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Multispectral Image Invariant to Illumination Colour, Strength, and Shading
Mark S. Drew and Amin Yazdani Salekdeh School of Computing Science, Simon Fraser University, Vancouver, BC, Canada
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Table of Contents Introduction RGB Illumination Invariant
Multispectral Image Formation Synthetic Multispectral Images Measured Multispectral Images Conclusion
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New Introduction Invariant Images – RGB:
Information from one pixel, with calibration Information from all pixels – use entropy New Multispectral data: Information from one pixel without calibration, but knowledge of narrowband sensors peak wavelengths
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RGB Illumination Invariant
Removing Shadows from Images, ECCV 2002 Graham Finlayson, Steven Hordley, and Mark Drew 4
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An example, with delta function sensitivities
RGB… An example, with delta function sensitivities B W R Y G P Narrow-band (delta-function sensitivities) Log-opponent chromaticities for 6 surfaces under 9 lights
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Deriving the Illuminant Invariant
RGB… Deriving the Illuminant Invariant Log-opponent chromaticities for 6 surfaces under 9 lights Rotate chromaticities This axis is invariant to illuminant colour
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An example with real camera data
RGB… An example with real camera data Normalized sensitivities of a SONY DXC-930 video camera Log-opponent chromaticities for 6 surfaces under 9 different lights
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Deriving the invariant
RGB… Deriving the invariant Log-opponent chromaticities Rotate chromaticities The invariant axis is now only approximately illuminant invariant (but hopefully good enough)
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Image Formation Multispectral
Illumination : motivate using theoretical assumptions, then test in practice Planck’s Law in Wien’s approximation: Lambertian surface S(), shading is , intensity is I Narrowband sensors qk(), k=1..31, qk()=(-k) Specular: colour is same as colour of light (dielectric):
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Multispectral Image Formation …
To equalize confidence in 31 channels, use a geometric-mean chromaticity: Geometric Mean Chromaticity: with
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Multispectral Image Formation …
surface-dependent sensor-dependent illumination-dependent So take a log to linearize in (1/T) ! 11
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Multispectral Image Formation …
Logarithm: known because, in special case of multispectral, *know* k ! Only sensor-unknown is ! ( spectral-channel gains)
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Multispectral Image Formation …
If we could identify at least one specularity, we could recover log k ?? Nope, no pixel is free enough of surface colour . So (without a calibration) we won’t get log k, but instead it will be the origin in the invariant space. Note: Effect of light intensity and shading removed: D 30-D Now let’s remove lighting colour too: we know 31- vector (ek – eM) (-c2/k - c2/M) Projection to (ek – eM) removes effect of light, 1/T : 30D 29-D
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Algorithm: Form 31-D chromaticity k Take log
Project to (ek – eM) using projector Pe
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What’s different from RGB?
Algorithm: What’s different from RGB? For RGB have to get “lighting-change direction” (ek – eM) either from calibration, or internal evidence (entropy) in the image. For multispectral, we know (ek – eM) !
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First, consider synthetic images, for understanding:
Surfaces: 3 spheres, reflectances from Macbeth ColorChecker Camera: Kodak DSC 420 31 sensor gains qk() Carry out all in 31-D, but show as camera would see it.
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Synthetic Images shading, for light 1, for light 2
Under blue light, P10500 Under red light, P2800
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Synthetic Images Original: not invariant Spectral invariant
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Measured Multispectral Images
Under D75 Under D48 Invt. #1 Invt. #2
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Measured Multispectral Images
After invt. processing In-shadow, In-light
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Measured Multispectral Images
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Measured Multispectral Images
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Measured Multispectral Images
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Next: removing shadows from
Conclusion A novel method for producing illumination invariant, multispectral image Successful in removing effects of Illuminant strength, colour, and shading Next: removing shadows from remote-sensing data.
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Funding: Natural Sciences and Engineering Research Council of Canada
Thanks! Funding: Natural Sciences and Engineering Research Council of Canada Multispectral Images Invariant to Illumination Colour, Strength and Shading
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