排序方式: 共有90条查询结果,搜索用时 203 毫秒
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为解决传统电动无人机在覆盖作业时存在的续航时间短的问题,提出应用多架太阳能无人机进行覆盖作业。首先,在建立了应用于覆盖作业的太阳能无人机的能量模型的基础上,提出了能量流动效率这一指标来评价太阳能无人机在作业过程中对能量的利用率。其次,针对边界存在障碍物的凹多边形区域和内部含障碍物的多边形区域,以总作业完成时间最短为优化目标,提出基于无向图搜索方法的覆盖路径优化模型,定义约束方程限制无人机按照一定规则访问无向图中的节点,通过混合整数线性规划的方法求解每架无人机的最优飞行路径。再次,考虑无人机转弯时的姿态变化对能量流动效率的影响,将总作业完成时间最短和总能量流动效率最高同时作为优化目标,建立双目标优化方程,在首先以作业时间最短为优化目标进行求解的基础上,通过有限遍历的方式选择使能流效率和作业时间相对最优的覆盖飞行方向及飞行路径。大量仿真实验表明,所提的优化模型选取不同的优化目标,应用于不同形状的待覆盖区域,适用性广,在工程上应用范围广、可行性强。 相似文献
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M.J. Birch J.K. Hargreaves 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):678-699
This study extends the investigation of the ripples in the solar wind and the interplanetary magnetic field at L1 reported by Birch and Hargreaves (2020) to cover heliospheric distances from 1 to 40 AU, using data from the Voyager 2, Ulysses, Juno, Cassini, Themis and Apollo-12 spacecraft. The ripples were extracted from the source data using a bandpass filter which reduces the noise component of the source data while removing long-term trends. The ripples were found to propagate throughout the heliosphere with an average periodicity of 26 min, without significant attenuation relative to the background. They also permeated within the magnetospheres of Earth, Jupiter and Saturn with an average periodicity of 25 min, though with some attenuation relative to the solar wind, especially in the case of Jupiter. Within the planetary magnetospheres, the ripples were suppressed by the intense fields in close proximity to each planet, and though the distance varied at which this cutoff occurred, the flux density was very similar in all three cases. 相似文献
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为明确双吸叶轮两侧叶轮之间的径向轮盘凸台尺寸变化对其总体性能及内部流场的影响,探索不同尺寸轮盘结构叶轮的流动损失机理,基于双吸叶轮两侧非均衡进气条件,采用数值方法对五种径向轮盘尺寸双吸叶轮的三维粘性流场进行了模拟研究。研究结果表明:从双吸叶轮最优性能及最高流动稳定性观点出发,均要求两侧叶轮之间的径向轮盘凸台超出叶片尾缘一定范围;具体超出尺寸范围则需要通过对双吸叶轮的压比、效率性能目标进行折衷确定。径向轮盘凸台尺寸的改变明显影响双吸叶轮两侧叶轮的流量分配,进而影响扩压器内分离流动损失大小及双吸叶轮的整体性能。另外,相比于较大径向轮盘凸台,无径向轮盘凸台结构更容易造成双吸叶轮两侧叶轮流量差距悬殊。 相似文献
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Sylvie Sahal-Bréchot Milan S. Dimitrijević Nicolas Moreau Nabil Ben Nessib 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
“Stark” broadening theories and calculations have been extensively developed for about 50 years and can now be applied to many needs, especially for accurate spectroscopic diagnostics and modeling. This requires the knowledge of numerous collisional line profiles. Nowadays, the access to such data via an online database becomes essential. STARK-B is a collaborative project between the Astronomical Observatory of Belgrade and the Laboratoire d’Étude du Rayonnement et de la matière en Astrophysique (LERMA). It is a database of calculated widths and shifts of isolated lines of atoms and ions due to electron and ion collisions (impacts). It is devoted to modeling and spectroscopic diagnostics of stellar atmospheres and envelopes, laboratory plasmas, laser equipments and technological plasmas. Hence, the domain of temperatures and densities covered by the tables is wide and depends on the ionization degree of the considered ion. STARK-B has been fully opened since September 2008 and is in free access. 相似文献
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Christina Plainaki Tim A. Cassidy Valery I. Shematovich Anna Milillo Peter Wurz Audrey Vorburger Lorenz Roth André Galli Martin Rubin Aljona Blöcker Pontus C. Brandt Frank Crary Iannis Dandouras Xianzhe Jia Davide Grassi Paul Hartogh Alice Lucchetti Melissa McGrath Valeria Mangano Alessandro Mura Stefano Orsini Chris Paranicas Aikaterini Radioti Kurt D. Retherford Joachim Saur Ben Teolis 《Space Science Reviews》2018,214(1):40
Despite the numerous modeling efforts of the past, our knowledge on the radiation-induced physical and chemical processes in Europa’s tenuous atmosphere and on the exchange of material between the moon’s surface and Jupiter’s magnetosphere remains limited. In lack of an adequate number of in situ observations, the existence of a wide variety of models based on different scenarios and considerations has resulted in a fragmentary understanding of the interactions of the magnetospheric ion population with both the moon’s icy surface and neutral gas envelope. Models show large discrepancy in the source and loss rates of the different constituents as well as in the determination of the spatial distribution of the atmosphere and its variation with time. The existence of several models based on very different approaches highlights the need of a detailed comparison among them with the final goal of developing a unified model of Europa’s tenuous atmosphere. The availability to the science community of such a model could be of particular interest in view of the planning of the future mission observations (e.g., ESA’s JUpiter ICy moons Explorer (JUICE) mission, and NASA’s Europa Clipper mission). We review the existing models of Europa’s tenuous atmosphere and discuss each of their derived characteristics of the neutral environment. We also discuss discrepancies among different models and the assumptions of the plasma environment in the vicinity of Europa. A summary of the existing observations of both the neutral and the plasma environments at Europa is also presented. The characteristics of a global unified model of the tenuous atmosphere are, then, discussed. Finally, we identify needed future experimental work in laboratories and propose some suitable observation strategies for upcoming missions. 相似文献
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喷雾场测试技术研究进展 总被引:2,自引:0,他引:2
喷注器的喷雾质量直接影响推进剂在燃烧室中的燃烧效率。为了准确获得其喷雾特性,以收集法、PDA及PIV为代表的喷雾场测试技术一直在不断发展和完善中,其中PIV技术与数字全息技术相结合发展的DHPIV技术具有较好的应用前景。对近年来的喷雾场测试技术进行了综述,介绍了各种测试技术的原理、特点及其在喷雾场测试中存在的问题。 相似文献