M (
m3 /m
3 )
125 126 127 128 129 130 131 132 133 134 1350.05
0.1
0.15
0.2(b)
VS
M (
m3 /m
3 )
125 126 127 128 129 130 131 132 133 134 1350.05
0.1
0.15
0.2(c)
VS
M (
m3 /m
3 )
125 126 127 128 129 130 131 132 133 134 1350.05
0.1
0.15
0.2(d)
VS
M (
m3 /m
3 )
125 126 127 128 129 130 131 132 133 134 1350.05
0.1
0.15
0.2(e)
VS
M (
m3 /m
3 )
125 126 127 128 129 130 131 132 133 134 1350.05
0.1
0.15
0.2(f)
DoY 2004 (EST)
VS
M (
m3 /m
3 )
MicroWEX−2 LSP LSP−DSSAT
Figure 4-21. Comparison of volumetric soil moisture estimated by the coupledLSP-DSSAT and stand-alone LSP model simulation and those observedduring MicroWEX-2, between DoY 125 to 135: (a) 2 cm, (b) 4 cm, (c) 8 cm,(d) 32 cm, (e) 64 cm, and (f) 100 cm.
72
125 126 127 128 129 130 131 132 133 134 135
280
300
320
(a)Tem
p. (
K)
125 126 127 128 129 130 131 132 133 134 135
280
300
320
(b)Tem
p. (
K)
125 126 127 128 129 130 131 132 133 134 135
280
300
320
(c)Tem
p. (
K)
125 126 127 128 129 130 131 132 133 134 135
280
300
320
(d)Tem
p. (
K)
125 126 127 128 129 130 131 132 133 134 135
280
300
320
(e)Tem
p. (
K)
125 126 127 128 129 130 131 132 133 134 135
280
300
320
DoY 2004 (EST)
Tem
p. (
K)
(f)
MicroWEX−2 LSP LSP−DSSAT
Figure 4-22. Comparison of soil temperature estimated by the coupled LSP-DSSAT andstand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 125 to 135: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm.
73
135 140 145 150 155−200
0
200
400
600
800
1000
Net
Rad
iatio
n (W
/m2 )
(a)MicroWEX−2 LSP LSP−DSSAT
135 140 145 150 155
−300
−200
−100
0
100
200
300
Net
Rad
iatio
n (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-23. Comparison of net radiation, between DoY 135 to 154, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
LSP-DSSAT model simulations, the VSMs at all layers exhibit positive bias that increases
during the season. A bias of ∼0.02 m3/m3 could be introduced at the beginning of the
simulation due to improper initial conditions (Section 4.4.1) and significant uncertainty in
raingauge observations. During MicroWEX-2, the differences between daily accumulations
from the four raingauge observations and those observed independently by using
collection cans were up to 10s of mm/day. Previous studies have also found similarly
high uncertainties in precipitation, at 12 mm/h, using such raingauges [44].
The VSM bias of ∼ 0.06 m3/m3 for the layers 0.64 m and below (Figures 4-28 (e) and
(f)) could be due to the improper retention curve parameters in the clay layer (below 1.7
m). The parameters were based only on one soil sample from that layer and could have
resulted in lower flux estimates at the lower boundary and higher biases for the deeper
74
135 140 145 150 155−200
0
200
400
600
800
1000
Hea
t Flu
x (W
/m2 )
(a)
MicroWEX−2 LSP LSP−DSSAT
135 140 145 150 155
−300
−200
−100
0
100
200
300
Hea
t Flu
x (W
/m2 )
DoY 2004 (EST)
(b)
Figure 4-24. Comparison of soil heat flux, between DoY 135 to 154, estimated by thecoupled LSP-DSSAT and stand-alone DSSAT model simulation and thoseobserved during MicroWEX-2: (a) values and (b) residuals
layers. The decrease in drainage could also cause positive bias in VSM for the upper
layers, closer to the land surface.
