2009
DOI: 10.1016/j.pss.2009.03.009
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Automatic detection of sub-km craters in high resolution planetary images

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Cited by 118 publications
(74 citation statements)
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“…By computing the mapping between parameter space and image space, the algorithm can find the target objects within a certain class of shapes. The work most related to our framework is the crater-detection method proposed by Urbach and Stepinski in [2]. Similarly in [2], we identify a crater by two components: a bright region and a shadow region.…”
Section: Related Workmentioning
confidence: 99%
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“…By computing the mapping between parameter space and image space, the algorithm can find the target objects within a certain class of shapes. The work most related to our framework is the crater-detection method proposed by Urbach and Stepinski in [2]. Similarly in [2], we identify a crater by two components: a bright region and a shadow region.…”
Section: Related Workmentioning
confidence: 99%
“…Similarly in [2], we identify a crater by two components: a bright region and a shadow region. Based on the preliminary work done in [2], we perform efficient KDD process [3] on feature creation and feature selection, training set sampling, and utilizing multiple classification methods to improve the detection accuracy.…”
Section: Related Workmentioning
confidence: 99%
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“…A state-of-art framework for crater recognition was developed including crater candidates selection and craters classification by supervised machine learning [2]. Automatic detection of craters is difficult when their rims are unclear, segmented, or the image is noisy (degradation, internal morphologies).…”
Section: Introductionmentioning
confidence: 99%