Abstract

Machine learning (ML) algorithmic developments and improvements in Earth and planetary science are expected to bring enormous benefits for areas such as geospatial database construction, automated geological feature reconstruction, and surface dating. In this study, we aim to develop a deep learning (DL) approach to reconstruct the subsurface discontinuities in the subsurface environment of Mars employing the echoes of the Shallow Subsurface Radar (SHARAD), a sounding radar equipped on the Mars Reconnaissance Orbiter (MRO). Although SHARAD has produced highly valuable information about the Martian subsurface, the interpretation of the radar echo of SHARAD is a challenging task considering the vast stocks of datasets and the noisy signal. Therefore, we introduced a 3D subsurface mapping strategy consisting of radar echo pre-processors and a DL algorithm to automatically detect subsurface discontinuities. The developed components the of DL algorithm were synthesized into a subsurface mapping scheme and applied over a few target areas such as mid-latitude lobate debris aprons (LDAs), polar deposits and shallow icy bodies around the Phoenix landing site. The outcomes of the subsurface discontinuity detection scheme were rigorously validated by computing several quality metrics such as accuracy, recall, Jaccard index, etc. In the context of undergoing development and its output, we expect to automatically trace the shapes of Martian subsurface icy structures with further improvements in the DL algorithm.

Highlights

  • Conventional computer algorithms in the geoscience field have been applied mainly for spatial data processing such as stereo analysis of topography, multispectral/hyperspectral analysis, and other remote sensing data compiling

  • In this study, we focused on the development of an automated algorithm for subsurface discontinuity detection using deep learning (DL)

  • The first target area to test the discontinuity detection is lobate debris aprons (LDAs), which is regarded as an evidence of potential glacial processes [28] or ice debris transport in the ancient Martian environment [29]

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Summary

Introduction

Conventional computer algorithms in the geoscience field have been applied mainly for spatial data processing such as stereo analysis of topography, multispectral/hyperspectral analysis, and other remote sensing data compiling These days, novel approaches combined with contemporary machine learning algorithms are changing the trend of computational geoscience. With the advancement in powerful analytical approaches such as stereo topographic construction [5], the research communities would be benefited enormously by tracing the shape of and changes in the planetary surface. We expect that the success of this effort will result in a highly valuable interpretation tool for future planetary missions as well as contemporary GPR sensors (for instance, SHARAD, in Martian orbit, which provides the target data in this study). The result and validation outcomes employing error metrics are presented in Sections 4 and 5, along with relevant discussion

Target Area
Introduction to to SHARAD
Introduction to SHARAD Data Products
Processing Method
Pre-Processing
A filtering result
Machine Vision Algorithm
Evaluation Metric
Results and Discussion
11. Euripus
Conclusion and Future
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