基于拉丁超立方抽样的五孔探针标定方法

为提高五孔探针的标定效率,研究了一种采用拉丁超立方抽样技术开展变马赫数五孔探针标定的试验方法.马赫数在0.2～0.5范围内的对比试验结果表明:采用改进的拉丁超立方抽样标定技术可使攻角与侧滑角的拟合误差较一般拉丁超立方抽样方法下降14.3％～28.6％,且攻角与侧滑角的拟合方均根误差均在1°以内,马赫数的拟合方均根误差不...     

基于改进ORB的月面着陆视觉导航的配准方法

月球探测器在下降着陆过程中探测到的月面图像灰度均匀,缺少纹理信息,而视觉辅助导航采用传统ORB算法对灰度均匀的月面图像检测出的特征点数量较少,容易出现团簇现象,因此提出一种基于改进ORB算法的图像特征提取与匹配算法.首先对月面图像构建金字塔尺度空间模型,设置自适应阈值并构建掩膜逐一分块检测特征点;然后采用非极大值抑制使...     

无强波构型理论发展现状研究

本文引入了一种由Busemann超声速双翼理论发展而来的无强激波构型,该构型可明显消弱超声速飞行时带来的波阻和声爆。文中分析了无强波构型的机理和气动特性,介绍了该构型理论研究和应用研究进展,并探讨了该构型在超声速飞行器设计应用中的关键性问题。该理论为未来低声爆超声速飞机的设计提供了一个全新的思路,是未来超声速/高超声速飞行器发展必要的技术基础。     

模块化月球表层采样力学模型

因不受作业空间的限制，月球表层采样机具设计形式多样，为建模分析带来较大难度。为避免不同结构机具分析时重复建模，建立了一种模块化的月球表层采样力学模型。该模型将复杂的采样机具拆分成若干个基本面单元，基于朗肯土压力理论、最大抗剪强度理论和地基极限承载力理论对面单元在采样过程中的受力进行分析，组合各个面单元所受到的力获得复杂机具的力学模型。基于不同机具形式与贯入角度的模拟月壤贯入试验，对理论模型进行了试验验证，通过引入月壤密度沿深度的影响修正公式，将理论模型的误差率降低至8.2%。结果证明该力学模型和模块化理论可行，为后期月球表层采样机具的设计研发提供了参考。     

Effect of the continental shelf in seasonal oceanographic conditions at the Northern edge of the Eastern Tropical Pacific

The continental shelf in front of Nayarit is located in the northern limit of the tropical Eastern Pacific, characterized by constituting a convergence zone of different masses of water, forming an area of significant hydrographic variability. Based on satellite remote sensing data and reanalysis between 2003 and 2019 of sea surface temperature (SST), wind stress, Ekman velocity, and geostrophic velocity, the contribution of the seasonal cycle to the variability of the study area were analyzed through climatological means, Hovmöhler diagrams, and Empirical Orthogonal Functions. The results show that in the zone in front of Matanchén Bay (21.5 °N) and the adjacent continental shelf, there is a core of warm surface water. The distribution of the SST is explained by the seasonal pattern of meridional/zonal variability in the thermal gradient, where the EOFs show the influence of the annual scale in both modes, with the only difference being that the first describes the meridional gradient as the dominant signal (66.2%), and the second shows the zonal behavior of the thermal gradient (16.6%). The summer weakening of the wind stress and Ekman speed is the product of the irregular shape of the coastline, the extension of the continental shelf, and the divergence of the North American monsoon around 21°N, whereas during the rest of the year an intensification of these parameters prevailed in front of Cabo Corrientes. On the other hand, the intense geostrophic flow in summer does not contribute to the increase in SST on the continental shelf because it diverges around 22.5°N. Likewise, during the winter, the formation of a cyclonic geostrophic gyre located inside the continental shelf, between the coast and the Marías Islands, stands out.     

