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Shedding Light on the Weather
Srinivasa Narasimhan and Shree Nayar Computer Science Department Columbia University IEEE CVPR Conference June 2003, Madison, USA Sponsors : DARPA Human ID, NSF
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Computer Vision in Bad Weather
Mild Haze Dense Haze Computed Dehazed Image 3D Visualization Removing Weather Structure from Weather Color Contrast Polarization Models Algorithms (Narasimhan , Nayar ’00) (Narasimhan , Nayar ’01) (Narasimhan , Nayar ’02) (Schechner et. al. ’01)
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Light Sources in Bad Weather
Mist Fog
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Multiple Scattering in the Atmosphere
Phase Function Incident Beam Particle Light Source A T M O S P H E R E Imaging Plane Glow Pinhole
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Radiance Rate of Change
Radiative Transfer Infinitesimal Scattering Volume : Direction Exiting Beam Radiance dR Incident Beam Radiance Extinction Radiative Transfer Equation : Radiance Rate of Change Source Function Phase Function Optical Thickness
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Light Source in a Spherical Medium
Spherical Radiative Transfer Equation : Phase Function Light Field Cosine of Angle Optical Thickness [ Chandrasekhar 1960 ] Scattered Isotropic Source Homogeneous Medium
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Axially Symmetric Phase Functions
Exiting Direction Incident Direction Legendre Polynomial Expansion : [ Ishimaru 1997 ] [ Henyey et al., 1941 ] Legendre Polynomial Forward Scattering Parameter
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Light Source in a Spherical Medium
Scattered Light Field Isotropic Source Homogeneous Medium Spherical Radiative Transfer Equation : [ Chandrasekhar 1960 ] Cosine of Angle Optical Thickness Light Field Phase Function
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Analytic Multiple Scattering Solution
Scattered Light Field : Legendre Polynomial Phase Function Parameter Optical Thickness Exponential Coefficients : Source Radiant Intensity
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Highlights of the Model
Single and Multiple Scattering Absorbing and Purely Scattering Media Isotropic and Anisotropic Phase Functions T m 160 120 60 30 10 Small Number of Coefficients (m) :
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Scattered Light Field vs. Weather Condition
Angular PSF : Scattered Light Field at a Point Mild Weather (T = 1.2) Dense Weather (T = 4)
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Validation : Multiple Scattering in Milk
Image acquired With No Milk Original Milk Images Increasing Milk Concentrations Rendered Milk Images
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Model Fit Accuracy Low Milk Concentration High Milk Concentration
Number of Milk Concentrations : Model Fitting Error : [ 1 % to 3 % ] Diffusion Fitting Error : [ 20 % to 50 % ]
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Rendering Glows using Convolution
Increasing Fog Rendered Images Original Image Joint work with Ramamoorthi (submitted to TOG)
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Single versus Multiple Scattering
Single Scattering Original Image Multiple Scattering (Mild Condition) Multiple Scattering (Dense Condition) Joint work with Ramamoorthi (submitted to TOG)
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Inverse RTE : Weather from APSF
Measured APSF : Objective Function : Meteorological Visibility : [ Middleton 1952] Weather Condition : [ Van de Hulst 1957] 1 Pure Air Small Aerosols Haze Mist Fog Rain 0.1 0.4 0.7 0.9 0.8
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Atmospheric Visibilities
A Camera-based Weather Station 45 images of a light source (WILD Database ECCV 02) Computed Atmospheric Visibilities Estimated Ground Truth Computed Weather Conditions Estimated Ground Truth
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Active Visibility Meter for Ground Truth
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Summary Analytic Multiple Scattering Model Validation using Milk
Volume Rendering as Convolution Shedding Light on the Weather
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Prior Work on Radiative Transfer
[ Chandrasekhar 1960 , Ishimaru 1997 ] Sun Distant Source Plane Parallel Medium Scattered Light Field Our Problem : Divergent Source Inside Medium
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Scattering Space of Weather Conditions
Phase Function Parameter, q Single Scattering 1 Diffusion Pure Air Small Aerosols Haze Mist Fog 10 Optical Thickness, T
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Axially Symmetric Phase Functions
Exiting Direction Incident Direction Legendre Polynomial Expansion : [ Ishimaru 1997 ] Legendre Polynomial Henyey – Greenstein Function : [ Henyey, Greenstein 1941 ] Forward Scattering Parameter
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Effect of Source Visibility
315 240 180 90 30 o Increasing Milk Concentrations Observed Milk Images
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Scattering is Everywhere…
Computer Vision Astronomy Oceanography Medical Imaging Computer Graphics
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