用超像素优化立体匹配,提升火星探测器地形建模精度
Stereovision Image Processing for Planetary Navigation Maps with Semi-Global Matching and Superpixel Segmentation
- 结合SGM与超像素分割,增强深度图上下文理解
- 在斜坡和遮挡区减少空洞,更清晰还原小石块等细节
- 适用于火星自主导航,可直接集成到未来探测任务
火星探测需要精确可靠的地形模型以保障漫游车在复杂多变、充满危险的地表安全行驶。立体视觉在漫游车感知中起关键作用,通过立体匹配生成高精度深度图实现场景重建。现有火星探测多采用传统局部块匹配方法,以方形窗口聚合代价并依赖平滑性约束优化视差,但在低纹理图像、遮挡和重复图案区域表现不佳,因仅考虑有限邻域像素且缺乏场景整体理解。本文提出基于超像素优化的半全局匹配(SGM)方法,缓解了块状伪影,恢复丢失细节。该方法兼顾SGM的效率与精度,并引入上下文感知的分割机制,提升深度推断一致性。在三个数据集上评估:在火星类比环境中,生成的地形图结构一致性显著提升,尤其在斜坡和遮挡区域;岩石后方常见空洞明显减少,小石块和边缘等表面细节捕捉更准确。另两个数据集验证了方法的鲁棒性与适应性,所得视差图更精确,地形模型更一致,满足火星自主导航需求,在非遮挡与全图误差指标上均达竞争力水平。本文完整阐述从特征匹配到最终2D导航地图生成的建模流程,提供可集成于未来行星探测任务的端到端解决方案。
原文摘要 · Abstract (English)
Mars exploration requires precise and reliable terrain models to ensure safe rover navigation across its unpredictable and often hazardous landscapes. Stereoscopic vision serves a critical role in the rover's perception, allowing scene reconstruction by generating precise depth maps through stereo matching. State-of-the-art Martian planetary exploration uses traditional local block-matching, aggregates cost over square windows, and refines disparities via smoothness constraints. However, this method often struggles with low-texture images, occlusion, and repetitive patterns because it considers only limited neighbouring pixels and lacks a wider understanding of scene context. This paper uses Semi-Global Matching (SGM) with superpixel-based refinement to mitigate the inherent block artefacts and recover lost details. The approach balances the efficiency and accuracy of SGM and adds context-aware segmentation to support more coherent depth inference. The proposed method has been evaluated in three datasets with successful results: In a Mars analogue, the terrain maps obtained show improved structural consistency, particularly in sloped or occlusion-prone regions. Large gaps behind rocks, which are common in raw disparity outputs, are reduced, and surface details like small rocks and edges are captured more accurately. Another two datasets, evaluated to test the method's general robustness and adaptability, show more precise disparity maps and more consistent terrain models, better suited for the demands of autonomous navigation on Mars, and competitive accuracy across both non-occluded and full-image error metrics. This paper outlines the entire terrain modelling process, from finding corresponding features to generating the final 2D navigation maps, offering a complete pipeline suitable for integration in future planetary exploration missions.
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