Overall, soil temperatures (Figure 4-29) for both model simulations match closely
with the MicroWEX-2 observations. During the bare soil period, soil temperature exhibits
positive bias of < 1.40 K and this bias is reduced during the intermediate vegetation cover
period to < 0.91 K due to a net reduction of soil heat flux estimates. As the soil heat flux
bias increases, the temperature bias increases to < 2.7 K after DoY 125. The seasonal
RMSDs decrease with depth with a maximum of 2.43 K (Table 4-6).
4.6 Conclusion
This chapter answers research questions 3, 4, and 5 given in Chapter 1.
75
135 140 145 150 1550.05
0.1
0.15
0.2 (a)V
SM
(m
3 /m3 )
135 140 145 150 1550.05
0.1
0.15
0.2 (b)
VS
M (
m3 /m
3 )
135 140 145 150 1550.05
0.1
0.15
0.2 (c)
VS
M (
m3 /m
3 )
135 140 145 150 1550.05
0.1
0.15
0.2 (d)
VS
M (
m3 /m
3 )
135 140 145 150 1550.05
0.1
0.15
0.2 (e)
VS
M (
m3 /m
3 )
135 140 145 150 1550.05
0.1
0.15
0.2 (f)
DoY 2004 (EST)
VS
M (
m3 /m
3 )
MicroWEX−2 LSP LSP−DSSAT
Figure 4-25. Comparison of volumetric soil moisture estimated by the coupledLSP-DSSAT and stand-alone LSP model simulation and those observedduring MicroWEX-2, between DoY 135 to 154: (a) 2 cm, (b) 4 cm, (c) 8 cm,(d) 32 cm, (e) 64 cm, and (f) 100 cm.
76
135 140 145 150 155
280
300
320
(a)Tem
p. (
K)
135 140 145 150 155
280
300
320
(b)Tem
p. (
K)
135 140 145 150 155
280
300
320
(c)Tem
p. (
K)
135 140 145 150 155
280
300
320
(d)Tem
p. (
K)
135 140 145 150 155
280
300
320
(e)Tem
p. (
K)
135 140 145 150 155
280
300
320
DoY 2004 (EST)
Tem
p. (
K)
(f)
MicroWEX−2 LSP LSP−DSSAT
Figure 4-26. Comparison of soil temperature estimated by the coupled LSP-DSSAT andstand-alone LSP model simulation and those observed during MicroWEX-2,between DoY 135 to 154: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm,and (f) 100 cm.
77
80 90 100 110 120 130 140 150−200
0
200
400
600
800
1000
Flu
x (W
/m2 ) (b)
80 90 100 110 120 130 140 150
0
500
1000F
lux
(W/m
2 )
(a)
80 90 100 110 120 130 140 150−200
0
200
400
600
800
1000
Flu
x (W
/m2 ) (c)
80 90 100 110 120 130 140 150−200
0
200
400
600
800
1000
Flu
x (W
/m2 )
(d)
MicroWEX−2 LSP LSP−DSSAT
Figure 4-27. Comparison of fluxes estimated by the coupled LSP-DSSAT and stand-aloneLSP model simulation and those observed during MicroWEX-2: (a) netradiation, (b) latent heat flux, (c) sensible heat flux, and 2 cm soil heat flux.
78
80 90 100 110 120 130 140 1500.05
0.1
0.15
0.2(a)
VS
M (
m3 /m
3 )
80 90 100 110 120 130 140 1500.05
0.1
0.15
0.2(b)
VS
M (
m3 /m
3 )
80 90 100 110 120 130 140 1500.05
0.1
0.15
0.2(c)
VS
M (
m3 /m
3 )
80 90 100 110 120 130 140 1500.05
0.1
0.15
0.2(d)
VS
M (
m3 /m
3 )
80 90 100 110 120 130 140 1500.05
0.1
0.15
0.2(e)
VS
M (
m3 /m
3 )
80 90 100 110 120 130 140 1500.05
0.1
0.15
0.2(f)
VS
M (
m3 /m
3 )
DoY 2004 (EST)
MicroWEX−2 LSP LSP−DSSAT
Figure 4-28. Comparison of volumetric soil moisture estimated by the coupledLSP-DSSAT and stand-alone LSP model simulation and those observedduring MicroWEX-2: (a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and(f) 100 cm.