我国载人航天电源系统的技术发展成就及趋势

载人航天电源系统是一个庞大的系统工程，状态复杂、可靠性要求高、技术难度大。本文在阐述我国载人航天电源系统组成和特点的基础上，从电源系统架构、太阳电池翼、储能电池组、并网控制以及在轨维修与更换等方面，详细论述了我国载人航天电源系统的各阶段技术突破和技术引领，并对后续载人月球探测提出展望，梳理了能源系统重点研究方向和关键技术，为未来载人月球探测任务顺利实施奠定技术基础。     

Gas-dynamic approach to the theory of non-linear ion-acoustic waves in plasma with Kaniadakis’ distributed species

The non-linear theory of ion-acoustic waves in two-spesies isotropic collisionless plasma is developed. Both light electron and heavy ion species in the plasma are distributed with Kaniadakis’ statistics. Kaniadakis’ gas law is derived. The exact formula for the Sagdeev pseudopotential in parametric form is derived by the method based on the integration of the inverse function. The pseudopotential is analyzed. It is shown that periodic ion-acoustic waves and solitons are possible in the studied plasma. The differential equation describing the profile of the ion concentration in the wave is derived. The profiles of this concentration in the periodic ion-acoustic wave and soliton are calculated.     

一种多源测距与视觉惯性融合的月球车定位方法

针对月球车月面探测活动任务中对高精度定位的需求,当前视觉惯性定位方法存在误差累积,并且在缺乏先验环境信息时无法消除,基于三角测量原理的无线电定位方法可以通过测量接收端到至少三个不同发射端的距离来确定目标物体位置,但需要架设三台以上基站,因此难以满足月面环境下大范围定位的需求。文章提出了一种基于基站无线测距和视觉惯性里程计融合定位方法,以解决上述定位手段存在的问题。该方法首先利用视觉惯性里程计构建的环境模型将WIFI、UHF和UWB三类无线电基站测距信息进行融合,然后将测距结果和视觉IMU信息进行位置联合解算来确定月球车位置,最后在Matlab和Gazebo软件平台上进行仿真验证,在距离基站最远行进1500米的条件下实现了0.92米定位误差。实验结果表明,该方法能够在满足月面探测任务对于精准定位的需求。     

载人月球科研试验站建设规划及设想

进入21世纪以来，月球再次成为太空探索的焦点，许多国家提出各自的探月计划。区别于在美国60年前完成的阿波罗工程，未来月球探测的重点聚焦月球的长期建设与开发。如何充分利用当前的技术积累，在有限的运载能力和合理的发射运营成本条件下，建设载人月球科研试验站，实现月球极端环境下的长期运行是一个值得关注和研究的课题。结合当前国内外载人航天与探月工程发展情况，提出我国载人月球科研试验站人货分落、分段建设的规划设想。通过对安全性设计、乘组规模、环控生保需求、选址等展开分析，明确初步月球科研试验站建设需求，并提出满足2人长期月面驻留“2+1”构型月球科研试验站方案。     

Hardware qualification for scientific ballooning missions

The European Stratospheric Balloon Observatory (ESBO) initiative aims at simplifying the access to stratospheric balloon missions. We plan to provide platforms and support with instrument design in order to support scientists. During the design process, the inevitable question of qualification for the harsh flight conditions arises. Unfortunately, there is no existing standard for qualification of stratospheric ballooning hardware. Thus, we developed a qualification procedure for use within ESBO and similar projects.In this paper, we present our analysis of the environmental conditions in the stratosphere. While conditions at typical balloon float altitudes are similar to the space environment, there are also some relevant differences. For example, the thermal environment is dominated by radiation and thermal conduction, but the remaining atmosphere still supports a certain amount of convection. The remaining atmospheric pressure in the stratosphere also leads to reduced arcing distances. Vibrational loads are far less than for space missions, but quasi-static or shock loads may occur. The criticality of radiation increases with mission duration.Based on the environmental conditions, we present the qualification procedures for ESBO, which are based on the European Cooperation for Space Standardization (ECSS) standards for space systems. Overtesting against too high requirements leads to overengineering, driving mission cost and mitigating the advantages of balloons over space missions. Therefore, we modified the ECSS standards to fit typical scientific ballooning missions over several days at altitudes up to 40 km. Furthermore, we analyzed design rules for space systems with regard to their relevance for scientific ballooning, including material and component selection. We present the experience from the hardware qualification process for the ESBO prototype STUDIO (Stratospheric UV Demonstrator of an Imaging Observatory). Even though boundary conditions are different for each individual mission, we aimed for a broader approach: We investigated more general requirements for scientific ballooning missions to support future flights.