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Fig. 3.2 Definition of the
surface normal n ,the
illumination direction s ,the
viewing direction v , the phase
angle α , the polar angle θ i
and azimuth angle φ i of
incidence, and the polar angle
θ e and azimuth angle φ e of
emission. The vectors n , s ,
and v are generally not
coplanar, such that
α θ i + θ e
map of the surface visible in the image (cf. Sect. 3.2.2.2 ). This approach is termed
shape from shading (Horn, 1986 , 1989 ; Horn and Brooks, 1989 ). An overview of
the variety of techniques to infer a height map from the determined surface gradients
is provided in Sect. 3.2.3 .
3.2.1 The Bidirectional Reflectance Distribution Function (BRDF)
Prior to the detailed description of intensity-based three-dimensional surface recon-
struction methods we introduce the basic radiometric quantities. The light power in-
cident on the apparent surface, measured in W m 2 , is termed irradiance. The light
quantity emitted into a specific direction by a surface is measured in W m 2 sr 1
and is termed radiance. The normalisation to unit solid angle is necessary due to the
generally direction-dependent emission from the surface (Horn, 1986 ).
According to Horn ( 1986 ), the radiance received by the imaging device is de-
pendent on both the viewing direction and the direction of the incident light. The
illumination direction s is given by the 'zenith angle' or 'polar angle' θ i and the 'az-
imuth angle' φ i of incidence, while the direction v into which the reflected light is
emitted is denoted by the zenith angle θ e and the azimuth angle φ e of emission (cf.
Fig. 3.2 ). At this point, the 'bidirectional reflectance distribution function' (BRDF)
f(θ i i e e ) is introduced, which denotes the radiance L surf of a surface viewed
from the direction given by e e ) divided by the irradiance E illum due to illumi-
nation from the direction given by i i ) . Accordingly, the BRDF is defined as
dL surf e e )
dE illum i i ) =
dL surf e e )
L illum i i ) cos θ i i
f(θ i i e e )
=
(3.6)
(Nicodemus et al. 1977 ;Dorseyetal. 2008 ). In ( 3.6 ), dL surf e e ) denotes the
differential radiance as perceived by the detector dE illum i i ) = L illum cos θ i i
the differential irradiance received from the light source situated in the direction
given by i i ) (cf. Fig. 3.3 ), L illum i i ) the radiance of the light source, and
i the differential solid angle under which the regarded surface element appears
from the position of the light source (Nicodemus et al. 1977 ). Horn ( 1986 ) states
(regarding the Lambertian case) that the factor cos θ i originates from geometrical
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