79
80 90 100 110 120 130 140 150
280
300
320
(a)Tem
p. (
K)
80 90 100 110 120 130 140 150
280
300
320
(b)Tem
p. (
K)
80 90 100 110 120 130 140 150
280
300
320
(c)Tem
p. (
K)
80 90 100 110 120 130 140 150
280
300
320
(d)Tem
p. (
K)
80 90 100 110 120 130 140 150
280
300
320
(e)Tem
p. (
K)
80 90 100 110 120 130 140 150
280
300
320
DoY 2004 (EST)
Tem
p. (
K)
(f)
MicroWEX−2 LSP LSP−DSSAT
Figure 4-29. Comparison of soil temperature estimated by the coupled LSP-DSSAT andstand-alone LSP model simulation and those observed during MicroWEX-2:(a) 2 cm, (b) 4 cm, (c) 8 cm, (d) 32 cm, (e) 64 cm, and (f) 100 cm.
80
Question 3:”What values of the twelve calibrated parameters give the
best LSP model performance for both latent heat flux and near surface soil
moisture for the MicroWEX-2 growing season?”
The calibrated values of the twelve parameters are given in Table 4-2.
Question 4:”How do the model estimates of soil moisture, temperature, and
surface fluxes compare with MicroWEX-2 observations?”
The RMSD for VSM at 2 cm is ∼ 0.04 m3/m3. For both the LSP and LSP-DSSAT
model simulations, the VSMs at all layers exhibit positive bias that increases during the
season. The seasonal RMSDs for temperature decrease with depth with a maximum of
2.43 K.
The RMSDs between the modeled and observed net radiation were ∼ 24 W/m2. LE
estimates had an RMSD of ∼ 48 W/m2, the sensible heat flux estimates had an RMSD of
∼ 36 W/m2, and the 2 cm soil heat flux estimates had RMSD of ∼ 47 W/m2.
Question 5:”What is the impact of coupling on both LSP and DSSAT model
estimates of LAI, biomass, soil moisture, temperature, and surface fluxes”
The estimates from the DSSAT and LSP-DSSAT differed by <0.2 for LAI and <0.6
kg/m2 for dry biomass, with the coupled LSP-DSSAT model estimating higher values than
the stand-alone DSSAT. The differences between the LSP and LSP-DSSAT estimates of
soil moisture, soil temperature, and surface fluxes are all small.
81
CHAPTER 5CANOPY MICROWAVE MODEL
5.1 Introduction
In this chapter a refractive model is developed for vegetation opacity of growing
sweet corn based upon moisture distribution in the canopy and incorporated into a
simple microwave brightness model linked with the coupled LSP-DSSAT model. The
refractive model developed by England and Galantowicz [19] was extended for sweet corn
using observed moisture distribution during the Fourth and Fifth Microwave Water and
Energy Balance Experiments (MicroWEX-4 and -5). The τ estimated by the model is
compared with that estimated using the Jackson model. The τ values obtained from the
two approximations were used in a microwave emission model at C-band and the model
estimates of brightness were compared with field observations.
5.2 Methodology
5.2.1 Moisture Distribution Measurements
Five measurements of moisture distribution were conducted during MicroWEX-4:
May 12 (Day After Planting (DAP) 63), May 17 (DAP 68), May 26 (DAP 77), June 2
(DAP 84), and June 6 (DAP 88). The samples collected on DAP 63 and 88 consisted of
plants in vegetative stage, i.e., before ear formation, while those collected on other days
consisted of plants at various reproductive stages. Additional plant sample was obtained
on DAP 88 to determine the density of wet vegetation (solid). Three measurements of
moisture distribution were conducted during MicroWEX-5: April 10 (DAP 32), May 1
(DAP 53), and May 15 (DAP 67). The samples collected on DAP 53 and 67 consisted of
plants in reproductive stages.
