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University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Camera Simulation
ReferencesPhotography, B. London and J. Upton
Optics in Photography, R. Kingslake
The Camera, The Negative, The Print, A. Adams
Effect Cause
Field of view Film size, stops and pupils
Depth of field Aperture, focal length
Motion blur Shutter
Exposure Film speed, aperture, shutter
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Topics
Ray tracing lenses
Focus
Field of view
Depth of focus / depth of field
Exposure
Lenses
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Refraction
I
′I
sin sinn I n I′ ′=
Snell’s Law
N
n n′
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Paraxial Approximation
0e ≈
Rays deviate only slightly from the axis
U
z
€
sin(U) ≈ U = u
tan(U) ≈ U = u
cos(U) ≈1
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Incident Ray
I
U φ−
φ= −I U
Angles: ccw is positive; cw is negative
The sum of the interior angles is equal to the exterior angle.
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Refracted Ray
− ′U′I
φ= −′ ′I U
φ− = + −′ ′( ) ( )I U
φ−
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Derivation
Paraxial approximationφ φ= − ⇒ = −I U i uφ φ= − ⇒ = −′ ′ ′ ′I U i u
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Derivation
Paraxial approximation
Snell’s Law= ⇒ =′ ′ ′ ′sin sinn I n I n i ni
φ φ= − ⇒ = −I U i uφ φ= − ⇒ = −′ ′ ′ ′I U i u
φ φ− = −′ ′( ) ( )n u n u
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Ray Coordinates
−z z′
Ru
φ− =h
R
φ− − ′u
=−h
uz
− =′′
hu
z
h
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Gauss’ Formula
Paraxial approximation to Snell’s Law
Ray coordinates
Thin lens equation
φ φ− = −′ ′( ) ( )n u n u
( ) ( )
( )
h h h hn n
z R z Rn n n n
z z R
′ − = −′
′ ′−= +
′
φ=−h
R=−′
′h
uz
=−h
uz
Holds for any height, any ray!
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Vergence
Vergence
Thin lens equation
Surface Power equation
⎡ ⎤≡ ≈ =⎢ ⎥⎣ ⎦
1n nV diopters
r z m
V V P′= +
< 0V =0V > 0V
≡ −′1
( )P n nR
Diverging Converging
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Lens-makers Formula
⎛ ⎞= − − =′ ⎜ ⎟⎝ ⎠1 2
1 1 1( )P n n
R R f
Converging Diverging
Refractive Power
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Conjugate Points
To focus: move lens relative to backplaneHorizontal rays converge on focal point in the focal plane
1 1 1
z z f= +
′
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Gauss’ Ray Tracing Construction
Parallel Ray
Focal RayChief Ray
Object Image
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Ray Tracing: Finite Aperture
Focal Plane Back PlaneAperture Plane
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Real Lens
Cutaway section of a Vivitar Series 1 90mm f/2.5 lensCover photo, Kingslake, Optics in Photography
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Double Gauss
Radius (mm) Thick (mm) nd V-no aperture
58.950 7.520 1.670 47.1 50.4
169.660 0.240 50.4
38.550 8.050 1.670 47.1 46.0
81.540 6.550 1.699 30.1 46.0
25.500 11.410 36.0
9.000 34.2
-28.990 2.360 1.603 38.0 34.0
81.540 12.130 1.658 57.3 40.0
-40.770 0.380 40.0
874.130 6.440 1.717 48.0 40.0
-79.460 72.228 40.0
Data from W. Smith, Modern Lens Design, p 312
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Ray Tracing Through Lenses
From Kolb, Mitchell and Hanrahan (1995)
200 mm telephoto
50 mm double-gauss
35 mm wide-angle
16 mm fisheye
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Thick Lenses
Refraction occurs at the principal planes
Equivalent Lens
Field of View
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Field of View
From London and Upton
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Field of View
From London and Upton
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Field of View
Field of view
Types of lensesNormal 26º
Film diagonal focal length
Wide-angle 75-90ºNarrow-angle 10º
Redrawn from Kingslake, Optics in Photography
tan2
fov filmsize
f=
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Perspective Transformation
Thin lens equation
Represent transformation as a 4x4 matrix
= + ⇒ =′+′
⇒ =′+
⇒ =′+
1 1 1 fzz
z z f z f
fxx
z f
fyy
z f
Depth of Field
