Pseudo-Spectral Spatial Feature Extraction and Enhanced Fusion Image for Efficient Meter-Sized Lunar Impact Crater Automatic Detection in Digital Orthophoto Map

• Published in: Sensors (Basel, Switzerland) Vol. 24; no. 16; p. 5206
• Main Authors: Liu, Huiwen, Lu, Ying-Bo, Zhang, Li, Liu, Fangchao, Tian, You, Du, Hailong, Yao, Junsheng, Yu, Zi, Li, Duyi, Lin, Xuemai
• Format: Journal Article
• Language: English
• Published: Switzerland MDPI AG 11.08.2024; MDPI
• Subjects: Algorithms; automatic crater detection; Datasets; Deep learning; Frequency distribution; Geology; Mars; meter-sized crater; Moon; Neural networks; optimization of post-processing parameters; pseudo-spectral spatial feature extraction; Remote sensing; YOLOv5; pseudo-spectral spatial feature extraction; meter-sized crater; optimization of post-processing parameters; YOLOv5; automatic crater detection
• ISSN: 1424-8220; 1424-8220
• DOI: 10.3390/s24165206

Impact craters are crucial for our understanding of planetary resources, geological ages, and the history of evolution. We designed a novel pseudo-spectral spatial feature extraction and enhanced fusion (PSEF) method with the YOLO network to address the problems encountered during the detection of the numerous and densely distributed meter-sized impact craters on the lunar surface. The illumination incidence edge features, isotropic edge features, and eigen frequency features are extracted by Sobel filtering, LoG filtering, and frequency domain bandpass filtering, respectively. Then, the PSEF images are created by pseudo-spectral spatial techniques to preserve additional details from the original DOM data. Moreover, we conducted experiments using the DES method to optimize the post-processing parameters of the models, thereby determining the parameter ranges for practical deployment. Compared with the Basal model, the PSEF model exhibited superior performance, as indicated by multiple measurement metrics, including the precision, recall, -score, , and robustness, etc. Additionally, a statistical analysis of the error metrics of the predicted bounding boxes shows that the PSEF model performance is excellent in predicting the size, shape, and location of impact craters. These advancements offer a more accurate and consistent method to detect the meter-sized craters on planetary surfaces, providing crucial support for the exploration and study of celestial bodies in our solar system.