基于深度学习的月球穹顶自动探测方法

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Planetary and Space Science Pub Date : 2024-05-31 DOI:10.1016/j.pss.2024.105916
Yunxiang Tian, Xiaolin Tian
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引用次数: 0

摘要

月穹是月球表面常见的结构,对研究月球的地质演变非常重要。月球穹隆的空间频率分布为月球火山的演化提供了重要证据。近年来,深度学习方法在许多领域得到了快速发展。然而,现有的圆顶检测算法大多采用人工或半自动的传统方法。本文提出了一种自动深度学习识别方法,简化了传统的圆顶识别过程,是一种端到端的检测方法。我们利用数字高程模型数据建立了月球穹顶数据集,并比较了 11 种先进的深度学习目标检测算法,其中包括三种检测架构。我们选取了马里乌斯丘陵地区进行验证,以评估方法的性能。通过与人工识别结果的比较,所提出的方法的识别精确度为 88.7%。此外,我们还发现了 12 个未记录的潜在圆顶/圆锥。形态特征和可视化结果表明,检测到的特征可能是穹顶/圆锥,我们的方法可以提供新颖的穹顶检测。
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Automatic lunar dome detection methods based on deep learning

Lunar domes are common structures on the lunar surface and are important for studying the geological evolution of the moon. The distribution of spatial frequencies of lunar domes provides significant evidence for the evolution of lunar volcanoes. In recent years, deep learning methods have been rapidly developing in many fields. However, most of the existing dome detection algorithms use manual or semi-automatic traditional methods. In this paper, we propose an automatic deep learning recognition method to simplify the traditional dome identification process, which is an end-to-end detection method. We built a lunar dome dataset using digital elevation model data and compared eleven advanced deep learning target detection algorithms, which include three types of detection architecture. The region of Marius Hills was selected for validation to evaluate method performance. By comparing the results with manual identification, the proposed method has an identification precision of 88.7%. In addition, we detected 12 unrecorded potential domes/cones. The morphological characterization and visualization results indicate that the detected features may be domes/cones and our method may provide novel dome detection.

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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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