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Non-uniform gravity field model on board learning during small bodies PROXIMITY OPERATIONS

机译:小型机构接近操作期间的非均匀重力场模型

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Proximity operations about asteroids are challenging because of the non-uniform gravity field that they generate, which is largely unknown even during the proximity operation phase. Much of their characterization, in fact, is based on insitu observations: mass is estimated thanks to flybys, while imaging the asteroid under various lighting conditions enables the reconstruction of the shape model and the determination of the spin rate. This allows ground controllers to understand the bodys gravitational field, identify a model and safely guide the satellite. Moreover, hovering and imaging the body are fundamental science phases, to characterize the small object composition and nature, and the gravity field reconstruction plays a fundamental role in the remote science data fusion and scientic knowledge of the specic object enhancement. Those operations became challenging in case the orbiting platform is a microsatellite, a CubeSat or, in general, a platform with reduced communication capabilities to ground. Even more challenging is the case is which a distributed system of platforms (such as a swarm of CubeSats) is considered and a relatively high autonomy is required. This paper proposes a new approach to reconstruct the gravity eld of either unknown or partially known objects using a modified Hopfield Neural Network (HNN). In particular, the gravity field of the object is represented through a spherical harmonics expansion the coefficients of which must be estimated. In general, the parametric identification of these coefficients can be written as an optimization problem. HNNs for parametric identification have been extensively studied in past years: this work, starting from the methodology state of the art, steps forward by extending their application to a new scenario and tuning them for online running; the gravity field coefficients are identified in flight and on board, by means of a specifically tailored HNN. Due to the inherent structure of the HNN, the proced
机译:关于小行星的接近操作是具有挑战性的,因为它们产生的非均匀重力场,即使在接近操作阶段也是很大程度上未知的。其特征在于,实际上是基于Insitu观察:据估计捕获群体,同时在各种照明条件下成像小行星,使得能够重建形状模型和旋转速率的确定。这允许地面控制器理解Bodys Gravitational场,识别模型并安全引导卫星。此外,悬停和成像身体是基本的科学阶段,以表征小物体组成和性质,并且重力场重建在远程科学数据融合和科学知识中起着基本作用,对象对象增强。这些操作在轨道平台是微卫星,立方体或一般的平台上,这些操作变得具有挑战性。甚至更具挑战是这种情况,哪种平台的分布式系统(例如群群)被认为是需要的,并且需要相对高的自主权。本文提出了一种新方法来使用改进的Hopfield神经网络(HNN)重建未知或部分已知的物体的重力eld。特别地,物体的重力场通过球面谐波扩展表示,其必须估计其系数。通常,可以写入这些系数的参数识别作为优化问题。过去几年已经广泛研究了参数识别的HNN:这项工作从本领域的方法,通过将应用程序扩展到新的场景并调整它们以进行在线运行的步骤进行前进;通过专门定制的HNN在飞行和船上识别重力场系数。由于HNN的固有结构,程序

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