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Basic Principles of Imaging and Photometry Lecture #2 Thanks to Shree Nayar, Ravi Ramamoorthi, Pat...
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Transcript of Basic Principles of Imaging and Photometry Lecture #2 Thanks to Shree Nayar, Ravi Ramamoorthi, Pat...
Basic Principles of Imaging and Photometry
Lecture #2
Thanks to Shree Nayar, Ravi Ramamoorthi, Pat Hanrahan
Computer Vision: Building Machines that See
Lighting
Scene
Camera
Computer
Physical Models
Scene Interpretation
We need to understand the Geometric and Radiometric relationsbetween the scene and its image.
Camera Obscura, Gemma Frisius, 1558
1558A Brief History of Images
Lens Based Camera Obscura, 1568
15581568
A Brief History of Images
Still Life, Louis Jaques Mande Daguerre, 1837
1558
1837
1568A Brief History of Images
Silicon Image Detector, 1970
1558
1837
1568
1970
A Brief History of Images
1558
1837
1568
1970
1995
A Brief History of Images
Digital Cameras
Geometric Optics and Image Formation
TOPICS TO BE COVERED :
1) Pinhole and Perspective Projection
2) Image Formation using Lenses
3) Lens related issues
Pinhole and the Perspective Projection
(x,y)
screen scene
Is an image being formedon the screen?
YES! But, not a “clear” one.
image plane
effective focal length, f’optical axis
y
x
z
pinhole
),,( zyxr
z
y
f
y
z
x
f
x
'
'
'
'
zf
rr
'
'
)',','(' fyxr
Magnification
image plane
f’optical axis
y
x
zPinhole
planar scene
A
B
A’
B’
d
d’
z
yy
f
yy
z
xx
f
xx
z
y
f
y
z
x
f
x
'
''
'
''
'
'
'
'
From perspective projection: Magnification:
z
f
yx
yx
d
dm
'
)()(
)'()'('22
22
),,(
),,(
zyyxxB
zyxA
)','',''('
)',','('
fyyxxB
fyxA
2mArea
Area
scene
image
Orthographic Projection
image plane
optical axis
y
x
z
),,( zyxr
)',','(' fyxr
zz
xmx ' ymy 'Magnification:
When m = 1, we have orthographic projection
This is possible only when zz In other words, the range of scene depths is assumed to be
much smaller than the average scene depth.
But, how do we produce non-inverted images?
Better Approximations to Perspective Projection
Problems with Pinholes
• Pinhole size (aperture) must be “very small” to obtain a clear image.
• However, as pinhole size is made smaller, less light is received by image plane.
• If pinhole is comparable to wavelength of incoming light, DIFFRACTION effects blur the image!
• Sharpest image is obtained when:
pinhole diameter
Example: If f’ = 50mm,
= 600nm (red),
d = 0.36mm
'2 fd
Image Formation using Lenses
• Lenses are used to avoid problems with pinholes.
• Ideal Lens: Same projection as pinhole but gathers more light!
i o
foi
111Gaussian Lens Formula:
• f is the focal length of the lens – determines the lens’s ability to bend (refract) light
• f different from the effective focal length f’ discussed before!
P
P’
f
Focus and Defocus
foi
111
Depth of Field: Range of object distances over which image is sufficiently well focused.i.e. Range for which blur circle is less than the resolution of the imaging sensor.
d
aperturediameter
aperture
foi
1
'
1
'
1Gaussian Law:
Blur Circle, b
)'()()'(
)'( oofo
f
fo
fii
Blur Circle Diameter : )'('
iii
db
i
'i
o
'o
Two Lens System
• Rule : Image formed by first lens is the object for the second lens.
• Main Rays : Ray passing through focus emerges parallel to optical axis.
Ray through optical center passes un-deviated.
imageplane
lens 2 lens 1
object
intermediatevirtual image
1i
1o2i 2o2f 1f
finalimage
d
• Magnification: 1
1
2
2
o
i
o
im
Exercises: What is the combined focal length of the system? What is the combined focal length if d = 0?
Lens related issues
Compound (Thick) Lens Vignetting
Chromatic Abberation Radial and Tangential Distortion
thickness
principal planes
nodal points
1L2L3L B
A
more light from A than B !
RFBF GF
Lens has different refractive indicesfor different wavelengths.
image plane
ideal actual
ideal actual
Radiometry and Image Formation
• To interpret image intensities, we need to understand Radiometric Concepts and Reflectance Properties.
