AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALS

Crater-detection approaches can be divided into four categories: manual recognition, shape-profile fitting algorithms, machine-learning methods and geological information-based analysis using terrain and spectral data. The mainstream method is Shape-profile fitting algorithms. Many scholars througho...

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Main Authors: L. Ye, X. Xu, D. Luan, W. Jiang, Z. Kang
Format: Article
Language:English
Published: Copernicus Publications 2017-07-01
Series:The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
Online Access:https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLII-3-W1/199/2017/isprs-archives-XLII-3-W1-199-2017.pdf
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spelling doaj-b396ea470d0e413bbbcc5dfd2d031c972020-11-24T21:59:21ZengCopernicus PublicationsThe International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences1682-17502194-90342017-07-01XLII-3-W119920410.5194/isprs-archives-XLII-3-W1-199-2017AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALSL. Ye0X. Xu1D. Luan2W. Jiang3Z. Kang4Surveying and Mapping Engineering, School of Land Science and Technology, University of Geosciences (Beijing), Xueyuan Road, Haidian District, Beijing, 100083, ChinaSurveying and Mapping Engineering, School of Land Science and Technology, University of Geosciences (Beijing), Xueyuan Road, Haidian District, Beijing, 100083, ChinaSurveying and Mapping Engineering, School of Land Science and Technology, University of Geosciences (Beijing), Xueyuan Road, Haidian District, Beijing, 100083, ChinaSurveying and Mapping Engineering, School of Land Science and Technology, University of Geosciences (Beijing), Xueyuan Road, Haidian District, Beijing, 100083, ChinaSurveying and Mapping Engineering, School of Land Science and Technology, University of Geosciences (Beijing), Xueyuan Road, Haidian District, Beijing, 100083, ChinaCrater-detection approaches can be divided into four categories: manual recognition, shape-profile fitting algorithms, machine-learning methods and geological information-based analysis using terrain and spectral data. The mainstream method is Shape-profile fitting algorithms. Many scholars throughout the world use the illumination gradient information to fit standard circles by least square method. Although this method has achieved good results, it is difficult to identify the craters with poor "visibility", complex structure and composition. Moreover, the accuracy of recognition is difficult to be improved due to the multiple solutions and noise interference. Aiming at the problem, we propose a method for the automatic extraction of impact craters based on spectral characteristics of the moon rocks and minerals: 1) Under the condition of sunlight, the impact craters are extracted from MI by condition matching and the positions as well as diameters of the craters are obtained. 2) Regolith is spilled while lunar is impacted and one of the elements of lunar regolith is iron. Therefore, incorrectly extracted impact craters can be removed by judging whether the crater contains "non iron" element. 3) Craters which are extracted correctly, are divided into two types: simple type and complex type according to their diameters. 4) Get the information of titanium and match the titanium distribution of the complex craters with normal distribution curve, then calculate the goodness of fit and set the threshold. The complex craters can be divided into two types: normal distribution curve type of titanium and non normal distribution curve type of titanium. We validated our proposed method with MI acquired by SELENE. Experimental results demonstrate that the proposed method has good performance in the test area.https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLII-3-W1/199/2017/isprs-archives-XLII-3-W1-199-2017.pdf
collection DOAJ
language English
format Article
sources DOAJ
author L. Ye
X. Xu
D. Luan
W. Jiang
Z. Kang
spellingShingle L. Ye
X. Xu
D. Luan
W. Jiang
Z. Kang
AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALS
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
author_facet L. Ye
X. Xu
D. Luan
W. Jiang
Z. Kang
author_sort L. Ye
title AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALS
title_short AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALS
title_full AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALS
title_fullStr AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALS
title_full_unstemmed AUTOMATIC DETECTION AND RECOGNITION OF CRATERS BASED ON THE SPECTRAL FEATURES OF LUNAR ROCKS AND MINERALS
title_sort automatic detection and recognition of craters based on the spectral features of lunar rocks and minerals
publisher Copernicus Publications
series The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
issn 1682-1750
2194-9034
publishDate 2017-07-01
description Crater-detection approaches can be divided into four categories: manual recognition, shape-profile fitting algorithms, machine-learning methods and geological information-based analysis using terrain and spectral data. The mainstream method is Shape-profile fitting algorithms. Many scholars throughout the world use the illumination gradient information to fit standard circles by least square method. Although this method has achieved good results, it is difficult to identify the craters with poor "visibility", complex structure and composition. Moreover, the accuracy of recognition is difficult to be improved due to the multiple solutions and noise interference. Aiming at the problem, we propose a method for the automatic extraction of impact craters based on spectral characteristics of the moon rocks and minerals: 1) Under the condition of sunlight, the impact craters are extracted from MI by condition matching and the positions as well as diameters of the craters are obtained. 2) Regolith is spilled while lunar is impacted and one of the elements of lunar regolith is iron. Therefore, incorrectly extracted impact craters can be removed by judging whether the crater contains "non iron" element. 3) Craters which are extracted correctly, are divided into two types: simple type and complex type according to their diameters. 4) Get the information of titanium and match the titanium distribution of the complex craters with normal distribution curve, then calculate the goodness of fit and set the threshold. The complex craters can be divided into two types: normal distribution curve type of titanium and non normal distribution curve type of titanium. We validated our proposed method with MI acquired by SELENE. Experimental results demonstrate that the proposed method has good performance in the test area.
url https://www.int-arch-photogramm-remote-sens-spatial-inf-sci.net/XLII-3-W1/199/2017/isprs-archives-XLII-3-W1-199-2017.pdf
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