STAR:用于大尺寸卫星图像场景图生成的首个数据集和大规模基准

Yansheng Li;Linlin Wang;Tingzhu Wang;Xue Yang;Junwei Luo;Qi Wang;Youming Deng;Wenbin Wang;Xian Sun;Haifeng Li;Bo Dang;Yongjun Zhang;Yi Yu;Junchi Yan
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摘要

卫星图像(SAI)中的场景图生成(SGG)有助于促进对地理空间场景从感知到认知的理解。在SAI中,物体在尺度和纵横比上表现出很大的变化,并且物体之间(甚至在空间不相交的物体之间)存在丰富的关系,这使得在大尺寸非常高分辨率(VHR) SAI中整体进行SGG具有吸引力。然而,缺乏这样的SGG数据集。由于大型SAI的复杂性,挖掘三元组$<;$<;主体,关系,客体$>;在美元;严重依赖于长期语境推理。因此,为小尺寸自然图像设计的SGG模型不能直接适用于大尺寸SAI。本文构建了大尺寸VHR SAI中SGG的大规模数据集STAR (Scene graph generaTion in large-size satellite imageRy),图像尺寸为512 × 768 ~ 27 860 × 31 096像素,包含超过210K个对象和超过400K个三联体。为了在大尺度SAI中实现SGG,我们提出了一个上下文感知级联认知(CAC)框架来理解基于对象检测(OBD)、对剪枝和关系预测的SAI。我们还发布了一个面向sai的SGG工具包,其中包含大约30个OBD和10个SGG方法,这些方法需要我们设计的模块进一步适应我们具有挑战性的STAR数据集。
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STAR: A First-Ever Dataset and a Large-Scale Benchmark for Scene Graph Generation in Large-Size Satellite Imagery
Scene graph generation (SGG) in satellite imagery (SAI) benefits promoting understanding of geospatial scenarios from perception to cognition. In SAI, objects exhibit great variations in scales and aspect ratios, and there exist rich relationships between objects (even between spatially disjoint objects), which makes it attractive to holistically conduct SGG in large-size very-high-resolution (VHR) SAI. However, there lack such SGG datasets. Due to the complexity of large-size SAI, mining triplets $< $<subject, relationship, object$> $> heavily relies on long-range contextual reasoning. Consequently, SGG models designed for small-size natural imagery are not directly applicable to large-size SAI. This paper constructs a large-scale dataset for SGG in large-size VHR SAI with image sizes ranging from 512 × 768 to 27 860 × 31 096 pixels, named STAR (Scene graph generaTion in lArge-size satellite imageRy), encompassing over 210K objects and over 400K triplets. To realize SGG in large-size SAI, we propose a context-aware cascade cognition (CAC) framework to understand SAI regarding object detection (OBD), pair pruning and relationship prediction for SGG. We also release a SAI-oriented SGG toolkit with about 30 OBD and 10 SGG methods which need further adaptation by our devised modules on our challenging STAR dataset.
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