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排序方式: 共有82条查询结果,搜索用时 31 毫秒
1.
Yi Wei Qingjun Li Fangnuan Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):393-400
A new orbit-attitude-vibration coupled dynamic model of the tethered solar power satellite (Tethered SPS) is established based on absolute nodal coordinate formulation. The Hamilton’s equation of the system is derived by introducing generalized momentum through Legendre transformation. The correctness of the proposed model is verified by an example. The dynamic characteristics of the Tethered SPS are studied using the symplectic Runge-Kutta method. Simulation results show that the orbital radius and the total energy of the system are well preserved. The attitude of the system is unstable when the mass of the bus system is small. However, the attitude stability is dependent on some other parameters of the system, which requires further studies. It is also found that the average tether force/deformation can be roughly estimated by simplifying the solar panel as a particle. The proposed model can be used to study the orbit-attitude-vibration coupled dynamics and control problems. 相似文献
2.
统一S波段测控信道调制指数设计方程 总被引:2,自引:0,他引:2
《遥测遥控》1999,(2)
考虑了测距音提取滤波器以及返回噪声对统一S波段卫星测控信道的影响,采用图解和数学分析两种方法详细分析了已调载波的功率效率。在此基础上,分别推导出在有、无测距音提取滤波器两种情况下,调制指数的设计方程 相似文献
3.
改性双基低特征信号推进剂研究进展 总被引:6,自引:0,他引:6
综述了国外改性双基低特征信号推进剂研究的最新进展,提出了改性双基推进剂实现低特征信号并提高性能的主要技术途径和性能指标,重点介绍了几种含有新型含能材料、新型燃速改良剂和新型键合剂的改性双基低特征信号推进利配方。 相似文献
4.
基于Lagrange方法的航天员舱外活动计算机仿真 总被引:2,自引:0,他引:2
在比较各种地面微重力模拟设备的优缺点的基础上,阐述了计算机动态仿真航天员舱外活动(EVA,Extra Vehicular Activity)的必要性。简要的概述了应用计算多刚体系统动力学对EVA进行仿真的步骤。描述了拉格朗日方程在仿真过程中的应用,建立了用于仿真的动力学方程。选取典型的EVA,得出了描述该EVA系统运动的拉格朗日动力学方程。利用反向运动学和反向动力学对该EVA进行了仿真计算,并对结果进行了分析。 相似文献
5.
扩频角度跟踪系统是实现扩频测控的前提,研究无数据包络情况下的直接扩频角度跟踪系统,在系统建模的基础上进行了数学建模、精度分析和数学仿真。结果表明:扩频角跟踪精度可达到单脉冲信标跟踪的精度;精度不仅受接收机输入端噪声的影响,还受数据自噪声的影响;高信噪比情况下,角误差通道的相移限制跟踪精度,但合理设置参数仍可实现多目标、高精度的扩频角度跟踪。 相似文献
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7.
This paper presents an analytical solution for static analysis of thick rectangular beams with different boundary conditions.Carrera's Unified Formulation (CUF) is used in order to consider shear deformation theories of arbitrary order.The novelty of the present work is that a boundary discontinuous Fourier approach is used to consider clamped boundary conditions in the analytical solution,unlike Navier-type solutions which are restricted to simply supported beams.Governing equations are obtained by employing the principle of virtual work.The numerical accuracy of results is ascertained by studying the convergence of the solution and comparing the results to those of a 3D finite element solution.Beams subjected to bending due to a uniform pressure load and subjected to torsion due to opposite linear forces are considered.Overall,accurate results close to those of 3D finite element solutions are obtained,which can be used to validate finite element results or other approximate methods. 相似文献
8.
9.
Zhu Jiang Abimael F D Loula Laboratório Nacional de Computaco Científica MCT Av Getúlio Vargas Petrópolis RJ Brazil 《南京航空航天大学学报(英文版)》2001,18(Z1)
INTRODUCTIONThe stationary incompressible Navier- Stokesequations in the primitive variables( velocity uand pressure p)- vΔu + u . u + p =f . u =0u =g inΩinΩonΓ( 1 )whereΩ is a set of R2 ,Γ its boundary,v thekinematic viscosity of the fluid,f a field of givenbody forces,and g a given field defined onΓ sa-tisfying the global conservation property∫Γg . n =0 ( 2 )n denotes the unit outer normal vector toΓ.The vorticity- velocity system of Eq.( 1 ) ,byintroducing the vorticityω… 相似文献
10.
David N. Schramm 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
To illustrate the interaction of Grand Unified Theories (GUTs), supersymmetry (SUSY), and cosmology, a worked example is carried out. This example is the dark matter problem, or “What is the dominant matter of the Universe?” It is shown that if GUTs are assumed then the primordial perturbations are probably adiabatic, if inflation is assumed then Ω = 1 and GUTs first name is probably SUSY. If Ω = 1, big bang nucleosynthesis tells us that the bulk of the matter is non-baryonic. SUSY-GUTs gives us some possible candidate inos to which massive neutrinos, axion or planetary mass black holes can be added. These candidates can be classified hot (or warm) or cold types of dark matter. It is shown that hot gives Ω = 1 and naturally gives large scale structure but does not give small scale structure or galaxy formation times, whereas cold gives small scale structure and formation times but cannot easily yield Ω = 1. It is concluded that either a hybrid of both hot and cold or non-random phases for the perturbations may be needed. 相似文献