Full text: Technical Commission IV (B4)

  
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XXXIX-B4, 2012 
XXII ISPRS Congress, 25 August — 01 September 2012, Melbourne, Australia 
Once the images are adequately registered to each other, as well 
as the LOLA data, the process of extracting DEMs can begin 
with NGATE (SOCET SET- Next Generation Automatic 
Terrain Extraction). NGATE performs image correlation and 
edge matching for every pixel in the image to create a dense 
model. The DEM is then resampled to at least three times the 
ground sampling distance of the image in order to reduce noise. 
In the nominal phase of the mission (50 km circular orbit) 
DEMs were typically sampled at a two meter pixel scale. 
Results from NGATE require very little editing if the stereo pair 
was acquired under nominal conditions (35° to 65° incidence 
angle and 10° to 45° convergence angle). Low incidence angles 
can cause LROC images to be difficult to co-register between 
images while images with a high incidence angle are 
significantly affected by shadows and thus require extensive 
editing. NGATE is not optimized to work with the linear 
pushbroom images. In order to increase effectiveness, a pair- 
wise rectification is performed on the images used for DEM 
extraction. Pair-wise rectification rotates the images so that the 
epipolar lines are horizontal and scales are set to a common 
pixel scale. The rectified images make stereovision easier on the 
analyst, and are required for the accurate generation of the DEM 
(Tran et al. 2010). 
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Figure 4. Workflow diagram for DEM production. 
Orthorectified images are created upon completion of the DEM 
using SOCET SET's Orthophoto Generation. Orthophotos are 
images that have had all distortion due to camera obliquity and 
terrain relief removed. An orthophoto represents what you 
would see if you were looking at the ground orthogonally from 
a distance above (every pixel is viewed as if nadir). In addition, 
a hill shade image, color shaded relief image, slope map, and 
confidence map are provided in GeoTIFF format. These 
products are made using the Geospatial Data Abstraction 
Library (GDAL) (Warmerdam 2008). 
4. ERROR ANLAYSIS 
The overall quality of the DEM is a measurement of both the 
absolute and relative accuracies. The absolute accuracies are 
determined by how far the coordinates of the DEM align with 
the true latitude and longitude. LOLA altimetry provides the 
absolute geodetic reference frame for the NAC DEMs. A 
crossover correction analysis with the LOLA data shows 
improvement in the RMS differences between the LOLA track 
data to 10.18 m along track, 8.37 m cross track, and 1.8 m 
radially (Mazarico et al 2011). On average then, it can be 
expected that the positional accuracy of LOLA data approaches 
these levels. 
4.1 Relative Error 
The theoretical expected vertical precision of NAC DEMs can 
be calculated based on the spacecraft orbit and camera 
geometry. While acquiring stereo images, the spacecraft is 
either pointed nadir or rolled about the flight line. In some cases 
near the poles, LRO is pitched forward to acquire stereo images 
(Tran et al. 2010). The convergence angle is the magnitude of 
the parallax angles between the two stereo pairs. SOCET SET 
calculates the linear error between stereo mates upon 
completion of the DEM. The linear error gives an estimate of 
the overall precision of the DEM at the 90% confidence level 
(Subramanian et al. 2003). The horizontal linear error in the 
DEM is the same as the spatial resolution of the DEM. The 
relative precision of DEMs produced from nominal phase 
images is theoretically 0.5 meters, but can be as large as 2.0 
meters. DEMs produced in the commissioning phase and frozen 
orbit will have an expected vertical precision of as much as 3.0 
m. 
4.2 LOLA Registration 
Alimetric observations obtained by LOLA provide 
measurements of +0.1 m between the spacecraft and the lunar 
surface (Smith et al. 2010). However, uncertainties in the 
spacecraft positioning can result in offsets (£15m) between 
altimeter tracks over many orbits. The LROC team is currently 
developing a tool to automatically register alimetric 
observations to NAC DEMs (Speyerer et al. 2012). Using a 
generalized pattern search (GPS) algorithm, the new automatic 
registration adjusts the spacecraft position and pointing 
information for the times when NAC images are acquired as 
well as when LOLA collects measurements of the same region. 
  
  
  
  
    
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improvement in the RMS error and a partition of the final 
registration. 
The absolute horizontal and vertical accuracy of the DEM 
largely depends on the accuracy of the LOLA profiles. 
Currently, our strategy is to register the DEM to only one 
profile with the help of the GPS. This procedure ensures that the 
model is fixed in the down track direction. Other profiles that 
are coincident with the DEM may not be consistent from 
profile-to-profile and have errors due to small unknowns In 
spacecraft position. Areas that are relatively flat are used as 
elevation controls throughout the remaining portion of the 
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