All representative plant samples were cut every 10 cm and weighed wet. The samples
were dried at 70o C for at least 48 hours and weighed to obtain dry biomass. The samples
on DAP 63, 2005 were cut every 5 cm to ensure that finer samples were not needed to
82
10 20 30 40 50 60 70 80 90
(a)
EarTotal
10 20 30 40 50 60 70 80 90Days After Planting
(b)
Figure 5-1. Observations of total and ear wet biomass during (a) MicroWEX-4 in 2005and (b) MicroWEX-5 in 2006.
obtain accurate moisture distribution. The density of vegetation material for each layer
was measured by volume displacement in a graduated cylinder.
Density of wet vegetation and air, ρ(z), called the cloud density, was calculated for
each layer as a ratio of wet biomass of each layer and the thickness of the layer (10 cm).
The mass of air is negligible. To obtain seasonal pattern, the cloud density of each layer
was plotted as a function of height of the layer, shown in Figure 5-3.
5.2.2 Canopy Opacity
The canopy opacity (τ) is estimated as [59, 60]:
τ =
∫ h
0
2 k0 κ(z) dz (5–1)
83
10 20 30 40 50 60 70 80 90
(a)
10 20 30 40 50 60 70 80 90
(b)
Days After Planting
Figure 5-2. Observations of canopy height during (a) MicroWEX-4 in 2005 and (b)MicroWEX-5 in 2006.
where h is canopy height (m), k0 is vacuum wavenumber (m−1), and κ(z) = −Imnt(z)(Np/m) is the absorption coefficient of the canopy. Imnt(z) is the imaginary part of the
complex refractive index, estimated as the sum of volume fraction of components,
nt(z) = 1 + vwcnwc vwc =ρ(z)
ρs
(5–2)
where, vwc is the volume fraction of the wet vegetation (m3/m3), nwc is the refractive
index of the wet vegetation , and ρs is the density of wet vegetation (697.72 kg/m3 for this
study [7]). Ulaby and El-Rayes’ model [57] estimates nwc as a function of frequency (6.7
GHz for this study) and moisture mixing ratio (Mg). Mg is defined as the ratio of weight
of water in the canopy to the weight of wet canopy. Figure 5-4 shows the mixing ratio
during MicroWEX-4 and -5. In this model, an isothermal canopy is assumed, so that the
84
κ(z) profiles can be integrated over the height of the canopy to obtain τ . The isothermal
assumption was appropriate for a short sweet corn canopy of 1.5m. The absolute difference
between the temperatures at the top and at the bottom of the canopy was < 4 K during
the simulation period.
5.2.3 Microwave Brightness Model
The microwave brightness (MB) model is a widely-used τ -ω model [59], in which the
total brightness temperature of a terrain (TB) is a sum of three contributions: TBs,p (from
the soil), TBc,p (from the canopy), and TBsky,p (from the sky).
0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
(a)
0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2Canopy Height (m)
(b)
DAP 32DAP 53DAP 67
DAP 63DAP 68DAP 77DAP 84DAP 88
Figure 5-3. Cloud densities measured during (a) MicroWEX-4 in 2005 and (b)MicroWEX-5 in 2006. The symbols and the lines represent the measurementsand the best curve-fits, respectively.
85
10 20 30 40 50 60 70 80 90
(a)
10 20 30 40 50 60 70 80 90
(b)
Days After Planting
Figure 5-4. Moisture mixing ratios measured during (a) MicroWEX-4 in 2005 and (b)MicroWEX-5 in 2006.
TBs,p = (1− rp)Teffexp(−τ/µ)
TBc,p = Tc[1− exp(−τ/µ)](1− ω)
× [1 + rpexp(−τ/µ)]
TBsky,p = Tskyrpexp(−2τ/µ)
(5–3)
where p is polarization, rp is the reflectivity of the rough soil surface, Teff is the
effective radiating temperature of the soil calculated using the first order approximation
from [18] (K), µ = cos(θ) where θ is the look angle (50o for MicroWEX-5), Tc is the
physical temperature of the isothermal canopy (K), measured during the experiments, ω is
the single scattering albedo, and Tsky is the sky brightness (assumed 5 K at C-band). In
this model, rp is based upon the semi-empirical model of Wegmuller and Matzler [63]:
86
rH = |ΓH |2e−(k0σ)√
0.1cos(θ)
rV = rHcos(θ)0.655
(5–4)
where ΓH is the H-polarized Fresnel coefficient, k0 is the vacuum wavenumber, θ is
the look angle, and σ is the surface roughness height, set to 0.0005 m [27]. Soil dielectric
properties are determined using a four component mixing model following Dobson et al
[13].
