1 / 56

GEOGG121: Methods Inversion I : linear approaches

GEOGG121: Methods Inversion I : linear approaches. Dr. Mathias (Mat) Disney UCL Geography Office: 113, Pearson Building Tel: 7670 0592 Email: mdisney@ucl.geog.ac.uk www.geog.ucl.ac.uk /~ mdisney. Lecture outline. Linear models and inversion Least squares revisited, examples

rippeon
Télécharger la présentation

GEOGG121: Methods Inversion I : linear approaches

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. GEOGG121: MethodsInversion I: linear approaches Dr. Mathias (Mat) Disney UCL Geography Office: 113, Pearson Building Tel: 7670 0592 Email: mdisney@ucl.geog.ac.uk www.geog.ucl.ac.uk/~mdisney

  2. Lecture outline • Linear models and inversion • Least squares revisited, examples • Parameter estimation, uncertainty • Practical examples • Spectral linear mixture models • Kernel-driven BRDF models and change detection

  3. Reading • Linear models and inversion • Linear modelling notes: Lewis, 2010 • Chapter 2 of Press et al. (1992) Numerical Recipes in C (online version http://apps.nrbook.com/c/index.html) • http://en.wikipedia.org/wiki/Linear_model • http://en.wikipedia.org/wiki/System_of_linear_equations

  4. Linear Models • For some set of independent variables x = {x0, x1, x2, … , xn} have a model of a dependent variable y which can be expressed as a linear combination of the independent variables.

  5. Linear Models?

  6. Linear Mixture Modelling • Spectral mixture modelling: • Proportionate mixture of (n) end-member spectra • First-order model: no interactions between components

  7. Linear Mixture Modelling • r = {rl0, rl1, … rlm, 1.0} • Measured reflectance spectrum (m wavelengths) • nx(m+1) matrix:

  8. Linear Mixture Modelling • n=(m+1) – square matrix • Eg n=2 (wavebands), m=2 (end-members)

  9. r1 r2 Reflectance Band 2 r r3 Reflectance Band 1

  10. 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

  11. 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)

  12. Error Minimisation • Set (partial) derivatives to zero

  13. Error Minimisation • Can write as: Solve for P by matrix inversion

  14. e.g. Linear Regression

  15. RMSE

  16. x x1 x2 y x

  17. Weight of Determination (1/w) • Calculate uncertainty at y(x)

  18. P1 RMSE P0

  19. P1 RMSE P0

  20. Issues • Parameter transformation and bounding • Weighting of the error function • Using additional information • Scaling

  21. Parameter transformation and bounding • Issue of variable sensitivity • E.g. saturation of LAI effects • Reduce by transformation • Approximately linearise parameters • Need to consider ‘average’ effects

  22. Weighting of the error function • Different wavelengths/angles have different sensitivity to parameters • Previously, weighted all equally • Equivalent to assuming ‘noise’ equal for all observations

  23. Weighting of the error function • Can ‘target’ sensitivity • E.g. to chlorophyll concentration • Use derivative weighting (Privette 1994)

  24. Using additional information • Typically, for Vegetation, use canopy growth model • See Moulin et al. (1998) • Provides expectation of (e.g.) LAI • Need: • planting date • Daily mean temperature • Varietal information (?) • Use in various ways • Reduce parameter search space • Expectations of coupling between parameters

  25. Scaling • Many parameters scale approximately linearly • E.g. cover, albedo, fAPAR • Many do not • E.g. LAI • Need to (at least) understand impact of scaling

  26. LAI 1 LAI 4 LAI 0 Crop Mosaic

  27. LAI 1 LAI 4 LAI 0 Crop Mosaic • 20% of LAI 0, 40% LAI 4, 40% LAI 1. • ‘real’ total value of LAI: • 0.2x0+0.4x4+0.4x1=2.0. visible: NIR

  28. canopy reflectance over the pixel is 0.15 and 0.60 for the NIR. • If assume the model above, this equates to an LAI of 1.4. • ‘real’ answer LAI 2.0

  29. 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

  30. Satellite, Day 1 Satellite, Day 2 X

  31. AVHRR NDVI over Hapex-Sahel, 1992

  32. Model parameters: Isotropic Volumetric Geometric-Optics Linear BRDF Model • of form:

  33. Model Kernels: Volumetric Geometric-Optics Linear BRDF Model • of form:

  34. Volumetric Scattering • Develop from RT theory • Spherical LAD • Lambertian soil • Leaf reflectance = transmittance • First order scattering • Multiple scattering assumed isotropic

  35. Volumetric Scattering • If LAI small:

  36. Similar approach for RossThick Volumetric Scattering • Write as: RossThin kernel

  37. Geometric Optics • Consider shadowing/protrusion from spheroid on stick (Li-Strahler 1985)

  38. Geometric Optics • Assume ground and crown brightness equal • Fix ‘shape’ parameters • Linearised model • LiSparse • LiDense

  39. Retro reflection (‘hot spot’) Kernels Volumetric (RossThick) and Geometric (LiSparse) kernels for viewing angle of 45 degrees

  40. Kernel Models • Consider proportionate (a) mixture of two scattering effects

  41. Using Linear BRDF Models for angular normalisation • Account for BRDF variation • Absolutely vital for compositing samples over time (w. different view/sun angles) • BUT BRDF is source of info. too! MODIS NBAR (Nadir-BRDF Adjusted Reflectance MOD43, MCD43) http://www-modis.bu.edu/brdf/userguide/intro.html

  42. MODIS NBAR (Nadir-BRDF Adjusted Reflectance MOD43, MCD43) http://www-modis.bu.edu/brdf/userguide/intro.html

  43. And uncertainty via 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

  44. Linear BRDF Models to track change 220 days of Terra (blue) and Aqua (red) sampling over point in Australia, w. sza (T: orange; A: cyan). • Examine change due to burn (MODIS) Time series of NIR samples from above sampling FROM: http://modis-fire.umd.edu/Documents/atbd_mod14.pdf

  45. MODIS Channel 5 Observation DOY 275

  46. MODIS Channel 5 Observation DOY 277

  47. Detect Change • Need to model BRDF effects • Define measure of dis-association

  48. MODIS Channel 5 Prediction DOY 277

  49. MODIS Channel 5 Discrepency DOY 277

More Related