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671.
针对行星表面轻量化自主探测任务,基于仿生思想设计了一种仿海胆结构的十二足球形机器人,其具备自主改变构型以贴合复杂地形的能力,可实现无倾覆、高容错的全向运动;基于数据驱动方法,对该机器人设计了一种数据高效的无模型强化学习运动策略,可实现无先验知识的从0到1步态训练以及步态的实物样机快速部署。通过在平面地形和非结构化地形中对其进行仿真实验,验证了经过训练的机器人具备自主运动、适应非结构地形等能力;通过与常用基准策略进行对比,证实了本文提出的运动策略具有训练高效、鲁棒性好的优势;最后通过开发原理样机,开展实物实验验证了仿真环境中所生成的步态在真实物理环境中的动力学可行性。 相似文献
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《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(1):1089-1097
We report dusty photo-ionization models for two Planetary Nebulae NGC 2452 and IC 2003, which have [WR] type central stars, using 1D photo-ionization code Cloudy17.02. We used the medium resolution optical spectra and archival IRAS photometry to constrain our models. The physical size of the ionized nebula derived using accurate distance measurements and absolute H flux available in the literature were used as additional constrains. We examine the importance of photo-electric heating and found that models with and without considering photo-electric heating do not make significant difference for both PNe for the MRN grain size distribution considered in this study. We derive the nebular elemental abundances of these PNe by the empirical method as well as by making dusty photo-ionization models. The values of N/O ratios for both PNe obtained from our models are lower than their respective values arrived using empirical methods. The central stars are assumed to be black bodies and the photospheric temperatures derived respectively for NGC 2452 and IC 2003 from their best fit models are 182 kK and 155 kK and their respective luminosities are 630 and 1015. We propose that both the PNe were resulted from low-mass progenitors of mass 2.8 M⊙. 相似文献
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《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(1):816-828
Asteroid exploration has become a research hotspot, and anchoring probes to asteroids is essential for in situ scientific detections. The influence of ultrasonic drilling force-closure anchoring parameters on the anchoring performance and its influence mechanism are studied based on discrete element simulation. An anchoring simulation model is established after calibrating virtual asteroid soil, and its validity is verified by anchoring experiments. Discrete element simulations are performed to study the effect of cross-sectional shape and longitudinal cross-sectional shape of anchoring rods on anchoring force. The internal influence mechanism of anchor configurations on the anchoring force is analyzed by extracting the number of stressed particles in the simulation area. The anchoring force has a positive correlation with the cross-sectional area. The rotation of non-circular anchors causes fluctuations in the anchoring force. The effect of the anchored material strength on the anchoring force is studied with the calibrated virtual asteroid soil. The relationship between anchoring force and anchoring parameters is studied, and the optimal anchoring angle is 54° for anchored material strength of 100 kPa. Finally, the variation of the anchoring force with the direction of external force is studied. This work can guide the anchor configuration design and the anchoring condition parameter optimization. 相似文献
676.
针对月面超远距离移动规划任务因缺乏精确全局信息而导致的规划路径可通行性不足问题,提出了月面道路拓扑网的构建设想及相应路径规划技术,凭借复杂道路网络的连通能力确保巡视器超远距离规划路径的可通行性。首先进行月面道路拓扑网的设计方法研究,分别提出了基于滑动最优泊松采样算法的网络节点设计方法和基于均匀领邻网络拓扑模型网络结构设计方法,使月面道路网网络节点分布均匀、密度适中且覆盖完整,网络连接合理且各路径尽量远离障碍区域。然后进行基于月面道路拓扑网的超远距离移动规划研究,分析了基于月面道路拓扑网路径规划技术的概率完备性和整体可通行概率,并提出了基于月面道路拓扑网的K优路径规划方法,通过道路网的连通性来提高超远距离移动探测任务的整体可通行概率。最后以阿波罗两次登月任务的着陆点之间进行超远距离转移任务为仿真场景,验证了本方法的有效性。 相似文献