5.2.4 Model Comparison and Evaluation
Using the ρ(z), τ is obtained for the MicroWEX-4 and -5 growing seasons. The
estimates for τ are compared with those obtained using the Jackson model [51] as:
τ = bWc (5–5)
where, b is an empirical parameter and Wc is the water content in the canopy (kg/m2).
The τ from the biophysical model and from the Jackson model are evaluated in the
MB model during the latter part of the MicroWEX-5 season. The MB model simulated
TB for ten days (DAP 42-52), with DAP 42-47 during vegetative growth and DAP 47-52
during ear formation. The canopy cover was 100% during the period of simulation. The
MB model was driven with observed canopy and soil temperatures and moisture values.
The MB model was linked to the LSP-DSSAT model, which provides it with soil
temperature and moisture profiles as well as canopy properties used for calculating canopy
transmission and scattering, such as height, vegetation cover, and vegetative and ear
biomass. Using the same initial conditions, inputs, and parameters obtained for the
calibrated LSP-DSSAT model in Chapter 4, the LSP-DSSAT-MB model simulated H-pol
TB for the MicroWEX-2 growing season.
87
Table 5-1. Values of the Coefficients in equations 5–6 and 5–7
Coefficients Valuesa 2.054b -2.054αc -114.32αd 5.87αe -1.23βc 25.69βd -1.37βe 0.34γc 8.41γd 0.29γe -0.07
5.3 Results and Discussion
5.3.1 Moisture Distribution Function
As shown in Figure 5-3, the cloud density function consists of two terms, a linear
term representing the vegetative stage of the plant and a gaussian term representing the
moisture in the ear during the reproductive stages, as:
ρ(z) =Bv
h(a+ bhn) + c
Be
hexp
[−1
2
(hn − d
e
)2](5–6)
where a, b, c, d, and e are fitted parameters, hn = z/h is the normalized height, and Bv
and Be are the wet biomass of vegetation (stem and leaves) and ear (kg/m2), respectively.
Figure 5-3 also shows the best curve-fits obtained for each sample. The parameters c, d,
and e, governing the gaussian term, were estimated as quadratic functions of dry biomass
of the ear (Dear) as:
c = αc + βcDear + γcD2ear
d = αd + βdDear + γdD2ear
e = αe + βeDear + γeD2ear
(5–7)
Table 5-1 gives the values of the a and b parameters and the coefficients in equation 5–7.
88
10 20 30 40 50 60 70 80 90
10 20 30 40 50 60 70 80 90Days After Planting
Our τ model (with ears)Our τ model (without ears)Jackson model
Figure 5-5. Comparison of τ calculated using the biophysical τ model (with and withoutthe gaussian term) and that using the Jackson model during (a) MicroWEX-4in 2005, and (b) MicroWEX-5 and 2006.
5.3.2 Canopy Opacity
Figure 5-5 shows the τ estimated using the biophysical model and the Jackson model
with b = 0.25. The Jackson model estimates lower opacities throughout the growing
season compared to those obtained using the biophysical τ model with root mean square
differences (RMSD) between the two models of 0.16 Np during MicroWEX-4 and 0.23 Np
during MicroWEX-5. However, the Jackson model matched better when the change in
the moisture distribution due to ear formation was not included, with RMSDs of 0.10 Np
during MicroWEX-4 and 0.11 Np during MicroWEX-5. The contribution of moisture in
the ears to the optical depth is significant because they comprise a significant portion of
the total biomass (see Figure 5-1), with the increase in biomass primarily due to growth
89
in ears once corn reaches the reproductive stage. As a result, Figure 5-5 shows a sharp
increase in optical depth at the onset of ear development, at DAP 62 for MicroWEX-4 and
DAP 47 for MicroWEX-5. By the end of the seasons, the optical depth is doubled when
ears are included.
