Automated classification of landforms on Mars

被引:59
作者
Bue, B. D.
Stepinski, T. F.
机构
[1] Lunar & Planetary Inst, Houston, TX 77058 USA
[2] Purdue Univ, Dept Comp Sci, W Lafayette, IN 47907 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
landform classification; self-organizing maps; digital topography models; automated techniques; Mars;
D O I
10.1016/j.cageo.2005.09.004
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
We propose a numerical method for classification and characterization of landforms on Mars. The method provides an alternative to manual geomorphic mapping of the Martian surface. Digital elevation data is used to calculate several topographic attributes for each pixel in a landscape. Unsupervised classification, based on the self-organizing map technique, divides all pixels into mutually exclusive and exhaustive landform. classes on the basis of similarity between attribute vectors. The results are displayed as a thematic map of landforms and statistics of attributes are used to assign semantic meaning to the classes. This method is used to produce a geomorphic map of the Terra Cimmeria region on Mars. We assess the quality of the automated classification and discuss differences between results of automated and manual mappings. Potential applications of our method, including crater counting, landscape feature search, and large scale quantitative comparisons of Martian surface morphology, are identified and evaluated. (C) 2005 Elsevier Ltd. All rights reserved.
引用
收藏
页码:604 / 614
页数:11
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