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211.
Asteroid and comet hazard: Identification problem of observed space objects with the parental bodies
M.G. Sokolova Y.A. Nefedyev N.Y. Varaksina 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
This article focuses on the genetic identification of observed small cosmic bodies with alleged parental bodies; namely, comets, asteroids and meteoroid swarms. There is a problem of the upper D-value limit as a measure of proximity between the orbits of the bodies in the five-dimensional phase space (Southworth and Hawkins, 1963). In the study of genetic relationships of the comet and meteor complexes, the D value is usually taken as equal to 0.2 for all meteor showers. However, the upper D limit should be investigated for each meteoroid complex. For example, such investigation was performed for the Taurid meteor complex (Porub?an et al., 2006). In this paper, the upper D-criterion limit value was investigated for the Perseid meteor shower. The 1862 III Swift–Tuttle comet is its parental comet. 相似文献
212.
盘腔积液现象在舰用燃气轮机工作过程中时有发生,汽化的滑油和水蒸气凝结形成积液。转子带动腔内的积液旋转,引发振动失稳,严重时会对发动机结构造成致命性破坏。为此,本文开展燃气轮机压气机盘腔积液的模拟实验研究,以双盘双支承的卧式柔性转子系统作为研究对象,重点关注小积液量的特点,对积液转子的动力学稳定性进行了研究。观测到转子的失稳现象,开展了不同积液体积、不同积液类型(水、植物油和滑油)等因素的影响规律研究,揭示了小积液的卧式转子动力学特征。研究结果表明:①对于积液失稳振动,存在失稳边界积液量,当积液量大于该边界值时,失稳将会发生。②失稳边界转速及恢复转速均高于临界转速。当转速高于失稳边界转速时,失稳将会发生。转速进一步增加,高于恢复转速时,失稳现象可能消失。③失稳时的振动特征为:出现幅值突增,次谐波成分也随之增加;基频和次谐波发生调制,表现出拍振特征。④随着积液体积的增加,失稳边界转速先减小后增加。⑤随着积液粘度系数增大,失稳边界转速和边界积液量均增大。 相似文献
213.
为研究扑翼飞行器传动机构的能量特性,以特拉华大学机械系统实验室所研制样机为原型进行了建模。引入气动项和拉力弹簧建立了完整的动力学模型。分析发现,气动项的力矩峰值为惯性项的4.8倍,对电机的转矩峰值的影响起主要作用。运用正交法进行仿真发现,引入拉力弹簧可以使电机转矩峰值最大降低77.5%,与理论分析相符合。进一步的物理实验验证了理论分析和仿真结果的正确性,并得到了当弹簧的连接点位置为185 mm、原长为200 mm及刚度为0.1 N/mm时实验结果取得最优值,可为扑翼机传动机构的优化设计提供依据。此外,引入弹性元件也可有效降低电机的转速波动,进而为仿生扑翼飞行器的生产和实践应用提供理论指导。 相似文献
214.
A parameterized geometry design method for inward turning inlet compatible waverider 总被引:1,自引:1,他引:1
Intensive studies have been carried out on generations of waverider geometry and hypersonic inlet geometry. However, integration efforts of waverider and related air-intake system are restricted majorly around the X43A-like or conical flow field induced configuration, which adopts mainly the two-dimensional air-breathing technology and limits the judicious visions of developing new aerodynamic profiles for hypersonic designers. A novel design approach for integrating the inward turning inlet with the traditional parameterized waverider is proposed. The proposed method is an alternative means to produce a compatible configuration by linking the off-the-shelf results on both traditional waverider techniques and inward turning inlet techniques. A series of geometry generations and optimization solutions is proposed to enhance the lift-to-drag ratio. A quantitative but efficient aerodynamic performance evaluation approach (the hypersonic flow panel method) with lower computational cost is employed to play the role of objective function for opti- mization purpose. The produced geometry compatibility with a computational fluid dynamics (CFD) solver is also verified for detailed flow field investigation. Optimization results and other numerical validations are obtained for the feasibility demonstration of the proposed method. 相似文献
215.
An analysis of the orbital evolution of the ESA's Hipparcos satellite is presented. Hipparcos operated between August 1989
and March 1993 in a highly elliptical orbit: a geostationary transfer orbit with increased perigee height. The requirements
of the scientific mission included high accuracy knowledge of the position and velocity vectors of the spacecraft as a function
of time. Through a study of the variations in the total orbital energy, the loss of energy during the mission as a result
of non-conservative forces is recovered. These are explained as largely due to atmospheric drag during perigee passages. Apparent
variations in the drag coefficient are in agreement with orientation variations of the satellite during those perigee passages.
Two different models used for calculating the atmospheric drag give significantly different results, confirming earlier findings
by other users of those models.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
216.
何利军%赵云峰%詹茂盛%游少雄 《宇航材料工艺》2007,37(3):9-12
从组成、制备工艺、阻尼机理讨论了有机小分子杂化阻尼材料的研究现状,并给出了一些该类阻尼材料的实例及其阻尼性能数据,提出了有机小分子杂化阻尼材料目前存在的问题,指出该类阻尼材料阻尼性能突出、Tg可设计,是一种颇有前景的材料。 相似文献
217.
通过求解薄层近似的Navier-Stokes方程,数值模拟了带座舱飞船高超声速粘性绕流,首次系统地给出了攻角为5°、10°、20°、30°和40°情况下的物面分离形态、横戴面流线形态、纵剖面流线形态以及旋涡沿涡轴的演变形态。分析和比较表明,本文采用数值可视化方法给出的流场拓扑结构与相应的拓扑规律完全吻合。在飞船后体流场横截面流线中,本文发现了稳定的极限环流态,该极限环涡心处沿涡轴方向的速度是超声速 相似文献
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