5.3.3 Microwave Brightness
Figure 5-6 shows the comparison of the horizontally polarized (H-pol) TB observed
during MicroWEX-5 with those simulated by the MB model at C-band, with τ estimates
using the biophysical model and the Jackson model. Only H-pol brightness is examined
here because H-pol brightness is more sensitive to changes in soil moisture than V-pol, at
the incidence angle of 50o, that is close to the Brewster angle at microwave frequencies
[59]. The observed TB increased during the drydown from DAP 42 to DAP 46.7 and then
43 44 45 46 47 48 49 50 51 52Days After Planting (EST)
MB model (our τ)MB model (Jackson τ)MicroWEX−5 Observations
Figure 5-6. Comparison of the observed TB at H-pol during MW5 those simulated by theMB model using τ from the biophysical model and from the Jackson modelduring late-season MicroWEX-5.
90
Table 5-2. RMS differences between observed TB during MicroWEX-5 and those estimatedby the MB model
RMSD (K)τ model DAP < 47 DAP ≥ 47 DAP 42-52
Jackson (ω = 0.00) 5.84 12.50 9.74Jackson (ω = 0.06 for DAP ≥ 47) 5.84 3.65 4.88
Biophysical ω = 0.05 for 42<DAP<52 5.00 8.25 6.83Biophysical ω = 0.075 for DAP ≥ 47 5.00 5.22 5.13
decreased by 30 K due to an irrigation event. The TB at 6.7 GHz were sensitive to soil
moisture changes even when the canopy cover was 100% and biomass was 2.7 kg/m2 (see
Figure 5-1).
A small value for single-scattering albedo (ω) was included in the MB model when
using the biophysical τ estimates. The value of 0.05 before ear formation (DAP 47) and
0.075 after DAP 47 provided the least RMSD (see Table 5-2).
In the Jackson model, b = 0.25, similar to the literature-based values for corn [61],
provided the lowest RMSD. Typically ω is set to zero in the Jackson model [51], but it was
found that the TB using the Jackson model was overestimated after ear formation, with an
RMSD of 12.50 K. Including ω = 0.06 after ear formation in the Jackson model reduced
the RMSD to 3.65 K,as shown in Table 5-2. The values of ω needed to provide the least
RMSD for both τ models were small, < 0.1, implying that single scattering is sufficient to
provide realistic TB estimates for the mature sweet corn canopy and multiple scattering is
not needed. The overall RMSD between observed TB and the modeled TB using the two
τ models were similar, with 5.13 K for the biophysical model and 4.88 K for the Jackson
model (see Table 5-2).
91
8085
9095
100
105
110
115
120
125
140
160
180
200
220
240
260
280
300
320
H−pol Brightness Temp. (K)
(a)
8085
9095
100
105
110
115
120
125
140
160
180
200
220
240
260
280
300
320
H−pol Brightness Temp. (K)
(b)
DoY
200
4 (E
ST
)
M
icro
WE
X−
2LS
P−
DS
SA
T−
MB
Fig
ure
5-7.
Com
par
ison
ofm
icro
wav
ebri
ghtn
ess,
esti
mat
edby
the
LSP
-DSSA
T-M
Bm
odel
wit
hsp
ecula
rsu
rfac
e(a
)an
dW
egm
uller
and
Mat
zler
(b),
and
C-b
and
mic
row
ave
bri
ghtn
ess
obse
rved
duri
ng
Mic
roW
EX
-2,bef
ore
DoY
125.
92
125
130
135
140
145
150
155
180
200
220
240
260
280
300
320
H−pol Brightness Temp. (K)
(a)
125
130
135
140
145
150
155
180
200
220
240
260
280
300
320
H−pol Brightness Temp. (K)
(b)
DoY
200
4 (E
ST
)
Mic
roW
EX
−2
LSP
−D
SS
AT
−M
B
Fig
ure
5-8.
