Full text: Proceedings, XXth congress (Part 4)

  
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part B4. Istanbul 2004 
Since this sensor is a digital three-line scanner with sensing 
capabilities for nadir, fore and aft looks, already three different 
views of the target area exist. This forms an excellent basis for 
the calculation of further views for the lenticular foil vision (cf. 
Chapter 4. Data Processing). 
2. INPUT DATA 
2.1 Topographic Base 
As the major source of topographic information served the sheet 
"Mars" of the multi-lingual series of ICA Maps of the Planets 
and their Moons (Mars Map, 1999) plus other material out of 
which this maps has been compiled. 
2.2 Remote Sensing Imagery 
The imagery used has been acquired since January 2004. 
The post-processing carried out at DLR Berlin-Adlershof 
includes in a first step the rectification of the single image strips 
based on DGPS and INS data. In the second step the image 
strips have been mosaiced to the whole image. In the case of 
HRSC it means, that the majority of the pixels displays 
synthetic radiometric values, calculated for the overlap areas of 
the strips which amount to nearly 50 percent across track. 
  
Parameter Valua 
THX 7808B 
7 um x 7 um 
  
detector type 
  
sensor pixel size 
  
field of view per pixel (IFOV) 8.25 arcsec 
  
active pixels per ccd line 9 sensors a 5184 
  
radiometric resolution 8 bit 
  
spectral filters 5 panchromatic, 4 colour 
  
  
nadir, 2 stereo, 2 photometric 675490 nm 
stereo angle of stereo channel +18.9° 
  
stereo angle of photometric 
channel 2:12.09" 
440245 nm, 530445 nm, 
Blue, Green, Red, Near Infrared | 750420 nm, 970+45 nm 
  
  
  
  
  
stereo angle of Red, NIR £15.9° 
sterco angle of Blue, Green +33° 
maximum scan rate 450 lines/s 
  
  
  
Table 1. Technical data of HRSC Mars Camera, in part based 
on (Hauber, E., Jaumann, R,, Wewel, F., Gwinner, K., Neukum, 
G., Siupetzky, H., 2000). 
The original data, with their excellent ground resolution, have 
been resampled to an appropriate size which saites to the 
respective map product. The excellent radiometric properties of 
the imagery proved ideal for a true-colour depiction of this 
high-relief terrain. 
3. MAP DESIGN 
In order to reach an optimum balance between the area to be 
covered, the final geometric resolution of the remotely sensed 
image data, and the available sizes of lenticular foils, the final 
formats of the actual map areas had to be chosen. 
Due to the fact that an excellent image data material was at our 
disposal, already at an early stage the decision was made that 
the final product should be a so-called CIL (combined image- 
line) map, thus combining the advantages of a sort of photo- 
realistic depiction of the terrain in true-3D and the abstracted 
cartographic information (Buchroithner, M. F., Kostka, R, 
1997). For further remarks on the lettering and other 
cartographic aspects see Chapter 5. 
Based on the assessment of tentative map layouts, the final map 
designs with the title on the top, legend and overview map had 
to be determined. Some peculiarities in comparison with 
“normal” two-dimensional maps had to be considered. Since the 
lenticular foil will cover the whole map format including the 
margin special attention had to be paid to the legibility of all the 
collateral map information (imprint, legend, title, overview 
map). This process is determined by the initial image data 
resolution, the print resolution and the resolution of the human 
perception capability and led to a final map scales. The actual 
layout of the maps is slightly differing. 
4. DATA PROCESSING 
4.1 Geometric Modelling 
Initially, some basic remarks concerning the geometry of 
lenticular foil true-3D maps shall be made. With reference to 
the renowned textbook by Okoshil975 (Okoshi, T., 1976) and 
the paper by Buchroithner and Waelder (these proceedings; 
(Waelder, O., Buchroithner, M. F., 2003)), the ray geometry 
implied by the tunnel shape of the individual lenses can be 
derived from the Figures 1 and 2. 
In contrast to classical parallax stereoscopy, for a high-quality 
true-3D representation based on lenticular technology, a number 
of stereomates significantly higher than two had to be 
calculated. In a way simulating an east-west airplane overflight 
a minimum of seven convergent views was generated. This is a 
prerequisite for a "smooth" viewing of a lenticular scene from 
different east-west directions. Further research in the 
optimisation of the lenticular techniques is planned. 
y Lenticular Foil 
  
Figure 1. Scheme of lenticular foil principle. 
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