• TOPICS TO BE COVERED:
1) Image Intensities: Overview
2) Radiometric Concepts:
Radiant IntensityIrradianceRadianceBRDF
3) Image Formation using a Lens
4) Radiometric Camera Calibration
Image Intensities
Image intensities = f ( normal, surface reflectance, illumination )
Note: Image intensity understanding is an under-constrained problem!
source sensor
surfaceelement
normalNeed to considerlight propagation ina cone
Radiometric concepts – boring…but, important!
(1) Solid Angle : 22
cos'
R
dA
R
dAd i ( steradian )
What is the solid angle subtended by a hemisphere?
d (solid angle subtended by )dA
R'dA
dA
(foreshortened area)
(surface area)
i
(2) Radiant Intensity of Source :
Light Flux (power) emitted per unit solid angle
dd
J
( watts / steradian )
(3) Surface Irradiance :dA
dE
( watts / m )
Light Flux (power) incident per unit surface area.
Does not depend on where the light is coming from!
source
2
(4) Surface Radiance (tricky) :
d
ddA
dL
r )cos(
2 (watts / m steradian )
dA
r
• Flux emitted per unit foreshortened area per unit solid angle.
• L depends on direction
• Surface can radiate into whole hemisphere.
• L depends on reflectance properties of surface.
r
The Fundamental Assumption in Vision
Surface Camera
No Change in
Radiance
Lighting
Radiance properties
• Radiance is constant as it propagates along ray
– Derived from conservation of flux
– Fundamental in Light Transport.
1 21 1 1 2 2 2d L d dA L d dA d
2 21 2 2 1d dA r d dA r
1 21 1 2 22
dAdAd dA d dA
r
1 2L L
SceneRadiance L Lens Image
Irradiance E
CameraElectronics
Scene
ImageIrradiance E
Relationship between Scene and Image Brightness
Measured Pixel Values, I
Non-linear Mapping!
Linear Mapping!
• Before light hits the image plane:
• After light hits the image plane:
Can we go from measured pixel value, I, to scene radiance, L?
Relation between Image Irradiance E and Scene Radiance L
f z
surface patchimage plane
id
sd
Ld
idA
sdA
image patch
si dd 22 )cos/(
cos
)cos/(
cos
z
dA
f
dA si 2
cos
cos
f
z
dA
dA
i
s
• Solid angles of the double cone (orange and green):
(1)
2
2
)cos/(
cos
4
z
dd L
• Solid angle subtended by lens:
(2)
Relation between Image Irradiance E and Scene Radiance L
f z
surface patchimage plane
id
sd
Ld
idA
sdA
image patch
• Flux received by lens from = Flux projected onto image sdA idA
iLs dAEddAL )cos( (3)
• From (1), (2), and (3): 4
2
cos4
f
dLE
• Image irradiance is proportional to Scene Radiance!
• Small field of view Effects of 4th power of cosine are small.
Relation between Pixel Values I and Image Irradiance E
• The camera response function relates image irradiance at the image plane to the measured pixel intensity values.
CameraElectronics
ImageIrradiance E
Measured Pixel Values, I
IEg :
(Grossberg and Nayar)
Radiometric Calibration
•Important preprocessing step for many vision and graphics algorithms such as photometric stereo, invariants, de-weathering, inverse rendering, image based rendering, etc.
EIg :1
•Use a color chart with precisely known reflectances.
Irradiance = const * ReflectanceP
ixel V
alu
es
3.1%9.0%19.8%36.2%59.1%90%
• Use more camera exposures to fill up the curve.• Method assumes constant lighting on all patches and works best when source is far away (example sunlight).
• Unique inverse exists because g is monotonic and smooth for all cameras.
0
255
0 1
g
?
?1g
The Problem of Dynamic Range
• Dynamic Range: Range of brightness values measurable with a camera
(Hood 1986)
High Exposure Image Low Exposure Image
• We need 5-10 million values to store all brightnesses around us.• But, typical 8-bit cameras provide only 256 values!!
• Today’s Cameras: Limited Dynamic Range
Images taken with a fish-eye lens of the sky show the wide range of brightnesses.
High Dynamic Range Imaging
• Capture a lot of images with different exposure settings.
• Apply radiometric calibration to each camera.
• Combine the calibrated images (for example, using averaging weighted by exposures).
(Debevec)
(Mitsunaga)