Com
par
ison
ofm
icro
wav
ebri
ghtn
ess,
esti
mat
edby
the
LSP
-DSSA
T-M
Bm
odel
wit
hsp
ecula
rsu
rfac
e(a
)an
dW
egm
uller
and
Mat
zler
(b),
and
C-b
and
mic
row
ave
bri
ghtn
ess
obse
rved
duri
ng
Mic
roW
EX
-2,af
ter
DoY
125.
93
Table 5-3. RMS differences between observed H-pol TB during MicroWEX-2 and thoseestimated by the MB model.
rp model RMSD (K) MAD (K) Bias (K)Specular soil (DoY < 125) 35.87 28.94 -25.70
Wegmuller and Matzler (DoY < 125) 32.18 23.78 14.43Specular soil (DoY ≥ 125) 10.06 8.15 6.58
Wegmuller and Matzler (DoY ≥ 125) 12.43 10.83 9.97
During less than full vegetation cover (before DoY 125), the soil reflectivity strongly
affects the estimation of brightness. This leads to a wide disparity between the specular
and Wegmuller and Matzler rough surface model estimates, as can be seen in Figure 5-7.
The lower reflectivity of the rough surface model leads to higher brightness values than
the specular model. Sudden drops in brightness (DoY 98, 100, 104, 107, 109, 112, 114,
119, 122, 123, and 124) due to irrigation or precipitation events are only reached with
the specular model. As vegetation cover increases, the canopy contribution to brightness
increases so the specular and rough surface models’ estimates of brightness approach
eachother. Overall, the performance when vc < 1 is poor, as seen by the high RMSDs
Table 5-3. Neither reflectivity model matched sudden drops in brightness, and there is also
an underestimation due to the overestimation of soil moisture by the LSP model (Chapter
4).
During full vegetation cover (after DoY 125), model estimates of brightness are
dominated by the canopy contribution and thus by τ and ω. Both surface reflectivity
models give similar results and overestimate brightness, seen in Figure 5-8 and the RMSDs
in Table 5-3. This could be an indication that the ω values found for MicroWEX-5 are
not correct for MicroWEX-2. After modeled ear formation on DoY 139 brightness is less
overestimated as ω is increased to 0.075. This late in the season, there is almost no effect
from the soil, and as the τ model is biophysically based, the only way to improve model
estimates here would be to calibrate ω before and after ear formation.
5.4 Summary
This chapter answers the research question 6 and 7 outlined in Chapter 1.
94
Question 6:”How does a physically-based τ model compare to Jackson’s
widely-used empirical model?”.
The τ obtained from the biophysical model estimated higher values than the Jackson,
with an RMSD between the two of up to 0.23 Np. The τ values obtained from the two
approximations were used in a microwave emission model at C-band, the model estimates
of TB matched well with observations using both τ values when ω is included, with similar
RMSDs of ∼ 5 K.
Question 7:”How do the brightness estimates predicted by the linked LSP-
DSSAT-MB model compare to observations during MicroWEX-2?”
Preliminary results indicate the MB model is lacking in two main areas, the roughness
model and the ω model. For the first half of the season, where bare soil brightness is more
important, the constant roughness or specular surface models over- and under-estimate
brightness, respectively, both with RMSDs ∼ 33 K. During the later half of MicroWEX-2,
brightness is overestimated with RMSD of ∼ 11 K.
95
CHAPTER 6CONCLUSION
In this chapter, the results and contributions from this thesis are summarized and
reccomendations for future research are provided.
6.1 Summary
This thesis provides important insights into crop, SVAT, and microwave brightness
modeling for growing vegetation. Three season-long extensive field experiments (MicroWEX-2,
4, and 5) were conducted, monitoring radiobrightness, soil moisture, soil temperature,
surface fluxes, and crop growth for sweet corn. These experiments provided the datasets
used in forcing, developing, and calibrating the models.
First, a crop model and SVAT model were calibrated and coupled. The crop model
(CERES-Maize) was calibrated with simulated annealing using field observations for the
MicroWEX-2 site. The calibration was performed by minimizing the residuals for LAI
and biomass, the two most important canopy parameters in determining the microwave
signature of a vegetation canopy. The SVAT model (LSP) was calibrated with Latin
Hypercube Sampling to provide the least RMSD in LE with an RMSD in VSM at 2 cm of
∼0.04 m3/m3, using observations during MicroWEX-2. The LSP and DSSAT models were
coupled such that the LSP replaced the DSSAT soil and soil-plant-atmosphere modules
while DSSAT provides LSP with LAI, biomass, height, width, and root length density.