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Depth of Field
From London and Upton
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Circle of Confusion
d′
a
c d s z
a z z
′ ′ ′−= =
′ ′
s′sz z′
c
Circle of confusion proportional to the size of the aperture
Focal Plane Back Plane
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Depth of Focus [Image Space]
Depth of focus Equal circles of confusion
Two planes: near and far
−′ ′ ′= =
′ ′f f
f f
d s zc
a z zc
a
fz
s
nz
c
′s
′fz
′nz′fd
−′ ′ ′= =
′ ′n n
n n
d z sc
a z z
′nd
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Depth of Focus [Image Space]
Depth of focus Equal circles of confusion
−′ ′ ′ ⎛ ⎞= = ⇒ = +⎜ ⎟⎝ ⎠′ ′ ′ ′1 1
1f f
f f f
d s zc c
a z z z s ac
a
fz
s
nz
c
′s
′fz
′nz′fd
−′ ′ ′ ⎛ ⎞= = ⇒ = −⎜ ⎟⎝ ⎠′ ′ ′ ′1 1
1n n
n n n
d z sc c
a z z z s a
′nd
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Depth of Focus [Image Space]
Depth of focus Equal circles of confusion
⎛ ⎞= +⎜ ⎟⎝ ⎠′ ′1 1
1f
c
z s a
c
′s′fz
′nz
⎛ ⎞= −⎜ ⎟⎝ ⎠′ ′1 1
1n
c
z s a
+ =′ ′ ′
1 1 12
f nz z s
− =′ ′ ′
1 1 2 1
f n
c
z z a s
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Depth of Field [Object Space]
Depth of field Equal circles of confusion
+ =1 1 1
2n fz z s
⎛ ⎞− = − ≈⎜ ⎟⎝ ⎠
1 1 2 1 1 2 1
n f
c c
z z a f s a f
= +′
1 1 1
f fz z f= +
′1 1 1
n nz z fc
fz
nz
c
= +′
1 1 1
s s f
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Hyperfocal Distance
c
fz
nz
cWhen
→ ⇒ = =∞,2n f
Hs H z z
H is the hyperfocal distance
+ =1 1 1
2n fz z s
€
N ≡f
a
€
1
zn
−1
z f
=2c
a
1
f= 2
cN
f 2≡ 2
1
H
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Depth of Field Scale
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Factors Affecting DOFFrom http://www.kodak.com/global/en/consumer/pictureTaking/cameraCare/cameCar6.shtml
= 2
1 cN
H f
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Resolving Power
Diffraction limit
35mm film (Leica standard)
CCD/CMOS pixel aperture
[ ]λ μ= = × ×1.22 1.22 64 .500 m=0.040mmf
ca
=0.025mmc
=0.0116mm (Nikon D1)c
Exposure
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Image Irradiance
f
2
2cos sin4
aE L d L L
f
πθ ω π θΩ
⎛ ⎞= = = ⎜ ⎟
⎝ ⎠∫
a
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Image Irradiancen̂
θ
€
φ
€
φ
€
ω
€
ω =π4
a2 cosφ
(z /cosφ)2=
π
4
a
z
⎛
⎝ ⎜
⎞
⎠ ⎟2
cos3 φSolid angle subtended by thelens, as seen by the patch A
€
ω
€
δP =LΩ δA cosθ = LδAπ
4
a
z
⎛
⎝ ⎜
⎞
⎠ ⎟2
cos3 φcosθPower from patch Athrough the lens
€
E =δP
δI=L
δA
δI
π
4
a
z
⎛
⎝ ⎜
⎞
⎠ ⎟2
cos3 φcosθIrradiance at thesensor element
€
δA
€
δI
€
a
€
f
€
z
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Image Irradiance
€
ˆ n
θ
€
φ
€
φ
€
δAcosθ
(z /cosφ)2=
δI cosφ
( f /cosφ)2
€
δA
δI=
cosφ
cosθ
z
f
⎛
⎝ ⎜
⎞
⎠ ⎟
2€
δI
€
δA
€
z
€
a
€
f
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Image Irradiance
€
E =δP
δI=L
δA
δI
π
4
a
z
⎛
⎝ ⎜
⎞
⎠ ⎟2
cos3 φcosθ
€
E = Lπ
4
a
f
⎛
⎝ ⎜
⎞
⎠ ⎟
2
cos4 φ
€
δA
δI=
cosφ
cosθ
z
f
⎛
⎝ ⎜
⎞
⎠ ⎟
2
€
E = Lπ
4
a
f
⎛
⎝ ⎜
⎞
⎠ ⎟
2
On axis
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Relative Aperture or F-Stop
F-Number and exposure:
Fstops: 1.4 2 2.8 4.0 5.6 8 11 16 22 32 45 641 stop doubles exposure
f
π= 2
1
4E L
N
=f
aN
a
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Camera Exposure
Exposure
Exposure overdeterminedAperture: f-stop - 1 stop doubles H
Decreases depth of field
Shutter: Doubling the open time doubles HIncreases motion blur
H E T= ×
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Aperture vs Shutter
From London and Upton
f/161/8s
f/41/125s
f/21/500s
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
High Dynamic Range
Sixteen photographs of the Stanford Memorial Church taken at 1-stop increments from 30s to 1/1000s.From Debevec and Malik, High dynamic range photographs.
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Simulated Photograph
Adaptive histogram With glare, contrast, blur
University of Texas at Austin CS395T - Advanced Image Synthesis Spring 2007 Don Fussell
Camera Simulation
Sensor response
Lens
Shutter
Scene radiance
λ ω ω λ λ ω λΩ Λ
= •′ ′ ′ ′ ′ ′ ′∫∫∫∫r r
( , ) ( , , ) ( ( , , ), , ) ( )A T
R P x S x t L T x t dA x d dt d
ω ω λ= ′ ′( , ) ( , , )x T x
λ′( , )P x
( , , , )L x tω λω′ ′( , , )S x t
ω λ′ ′( , , , )L x tω λ( , , , )L x tA
Ω