Full text: Proceedings, XXth congress (Part 4)

  
  
GEOMORPHOMETRIC MAPPING OF GRAND CANYON FROM THE 1-DEGREE USGS 
DEMS 
Nikos A. Kokkas™ *, George Ch. Miliaresis h 
* Technological Educational Institute of Athens, Department of Topography, 4 Olympias Str. , Athens 165-61, Greece - 
nkokkas@mail.com 
* Geology Department, University of Patras, RION, 26500, Greece - miliaresis@email.com 
Commission PS WG IV/9 
KEY WORDS: Remote Sensing, Geomorphology, GIS, Segmentation, Comparison, Extraterrestrial, Visualization 
ABSTRACT: 
In a previous research effort a terrain partition framework was defined allowing the partition of the landscape of Valles Marineris 
chasma (an elongated steep-sided depression located in Mars) to elementary objects. Each object was parametrically represented on 
the basis of its spatial 3-dimensional arrangement and mapped according to a terrain classification scheme. In the current research 
effort Grand Canyon is delineated from the one degree USGS DEMs and various geomorphometric parameters are computed in an 
attempt to capture the geomorphometric signature of the largest canyon in earth. More specifically, the landscape was described on 
the basis of the statistical parameters computed for elevation and gradient, histogram frequency distributions and rose diagrams. The 
geomorphometric comparison indicates that Valles Marineris is a steeper terrain with higher relief variability. The rectilinear 
mountain fronts are a key indicator of the tectonic forces that shape the terrain of Valles Marineris chasma. The terrain of Grand 
Canyon is developed parallel to fluvial process direction while in Valles Marineris the terrain flows vertically to the mountain fronts. 
Thus, the key factor controlling the development of the landscape in Grand Canyon is fluvial process versus tectonism in Valles 
Marineris. Valles Marineris is less massive than Grand Canyon but this is due to the much greater elevation range observed (12 km 
versus 2.5 km). 
1. INTRODUCTION 
New concepts, data, and methods, emergent in geographic 
information science in recent years have presented scientists 
with new opportunities to gain fresh insights into the study of 
landscape (Pike, 1995; Pike, 2000; Saura and Martinez, 2001). 
Landscape dynamics is considered to involve scale, pattern and 
process that extend across various geographical domains 
through their spatial interactions. In the current approach, a) 
scale is regional or physiographic, b) pattern expresses the 
partition of landscape to elementary units and their 
representation on the basis of their spatial 3-dimensional 
arrangement (Evans, 1981; Miliaresis, 2001a) and c) process 
expresses the relationship between tectonics and topography 
(Merits and Ellis, 1995; Summerfield, 2000). 
Towards this end the mountains were considered to form the 
elementary morphotectonic units at regional scale and their 
definition and modeling characterized the landscape (Miliaresis, 
2001a) The previous studies were based on the moderate 
resolution digital elevation models (DEMs) GTOPO30 and 
GLOBE. On the other hand nowadays, moderate resolution 
DEMs and imagery are available for Mars (MOLA 
Topographic Map, 2002). For example the equatorial system of 
troughs was first seen on Mariner 9 images and was one of the 
most spectacular discoveries of this mission (Kieffer et al. 
1992; Greeley, 1994). The main trough system (Valles 
Marineris) was named in honor of the achievement of the 
Mariner 9 mission. 
Thus, it would be of a great research interest to study the 
planetary landscapes and compare them to the terrestrial one. A 
  
* Corresponding author. 
840 
previous effort in characterizing the landscape of the Valles 
Marineris chasma has been completed and therefore various 
geomorphometric parameters is calculated (Miliaresis and 
Kokkas, 2003). 
  
  
  
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Figure 1. Index map of the one degree DEM available from 
USGS. 
This paper focuses on the mapping and characterization of the 
landscape dynamics in Grand Canyon from the one degree 
DEM available from USGS (Figure 1). With the calculation of 
the geomorphometric parameters a comparison between the 
Valles Marineris chasma and the Grand Canyon will be 
performed.
	        
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