Toward the recognition of spacecraft feature components: A new benchmark and a new model

IF 2.7 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Linwei Qiu, Liang Tang, Rui Zhong
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引用次数: 4

Abstract

Countries are increasingly interested in spacecraft surveillance and recognition which play an important role in on-orbit maintenance, space docking, and other applications. Traditional detection methods, including radar, have many restrictions, such as excessive costs and energy supply problems. For many on-orbit servicing spacecraft, image recognition is a simple but relatively accurate method for obtaining sufficient position and direction information to offer services. However, to the best of our knowledge, few practical machine-learning models focusing on the recognition of spacecraft feature components have been reported. In addition, it is difficult to find substantial on-orbit images with which to train or evaluate such a model. In this study, we first created a new dataset containing numerous artificial images of on-orbit spacecraft with labeled components. Our base images were derived from 3D Max and STK software. These images include many types of satellites and satellite postures. Considering real-world illumination conditions and imperfect camera observations, we developed a degradation algorithm that enabled us to produce thousands of artificial images of spacecraft. The feature components of the spacecraft in all images were labeled manually. We discovered that direct utilization of the DeepLab V3+ model leads to poor edge recognition. Poorly defined edges provide imprecise position or direction information and degrade the performance of on-orbit services. Thus, the edge information of the target was taken as a supervisory guide, and was used to develop the proposed Edge Auxiliary Supervision DeepLab Network (EASDN). The main idea of EASDN is to provide a new edge auxiliary loss by calculating the L2 loss between the predicted edge masks and ground-truth edge masks during training. Our extensive experiments demonstrate that our network can perform well both on our benchmark and on real on-orbit spacecraft images from the Internet. Furthermore, the device usage and processing time meet the demands of engineering applications.

面向航天器特征部件的识别:一个新的基准和一个新模型
各国对航天器监视和识别越来越感兴趣,这在在轨维护、空间对接和其他应用中发挥着重要作用。包括雷达在内的传统探测方法有许多限制,例如成本过高和能源供应问题。对于许多在轨服务航天器来说,图像识别是一种简单但相对准确的方法,可以获得足够的位置和方向信息来提供服务。然而,据我们所知,很少有实用的机器学习模型专注于航天器特征组件的识别。此外,很难找到大量的在轨图像来训练或评估这样的模型。在这项研究中,我们首先创建了一个新的数据集,其中包含带有标记组件的在轨航天器的大量人工图像。我们的基础图像来源于3DMax和STK软件。这些图像包括许多类型的卫星和卫星姿态。考虑到现实世界的照明条件和不完美的相机观测,我们开发了一种退化算法,使我们能够生成数千张航天器的人造图像。所有图像中航天器的特征部件都是手动标记的。我们发现,直接使用DeepLab V3+模型会导致边缘识别较差。定义不周的边缘提供了不精确的位置或方向信息,并降低了在轨服务的性能。因此,将目标的边缘信息作为监督指南,并用于开发所提出的边缘辅助监督DeepLab网络(EASDN)。EASDN的主要思想是通过计算训练期间预测的边缘掩码和真实边缘掩码之间的L2损耗来提供新的边缘辅助损耗。我们的大量实验表明,我们的网络在我们的基准和来自互联网的真实在轨航天器图像上都能表现良好。此外,设备的使用和处理时间满足工程应用的要求。
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来源期刊
Astrodynamics
Astrodynamics Engineering-Aerospace Engineering
CiteScore
6.90
自引率
34.40%
发文量
32
期刊介绍: Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.
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