ue for the 
ns in the 
sults in an 
relative to 
ve height 
r, can be 
e modeled 
heights are 
instruction 
differences 
opography. 
| results, if 
re modeled 
el-Seeliger 
od results, 
wn surface 
nally, this 
occur when 
cted from 
1 direction. 
een used; 
| be tested 
ces, such as 
aluate the 
Jel, and to 
e methods 
lbedo are 
> MARS96 
> three-line 
id WAOSS 
Neukum G. 
Mars 94/96 
Reflectance 
seophysical 
eflectance 
facroscopic 
Reflectance 
tion Effect. 
Hapke B. (1993): Theory of Reflectance and Emittance 
Spectroscopy. Topics in Remote Sensing III. 
Cambridge University Press 
Heipke C. (1992): Integration of Digital Image 
Matching and Multi Image Shape from Shading, in: 
Mustererkennung 1993, 15. DAGM-Symposium, Pöppl 
S.J., H. Handels (eds.). Informatik aktuell, Springer, 
Berlin, 367-374 
Heipke C., Piechullek C. (1994): Towards Surface 
Reconstruction Using Multi Image Shape from 
Shading. IntArchPhRS (30) 3/1, 361-369 
Horn B.K.P. (1986): Robot Vision. The MIT Press, 
Cambridge 
Horn B.K.P., Brooks M.J. (eds.) (1989): Shape from 
Shading. The MIT Press, Cambridge 
Lumme K.,, Bowell E. (1981): Radiative Transfer in the 
Surfaces of Atmosphereless Bodies; I. Theory. 
Astronomical Journal 86, 1694-1704 
McEwen A.S. (1991): Photometric Functions for 
Photoclinometry and Other Applications. Icarus 92, 
298-311 
Minnaert M. (1941): The Reciprocity Principle in 
Lunar Photometry. Astrophysical Journal 93, 403-410 
651 
ET HE Fe NT gén EE e REP " 
"uu ipsas ETE, 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B3. Vienna 1996