大质量飞行器质心测量方法

详细介绍了大质量飞行器质心测量的多支点称重法,针对某大质量飞行器,提出了径向测量的改进方法,算例表明,改进方法极大地提高了系统的测量准确度,可以满足大质量飞行器高准确度质心的测量要求。     

太阳电池阵的铰链副刚度参数识别

为正确识别太阳电池阵铰链副的刚度参数,用形状简单、建模相对容易的有机玻璃板列阵不同状态下模态试验结果估计待识别参数的初始值,通过线性化目标函数,将参数识别归为易求解的数学规划问题,最终直接用商用有限元分析程序和数学软件实现参数识别。识别结果表明,理论计算值与试验结果基本吻合。     

PE绳的特性及物理性能测试

文章简要介绍了新型超高分子量聚乙烯 (简称UHMW -PE)纤维的性能及其在中国航天器回收系统中的应用现状 ,并重点介绍了针对这种新型材料产品PE绳的测试方法。     

轴对称降落伞稳定下降阶段的流场特性

文章根据降落伞的特点，通过3点假设（伞衣的薄膜假设、降落伞的轴对称假设和流场的定常假设），将三维复杂流动问题，转化成二维轴对称问题，以节约计算时间。然后，建立轴对称降落伞的流体力学计算模型，利用数值模拟手段，求解RNG（Renormalization Group）k-epsilon湍流模型下的N-S方程组，获得与有关单位试验相吻合的计算结果。分析发现带顶孔的轴对称降落伞绕流和亚临界状态下带中心孔的圆球绕流，在尾流区拓扑结构上几乎完全一致。结果表明建立的轴对称降落伞模型，能够揭示降落伞流场的本质特性，为进一步研究降落伞流场的流动机理和流固耦合问题打下基础。     

Three-dimensional global simulation of multiple ICMEs’ interaction and propagation from the Sun to the heliosphere following the 25–28 October 2003 solar events

This study performs simulations of interplanetary coronal mass ejection (ICME) propagation in a realistic three-dimensional (3D) solar wind structure from the Sun to the Earth by using the newly developed hybrid code, HAFv.2+3DMHD. This model combines two simulation codes, Hakamada–Akasofu–Fry code version 2 (HAFv.2) and a fully 3D, time-dependent MHD simulation code. The solar wind structure is simulated out to 0.08 AU (18 Rs) from source surface maps using the HAFv.2 code. The outputs at 0.08 AU are then used to provide inputs for the lower boundary, at that location, of the 3D MHD code to calculate solar wind and its evolution to 1 AU and beyond. A dynamic disturbance, mimicking a particular flare’s energy output, is delivered to this non-uniform structure to model the evolution and interplanetary propagation of ICMEs (including their shocks). We then show the interaction between two ICMEs and the dynamic process during the overtaking of one shock by the other. The results show that both CMEs and heliosphere current sheet/plasma sheet were deformed by interacting with each other.     

直射式气动雾化喷嘴对燃烧室性能的影响

为了深入分析燃油喷嘴对燃气轮机燃烧室性能的影响，针对燃气轮机燃烧室中的直射式气动雾化喷嘴开展了数值模 拟，获得了气流流量、燃油流量和气液比对雾化性能的影响规律，喷嘴的雾化性能参数包括雾化粒径和雾化锥角。结果表明：气液 比和气流流量对该型喷嘴的雾化性能有显著影响，燃油流量对雾化性能的影响较小；气液两相间相对速度是影响该型喷嘴雾化性 能的决定因素，相对速度增大有利于减小雾化粒径，并增大雾化锥角；气流流量和气液比的增大均有利于雾化粒径的减小，燃油流 量的增加将使雾化粒径增大；增大气流流量、气液比和减小燃油流量均可使雾化锥角增大；该型喷嘴的雾化锥角变化范围为 30.12°～41.24°，雾化粒径变化范围为131.46～ 186.52 μm。喷嘴可实现在较小的雾化锥角变化范围内获得较宽的雾化粒径变化， 以此匹配燃气轮机燃烧室不同工作状态，具有较高的实用价值。     

Solar Neutrinos

The current status of solar neutrino experiments is reviewed. All the experimental measurements show deficits of solar neutrinos. Non monotonic suppression indicates that the problem may naturally be explained by neutrino oscillations, but not by modifying solar models. A new experiment shows very promising results. We hope that a definite answer to the question of whether solar neutrinos are oscillating will be obtained in the very near future. This revised version was published online in June 2006 with corrections to the Cover Date.     

Results from the study of an M7.6 flare and its associated CME

An M7.6 flare was well observed on October 24, 2003 in active region 10486 by a few instruments and satellites, including GOES, TRACE, SOHO, RHESSI and NoRH. Multi-wavelength study shows that this flare underwent two episodes. During the first episode, only a looptop source of <40 keV was observed in reconstructed RHESSI images, which showed shrinkage with a velocity of 12–14 km s⁻¹ in a period of about 12 min. During the second process, in addition to the looptop source, two footpoint sources were observed in energy channel of as high as ∼200 keV. One of them showed fast propagation along one of the two TRACE 1600 Å flare ribbons and the 195 Å loop footpoints, which could be explained by successive magnetic reconnection. The associated CME showed a mass pickup process with decreasing center-of-mass velocity. The decrease of the CME kinetic energy and the increase of its potential energy lead to an almost constant total energy during the CME propagation. Our results reveal that the flare and its associated CME have comparable energy content, and the flare is of non-thermal property.     

生物皮肤传质的研究

针对皮肤各层结构主要由细胞和细胞间液构成的特点提出了可行的3层多孔介质物理模型,根据不同层的具体特点建立了相应的浓度和能量数学方程.利用浓度方程对模型进行了浓度分析求解,和编程计算了在不同灌流率、传质系数和各层厚度下对浓度的影响.与传质系数实验所得结果相比较,结果一致.