空间站柔性展开机构仿真方法研究

空间站展开机构是典型的大型多柔体系统,其展开收拢过程涉及非线性大变形以及接触碰撞问题。首先采用绝对节点坐标法作为柔性体的建模方法,建立了梁单元的有限元单元格式,然后基于拉格朗日方法和Hertz接触理论建立了考虑接触碰撞问题的柔性多体系统动力学方程,采用向后差分方法数值求解柔性多体系统的微分代数方程,最后以自由梁、简支梁和柔性单摆进行数学仿真验证。结果表明,该方法可用作我国空间站大型柔性太阳电池翼的设计分析参考。     

Effect of Stagnation Temperature on the Supersonic Two Dimensional Plug Nozzle Conception. Application for Air

When the stagnation temperature of a perfect gas increases, the specific heats and their ratio do not remain constant any more and start to vary with this temperature. The gas remains perfect, its state equation remains always valid, except it will name in more calori-cally imperfect gas or gas at High Temperature. The goal of this research is to trace the profiles of the supersonic plug nozzle when this stagnation temperature is taken into account, lower than the threshold of dissociation of the molecules, by using the new formula of the Prandtl Meyer function, and to have for each exit Mach number, several nozzles shapes by changing the value of this temperature. A study on the error given by the PG (perfect gas) model compared to our model at high temperature is presented. The comparison is made with the case of a calorically perfect gas aiming to give a limit of application of this model. The application is for the air.     

体-翼干扰区热环境特性分析及预测

高速飞行器的体—翼干扰区热流精确预测对于飞行器生存能力与战术性能的提高具有重要的 意义,是高性能飞行器设计水平的一个重要标志。由于体—翼干扰区流场的复杂性,目前尚 无满足工程设计要求的热环境预测方法,在分析体—翼流场特性的基础上应用文献［1 ］的压力—热流关系式,提出体—翼干扰区的热流预测方法,即压力由N-S数值解给出,热 流应用压力—热流关系式得到,炮风洞的实验结果验证了本文预测方法的可 靠性 。
     

基于控制理论方法的翼型最大升力优化设计

使用控制理论方法建立了对翼型最大升力优化设计的模型.并且在给定约束力矩系数和约束翼型面积条件下对GAW-1低速高升力翼型进行了最大升力状态实例优化设计,验证了使用粘性伴随方法建立的以翼型最大升力为目标的多约束优化模型的有效性。     

含孔边裂纹有限大单块板的解析变分解法

本文利用复变函数方法导出含孔边双侧直线裂纹有限大板应力与位移的全场表达式,满足所有基本方程式、裂纹表面边界条件与复连通域位移单值条件。应用变分原理满足其余边界条件并求解应力强度因子。变分方程中只有线积分。故本方法计算效率较高。     

The COMPLEIK subroutine of the IONORT-ISP system for calculating the non-deviative absorption: A comparison with the ICEPAC formula

The present paper proposes to discuss the ionospheric absorption, assuming a quasi-flat layered ionospheric medium, with small horizontal gradients. A recent complex eikonal model (Settimi et al., 2013b) is applied, useful to calculate the absorption due to the ionospheric D-layer, which can be approximately characterized by a linearized analytical profile of complex refractive index, covering a short range of heights between h₁ = 50 km and h₂ = 90 km. Moreover, Settimi et al. (2013c) have already compared the complex eikonal model for the D-layer with the analytical Chapman’s profile of ionospheric electron density; the corresponding absorption coefficient is more accurate than Rawer’s theory (1976) in the range of middle critical frequencies. Finally, in this paper, the simple complex eikonal equations, in quasi-longitudinal (QL) approximation, for calculating the non-deviative absorption coefficient due to the propagation across the D-layer are encoded into a so called COMPLEIK (COMPLex EIKonal) subroutine of the IONORT (IONOspheric Ray-Tracing) program ( Azzarone et al., 2012). The IONORT program, which simulates the three-dimensional (3-D) ray-tracing for high frequencies (HF) waves in the ionosphere, runs on the assimilative ISP (IRI-SIRMUP-P) discrete model over the Mediterranean area ( Pezzopane et al., 2011). As main outcome of the paper, the simple COMPLEIK algorithm is compared to the more elaborate semi-empirical ICEPAC formula (Stewart, undated), which refers to various phenomenological parameters such as the critical frequency of E-layer. COMPLEIK is reliable just like the ICEPAC, with the advantage of being implemented more directly. Indeed, the complex eikonal model depends just on some parameters of the electron density profile, which are numerically calculable, such as the maximum height.     

The calculation of ionospheric absorption with modern computers

New outcomes are proposed for ionospheric absorption starting from the Appleton–Hartree formula, in its complete form. The range of applicability is discussed for the approximate formulae, which are usually employed in the calculation of non-deviative absorption coefficient. These results were achieved by performing a more refined approximation that is valid under quasi-longitudinal (QL) propagation conditions. The more refined QL approximation and the usually employed non-deviative absorption are compared with that derived from a complete formulation. Their expressions, nothing complicated, can usefully be implemented in a software program running on modern computers. Moreover, the importance of considering Booker’s rule is highlighted. A radio link of ground range D = 1000 km was also simulated using ray tracing for a sample daytime ionosphere. Finally, some estimations of the integrated absorption for the radio link considered are provided for different frequencies.     

竟拍过程的概率延拓分析

到拍卖行去竟拍拍品,已经成为我们生活中越来越平常的经济行为,在竟拍过程中,两人轮流举牌,甲先乙后,谁先拍到呢?结合概率论中的全概率公式,给出了甲先拍到的充要条件;在此基础上进行延拓,探讨随着竟价的提升,两人心理承受能力的等差下降和非等差下降对竟拍的影响,甲先拍到的概率变化,并推导出相应的概率计算公式.     

Space debris mitigation in geosynchronous orbit

In order to preserve the geosynchronous region, the Inter-Agency Space Debris Coordination Committee (IADC) proposed and endorsed a re-orbiting strategy for spacecraft at the end-of-life: they should be disposed above the synchronous altitude and passivated, to reduce the risk of inadvertent explosions. The recommended perigee altitude of the disposal orbit took into account all relevant perturbations and was a function of the expected perturbing acceleration induced by solar radiation pressure. It was intended to prevent any further interference with a properly defined geostationary protected region.     

改进的万有引力公式

根据广义相对论给出的行星运动方程，导出如下改进的万有引力公式F＝－GMm/r^2-3G^2M^2mp/c^2r^4应用该公式可给出光线近日偏折问题的准确解。