Model estimates of surface fluxes, VSM, and soil temperature were very similar using both
the coupled LSP-DSSAT and stand-alone LSP that used observed vegetation parameters.
Second, a microwave transmission model was developed and compared with the
widely-used empirical Jackson model, and with observations of of microwave brightness
for a period during MicroWEX-5. This τ model was incorporated in a MB linked with
the coupled LSP-DSSAT model, and tested for the MicroWEX-2 growing season.
The τ obtained from the biophysical model estimated higher values than the Jackson,
with an RMSD between the two of up to 0.23 Np. The τ values obtained from the two
96
approximations were used in a microwave emission model at C-band, the model estimates
of TB matched well with observations during MicroWEX-5, using both τ values when ω is
included, with similar RMSDs.
The brightness temperatures predicted by the linked LSP-DSSAT-MB model
during the first half of the MicroWEX-2tested for MicroWEX-2, for the first half of
the MicroWEX-2 season were higher than those observed when the Wegmuller and
Matzler reflectivity model was used and were significantly lower than observations when
a specular model was used. In addition, overestimation of moisture by the LSP model
lead to underestimation of brightness. Later in the MicroWEX-2 season, brightness is
overestimated when using the ω values found for MicroWEX-5, suggesting they are too
low.
6.2 Contributions
One of the major contributions of this thesis is the development and calibration of
the coupled SVAT-Crop model as well as the development of the physically-based canopy
transmission model for sweet corn. The techniques used to couple the LSP and DSSAT
models can be extended to other SVAT-Crop combinations; likewise, the methodology for
developing the optical depth model for sweet corn can be extended to other plant types, as
has been done for cotton during MicroWEX-6 [67].
Other significant contributions are the extensive datasets of soil temperature, soil
moisture, vegetation, surface fluxes, and radiobrightness collected during MicroWEX-2,
4, and 5. They provide season-long and high temporal resolution observations to allow
interdisciplinary studies.
6.3 Recommendations for Future Research
As seen in Chapter 4, the LSP-DSSAT model overestimates soil moisture, largely
due to uncertainty in soil hydrologic properties and in precipitation. This indicates that
the model estimates would improve with a calibration of the soil hydrologic parameters
in addition to the twelve parameters calibrated in Chapter 4. In addition, since a major
97
source of uncertainty in the model is the precipitation input, model estimates of soil
moisture are likely to improve from a data assimilation method which takes into account
the uncertainty in inputs and parameters, such as Kalman filtering.
Before the LSP-DSSAT-MB model can be used in a data assimilation scheme, the
rough soil reflectivity model in the MB model needs to be improved. As is shown in
Section 5.3.3, from the high brightness RMSDs during the first half of the season, either
the specular (Fresnel) reflectivity or the rough surface reflectivity alone are insufficient
to match the sudden drops in brightness associated with precipitation events. This is a
challenge because of the extremely limited bare soil brightness data during MicroWEXs
2, 4, and 5. To fill the dearth of bare soil data, bare soil tests were conducted during
May and June 2007 in which extensive soil roughness measurements were taken along
with brightness measurements, before, during, and after irrigation events. This data
would be useful in the future for the development of a more rigorous rough surface
reflectivity model. A moisture-dependent roughness model could capture the sudden drops
in brightness associated with precipitation events but needs to be refined.
In addition, the LSP-DSSAT-MB model overestimated brightness in the later
half of the MicroWEX-2 season, indicating that the ω values need to be higher for the
MicroWEX-2, and that they should be calibrated. The optimal ω values for MicroWEX-2
and MicroWEX-5 are apparently different, indicating that there is some difference between
the canopies of the two seasons that would produce a difference in ω. Future research
could find some physical relationship between canopy characteristics such as leaf or stem
biomass and ω, similar to the physical relationship found for τ .
98
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