Lumped Parameter Modelling UoL MSc Remote Sensing Dr Lewis
Introduction introduce simple lumped parameter models Build on RT modelling RT: formulate for biophysical parameters –LAI, leaf number density, size etc –investigate eg sensitivity of a signal to canopy properties e.g. effects of soil moisture on VV polarised backscatter or Landsat TM waveband reflectance –Inversion? Non-linear, many parameters
Linear Models For some set of independent variables x = {x 0, x 1, x 2, …, x n } have a model of a dependent variable y which can be expressed as a linear combination of the independent variables.
Linear Models?
Linear Mixture Modelling Spectral mixture modelling: –Proportionate mixture of (n) end-member spectra –First-order model: no interactions between components
Linear Mixture Modelling r = {r, r, … r m, 1.0} –Measured reflectance spectrum (m wavelengths) nx(m+1) matrix:
Linear Mixture Modelling n=(m+1) – square matrix Eg n=2 (wavebands), m=2 (end-members)
Reflectance Band 1 Reflectance Band r
Linear Mixture Modelling as described, is not robust to error in measurement or end-member spectra; Proportions must be constrained to lie in the interval (0,1) –- effectively a convex hull constraint; m+1 end-member spectra can be considered; needs prior definition of end-member spectra; cannot directly take into account any variation in component reflectances –e.g. due to topographic effects
Linear Mixture Modelling in the presence of Noise Define residual vector minimise the sum of the squares of the error e, i.e. Method of Least Squares (MLS)
Error Minimisation Set (partial) derivatives to zero
Error Minimisation Can write as: Solve for P by matrix inversion
e.g. Linear Regression
RMSE
y x xx1x1 x2x2
Weight of Determination (1/w) Calculate uncertainty at y(x)
Lumped Canopy Models Motivation –Describe reflectance/scattering but dont need biophysical parameters Or dont have enough information –Examples Albedo Angular normalisation – eg of VIs Detecting change in the signal Require generalised measure e.g cover When can calibrate model –Need sufficient ground measures (or model) and to know conditions
Model Types Empirical models –E.g. polynomials –E.g. describe BRDF by polynomial –Need to guess functional form –OK for interpolation Semi-empirical models –Based on physical principles, with empirical linkages –Right sort of functional form –Better behaviour in integration/extrapolation (?)
Linear Kernel-driven Modelling of Canopy Reflectance Semi-empirical models to deal with BRDF effects –Originally due to Roujean et al (1992) –Also Wanner et al (1995) –Practical use in MODIS products BRDF effects from wide FOV sensors –MODIS, AVHRR, VEGETATION, MERIS
Satellite, Day 1 Satellite, Day 2 X
AVHRR NDVI over Hapex-Sahel, 1992
Linear BRDF Model of form: Model parameters: Isotropic Volumetric Geometric-Optics
Linear BRDF Model of form: Model Kernels: Volumetric Geometric-Optics
Volumetric Scattering Develop from RT theory –Spherical LAD –Lambertian soil –Leaf reflectance = transmittance –First order scattering Multiple scattering assumed isotropic
Volumetric Scattering If LAI small:
Volumetric Scattering Write as: RossThin kernel Similar approach for RossThick
Geometric Optics Consider shadowing/protrusion from spheroid on stick (Li-Strahler 1985)
Geometric Optics Assume ground and crown brightness equal Fix shape parameters Linearised model –LiSparse –LiDense
Kernels Retro reflection (hot spot) Volumetric (RossThick) and Geometric (LiSparse) kernels for viewing angle of 45 degrees
Kernel Models Consider proportionate ( ) mixture of two scattering effects
Using Linear BRDF Models for angular normalisation
BRDF Normalisation Fit observations to model Output predicted reflectance at standardised angles –E.g. nadir reflectance, nadir illumination Typically not stable –E.g. nadir reflectance, SZA at local mean And uncertainty via
Linear BRDF Models for albedo Directional-hemispherical reflectance –can be phrased as an integral of BRF for a given illumination angle over all illumination angles. –measure of total reflectance due to a directional illumination source (e.g. the Sun) –sometimes called black sky albedo. –Radiation absorbed by the surface is simply 1-
Linear BRDF Models for albedo
Similarly, the bi-hemispherical reflectance –measure of total reflectance over all angles due to an isotropic (diffuse) illumination source (e.g. the sky). –sometimes known as white sky albedo
Spectral Albedo Total (direct + diffuse) reflectance –Weighted by proportion of diffuse illumination Pre-calculate integrals – rapid calculation of albedo
Linear BRDF Models to track change E.g. Burn scar detection Active fire detection (e.g. MODIS) –Thermal –Relies on seeing active fire –Miss many –Look for evidence of burn (scar)
Linear BRDF Models to track change Examine change due to burn (MODIS)
MODIS Channel 5 Observation DOY 275
MODIS Channel 5 Observation DOY 277
Detect Change Need to model BRDF effects Define measure of dis-association
MODIS Channel 5 Prediction DOY 277
MODIS Channel 5 Discrepency DOY 277
MODIS Channel 5 Observation DOY 275
MODIS Channel 5 Prediction DOY 277
MODIS Channel 5 Observation DOY 277
Single Pixel
Detect Change Burns are: –negative change in Channel 5 –Of long (week) duration Other changes picked up –E.g. clouds, cloud shadow –Shorter duration –or positive change (in all channels) –or negative change in all channels
Day of burn
Other Lumped Parameter Optical Models Modified RPV (MRPV) model –Multiplicative terms describing BRDF shape –Linearise by taking log
Other Lumped Parameter Optical Models Gilabert et al. –Linear mixture model Soil and canopy: f = exp(-CL) Parametric model of multiple scattering
Conclusions Developed semi-empirical models –Many linear (linear inversion) –Or simple form Lumped parameters –Information on gross parameter coupling –Few parameters to invert
Conclusions Uses of models –E.g. linear, kernel driven –When dont need full biophysical parameterisation Forms of models –Similar forms (from RT theory) Applications: –BRDF normalisation –Albedo –Change detection