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基于视觉的着陆器脚垫与火卫一模拟表面接触建模方法

Vision-Based Approach in Contact Modelling between the Footpad of the Lander and the Analogue Representing Surface of Phobos.

作者信息

Cała Marek, Kohut Piotr, Holak Krzysztof, Wałach Daniel

机构信息

Department of Geomechanics, Civil Engineering and Geotechnics, Faculty of Civil Engineering and Resource Management, AGH University of Science and Technology, al. Mickiewicza 30, 30-059 Kraków, Poland.

Department of Robotics and Mechatronics, Faculty of Mechanical Engineering and Robotics, AGH University of Science and Technology, al. Mickiewicza 30, 30-059 Kraków, Poland.

出版信息

Sensors (Basel). 2021 Oct 22;21(21):7009. doi: 10.3390/s21217009.

Abstract

Identifying solar system surface properties of celestial bodies requires the conducting of many tests and experiments in conditions similar to those found on various objects. One of the first tasks to be solved by engineers is determining the contact condition between the lander and the surface of a given celestial body during landing in a microgravity environment. This paper presents the results of experimental studies and numerical simulations of the contact phenomenon between the lander foot model and the Phobos analogue. The main goal of the experimental tests was to obtain measured deformation data of the studied analogues using 2D and 3D vision systems, which were employed to analyze the behavior of the lander foot and the surface of the studied analogue itself and to calibrate the numerical models. The analogue representing the Phobos surface was foam concrete. The variable parameters in the study were the analogue thickness and the lander foot velocity at the time of contact. Tests were conducted for three different contact velocities of 1.2 m/s, 3.0 m/s, and 3.5 m/s. Taking into account the mass of the lander foot model, kinetic energies of 30.28 J, 189.22 J, and 257.56 J were obtained. The results showed that at low contact velocities, and thus low kinetic energies, no significant differences in behavior of the material directly under the lander foot were observed, and similar values of forces in the lander foot were obtained. For higher contact velocities, the behavior of analogues with varying thicknesses was different, resulting in different values of analogue deformation and dynamics of increments and decrements of force in the lander foot itself. Although performed on a single material, the experiments revealed different behaviors depending on its thickness at the same impact energy. This is an essential guideline for engineers who need to take this fact into account when designing the lander itself.

摘要

识别天体的太阳系表面特性需要在与各种天体上发现的条件相似的情况下进行许多测试和实验。工程师要解决的首要任务之一是确定着陆器在微重力环境下着陆时与给定天体表面之间的接触条件。本文介绍了着陆器足部模型与火卫一模拟物之间接触现象的实验研究和数值模拟结果。实验测试的主要目标是使用二维和三维视觉系统获取所研究模拟物的测量变形数据,这些系统用于分析着陆器足部和所研究模拟物本身表面的行为,并校准数值模型。代表火卫一表面的模拟物是泡沫混凝土。研究中的可变参数是模拟物厚度和接触时着陆器足部的速度。针对1.2米/秒、3.0米/秒和3.5米/秒这三种不同的接触速度进行了测试。考虑着陆器足部模型的质量,分别获得了30.28焦、189.22焦和257.56焦的动能。结果表明,在低接触速度下,即低动能下,未观察到着陆器足部正下方材料行为的显著差异,并且着陆器足部的力值相似。对于较高的接触速度,不同厚度模拟物的行为不同,导致模拟物变形值以及着陆器足部自身力的增减动态不同。尽管实验是在单一材料上进行的,但实验揭示了在相同冲击能量下,根据其厚度不同会有不同的行为。这对于在设计着陆器本身时需要考虑这一事实的工程师来说是一个重要的指导原则。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e66c/8588339/7a071bfca056/sensors-21-07009-g001.jpg

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