DTM REFINEMENT USING MULTI IMAGE SHAPE FROM SHADING
C. Piechullek, C. Heipke
Technical University Munich
Chair for Photogrammetry and Remote Sensing
Munich, Germany
E-Mail: peik@photo.verm.tu-muenchen.de
Working Group III/2: Geometric-Radiometric Models and Object Reconstruction
KEY WORDS: Shape from Shading, radiometric surface model, DTM reconstruction, simulation
ABSTRACT
We present a new approach to Shape from Shading (SFS) to be used with imagery of the MARS96
HRSC/WAOSS mission. The work builds upon prior investigations of multi image SFS [Heipke 1992; Heipke,
Piechullek 1994]. Our SFS approach simultaneously processes multiple images and incorporates an object space
model for the terrain surface. In contrast to most SFS methods which rely on the often too simple Lambertian
surface reflection we introduce the Lommel-Seeliger law widely used in planetary science [Lumme, Bowell 1981;
Hapke 1993] for modeling light reflection at the object surface. We investigate both the Lambertian and the
Lommel-Seeliger model using synthetic images in order to compare the characteristics of both approaches and
to show the advantages over existing SFS methods.
1. INTRODUCTION
Shape from Shading (SFS) is a technique for surface
reconstruction which exploits the fact that surface
patches, having different orientation towards a light
source, are imaged with different brightness in the
images. The grey values of these patches are directly
related to surface inclination. The surface is generally
assumed to have uniform reflectance properties.
Therefore, SFS only performs well in areas with poor
image texture.
Digital image matching is a widely used tool in digital
photogrammetry to derive surface information from
multiple images. In the absence of sufficient, non-
periodic image texture, however, digital image
matching techniques fail to produce correct and
reliable results. Thus, SFS can be used as a means to
complete and refine a digital terrain model (DTM)
which has been generated by digital image matching.
The basic assumption for all SFS algorithms states
that since different parts of a surface have different
orientations relative to the direction of illumination
they are imaged with different brightness. This spatial
variation in brightness, called shading, is used to
locally reconstruct the surface slope. The surface is
described by small planar surface elements; the size of
a surface element approximately equals the size of a
pixel multiplied with the average image scale factor.
The inclinations of neighbouring surface elements are
then integrated to produce a geometric model of the
object surface; all other influences which take part in
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International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B3. Vienna 1996
the image formation process, i.e. illumination, sensor
or atmosphere are assumed to be known.
The basic equation of SFS can be derived assuming a
constant albedo A along with Lambertian reflectance
for the whole surface. In this case, the grey value
g(X,y) at the position x', y' in image space only
depends on the angles between illumination direction,
viewing direction and the local surface normal. Since
the local normal vector n — [-ny;-ny;1]" contains two
unknown components for surface inclination, namely
ny and ny, but only one observation, namely g(x,y’),
for each point in object space, there exists an infinite
number of inclinations, which all result in the same
grey value. To overcome this indeterminability,
additional information must be brought to bear. For
possible solutions and a detailed bibliography on SFS
see [Horn, Brooks 1989].
2. IMAGE FORMATION
In this chapter the image formation process is shortly
reviewed, since the relation between surface
reflectance properties and image irradiance is the basis
for our SFS model.
Trying to express the orientations of the surface
patches as a function of the grey values makes it
necessary to take into account all influences in object
and image space which are part of the imaging
process. The amount of radiance reflected towards a
sensor is a function of
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