Artificial intelligence in remote sensing geomorphology—a critical study

Urs Mall, Daniel Kloskowski, Philip Laserstein
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Abstract

Planetary geomorphological maps over a wide range of spatial and temporal scales provide important information on landforms and their evolution. The process of producing a geomorphological map is extremely time-consuming and maps are often difficult to reproduce. The success of deep learning and machine learning promises to drastically reduce the cost of producing these maps and also to increase their reproducibility. However, deep learning methods strongly rely on having sufficient ground truth data to recognize the wanted surface features. In this study, we investigate the results from an artificial intelligence (AI)–based workflow to recognize lunar boulders on images taken from a lunar orbiter to produce a global lunar map showing all boulders that have left a track in the lunar regolith. We compare the findings from the AI study with the results found by a human analyst (HA) who was handed an identical database of images to identify boulders with tracks on the images. The comparison involved 181 lunar craters from all over the lunar surface. Our results show that the AI workflow used grossly underestimates the number of identified boulders on the images that were used. The AI approach found less than one fifth of all boulders identified by the HA. The purpose of this work is not to quantify the absolute sensitivities of the two approaches but to identify the cause and origin for the differences that the two approaches deliver and make recommendations as to how the machine learning approach under the given constraints can be improved. Our research makes the case that despite the increasing ease with which deep learning methods can be applied to existing data sets, a more thorough and critical assessment of the AI results is required to ensure that future network architectures can produce the reliable geomorphological maps that these methods are capable of delivering.
遥感地貌学中的人工智能--一项重要研究
大范围时空尺度的行星地貌图提供了有关地貌及其演变的重要信息。绘制地貌图的过程非常耗时,而且通常难以复制。深度学习和机器学习的成功有望大幅降低制作这些地图的成本,并提高其可重复性。然而,深度学习方法在很大程度上依赖于足够的地面真实数据来识别所需的表面特征。在本研究中,我们研究了基于人工智能(AI)的工作流程的结果,该流程可识别月球轨道器拍摄的图像上的月球巨石,并生成全球月球地图,显示在月球碎屑岩中留下轨迹的所有巨石。我们将人工智能的研究结果与人类分析师(HA)的研究结果进行了比较,后者使用相同的图像数据库来识别图像上带有轨迹的巨石。比较涉及来自月球表面各处的 181 个月球环形山。我们的结果表明,所使用的人工智能工作流程严重低估了所使用图像上已识别巨石的数量。人工智能方法发现的巨石数量不到 HA 识别出的所有巨石数量的五分之一。这项工作的目的不是量化两种方法的绝对灵敏度,而是找出两种方法产生差异的原因和根源,并就如何改进给定限制条件下的机器学习方法提出建议。我们的研究表明,尽管深度学习方法越来越容易应用于现有数据集,但仍需要对人工智能结果进行更全面、更严格的评估,以确保未来的网络架构能够生成这些方法所能提供的可靠地貌图。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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