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41.
Pengbin Guo Jian Sun Shuling Hu Ju Xue 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(3):787-798
Pulsar navigation is a promising navigation method for high-altitude orbit space tasks or deep space exploration. At present, an important reason for restricting the development of pulsar navigation is that navigation accuracy is not high due to the slow update of the measurements. In order to improve the accuracy of pulsar navigation, an asynchronous observation model which can improve the update rate of the measurements is proposed on the basis of satellite constellation which has a broad space for development because of its visibility and reliability. The simulation results show that the asynchronous observation model improves the positioning accuracy by 31.48% and velocity accuracy by 24.75% than that of the synchronous observation model. With the new Doppler effects compensation method in the asynchronous observation model proposed in this paper, the positioning accuracy is improved by 32.27%, and the velocity accuracy is improved by 34.07% than that of the traditional method. The simulation results show that without considering the clock error will result in a filtering divergence. 相似文献
42.
Yu Jiang Hexi Baoyin Hengnian Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(5):1371-1385
We investigate the orbital stability close to the unique L4-point Jupiter binary Trojan asteroid 624 Hektor. The gravitational potential of 624 Hektor is calculated using the polyhedron model with observational data of 2038 faces and 1021 vertexes. Previous studies have presented three different density values for 624 Hektor. The equilibrium points in the gravitational potential of 624 Hektor with different density values have been studied in detail. There are five equilibrium points in the gravitational potential of 624 Hektor no matter the density value. The positions, Jacobian, eigenvalues, topological cases, stability, as well as the Hessian matrix of the equilibrium points are investigated. For the three different density values the number, topological cases, and the stability of the equilibrium points with different density values are the same. However, the positions of the equilibrium points vary with the density value of the asteroid 624 Hektor. The outer equilibrium points move away from the asteroid’s mass center when the density increases, and the inner equilibrium point moves close to the asteroid’s mass center when the density increases. There exist unstable periodic orbits near the surface of 624 Hektor. We calculated an orbit near the primary’s equatorial plane of this binary Trojan asteroid; the results indicate that the orbit remains stable after 28.8375?d. 相似文献
43.
随着飞机液压系统向高压化、大功率化方向发展,液压系统的发热及温升问题受到了广泛关注。柱塞泵作为液压系统中重要的能量转换装置,对液压系统的功率损失和温度有重大的影响,良好的柱塞泵的热分析对液压系统的热设计和温度控制有重要的意义。然而传统的柱塞泵热分析方法,如平均油温法、软件仿真法和热节点网络法,因不够准确、高效和简洁而不能满足现代飞机液压系统热分析和热设计的相关需求。本文针对飞机液压系统柱塞泵发热的相关问题,采用基于集总参数的热网络分析方法,建立了柱塞泵热网络模型,通过对柱塞泵不同工况下的仿真,验证了模型的有效性和准确性,为柱塞泵及液压系统的热分析提供了参考。 相似文献
44.
空间站主动热控系统的作用是提供和保持航天员、仪器设备和结构部件所要求的温度、湿度和风速等热环境。本文以空间载荷机柜为热控系统的基本单元,建立了以单相流体循环回路为基础、采用液冷结合风冷的冷却方式的载荷机柜数学模型;介绍了模糊增量控制算法的工作原理;提出了采用模糊增量控制算法,以液冷支路进出口温差和风冷支路冷却量占总冷却量的比值为控制目标的反馈控制策略。同时文章采用数值模拟方法研究了控制系统的动态响应效果。仿真结果显示,模糊增量控制算法具有响应迅速、超调量小、无静态误差的特点,控制策略满足有效性、稳定性和高精确度的要求。 相似文献
45.
Categorical bias in location memory in geometric spaces is well established. The present study assessed the presence of the bias in locating eyes in images of human faces. Participants were presented with digital faces and indicated the position of one of the eyes in both upright and inverted orientations. Biases resulted from participants using multiple sources of accessible information. No differences were found for upright vs. inverted face images. Overall, the data were consistent with the retrieval category adjustment model. These distortions may be considered within the forensic context, when eyewitnesses work with a sketch artist or use a computer program to generate an image of the culprit. 相似文献
46.
S.A. Demin Y.A. Nefedyev A.O. Andreev N.Y. Demina S.F. Timashev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(2):639-644
The analysis of turbulent processes in sunspots and pores which are self-organizing long-lived magnetic structures is a complicated and not yet solved problem. The present work focuses on studying such magneto-hydrodynamic (MHD) formations on the basis of flicker-noise spectroscopy using a new method of multi-parametric analysis. The non-stationarity and cross-correlation effects taking place in solar activity dynamics are considered. The calculated maximum values of non-stationarity factor may become precursors of significant restructuring in solar magnetic activity. The introduced cross-correlation functions enable us to judge synchronization effects between the signals of various solar activity indicators registered simultaneously. 相似文献
47.
An improved numerical method that can construct Halo/Lissajous orbits in the vicinity of collinear libration points in a full solar system model is investigated. A full solar system gravitational model in the geocentric rotating coordinate system with a clear presentation of the angular velocity relative to the inertial coordinate system is proposed. An alternative way to determine patch points in the multiple shooting method is provided based on a dynamical analysis with Poincare′sections. By employing the new patch points and sequential quadratic programming, Halo orbits for L_1, L_2, and L_3 points as well as Lissajous orbits for L_1 and L_2 points in the EarthMoon system are generated with the proposed full solar system gravitational model to verify the effectiveness of the proposed method. 相似文献
48.
Fuyu Sun Jianping Zhou Zheyao Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):189-206
This study proposes a new simulation platform named Simulation Integrated Management (SIM) for the analysis of parallel and distributed systems. The platform eases the process of designing and testing both applications and architectures. The main characteristics of SIM are flexibility, scalability, and expandability. To improve the efficiency of project development, new models of early-warning satellite system were designed based on the SIM platform. Finally, through a series of experiments, the correctness of SIM platform and the aforementioned early-warning satellite models was validated, and the systematical analyses for the orbital determination precision of the ballistic missile during its entire flight process were presented, as well as the deviation of the launch/landing point. Furthermore, the causes of deviation and prevention methods will be fully explained. The simulation platform and the models will lay the foundations for further validations of autonomy technology in space attack-defense architecture research. 相似文献
49.
50.
Mingying Huo Giovanni Mengali Alessandro A. Quarta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(10):2617-2627
Propellantless continuous-thrust propulsion systems, such as electric solar wind sails, may be successfully used for new space missions, especially those requiring high-energy orbit transfers. When the mass-to-thrust ratio is sufficiently large, the spacecraft trajectory is characterized by long flight times with a number of revolutions around the Sun. The corresponding mission analysis, especially when addressed within an optimal context, requires a significant amount of simulation effort. Analytical trajectories are therefore useful aids in a preliminary phase of mission design, even though exact solution are very difficult to obtain. The aim of this paper is to present an accurate, analytical, approximation of the spacecraft trajectory generated by an electric solar wind sail with a constant pitch angle, using the latest mathematical model of the thrust vector. Assuming a heliocentric circular parking orbit and a two-dimensional scenario, the simulation results show that the proposed equations are able to accurately describe the actual spacecraft trajectory for a long time interval when the propulsive acceleration magnitude is sufficiently small. 相似文献