电磁波与TVP相互作用

基于时变等离子体(TVP)的场方程,根据麦克斯韦方程,推导了TVP对入射电磁波的频率上移、时间衰减常数、反射系数,以及TVP的透射波和反射波电场幅值计算公式。通过实例计算分析了不同时间的新波频率、时间衰减常数和电场幅值。方法简单易行,可为TVP的应用提供一定的理论依据。     

Gravity waves generated by thunderstorms: South-East Asia tropical region study

Gravity waves are recognized as an integral part of earth’s atmosphere which are mainly responsible for energy and momentum distribution among different layers and regions in the atmosphere. Various sources present in land, ocean, and atmosphere such as mountains, convection, jets and fronts etc. are responsible for gravity waves generation. Thunderstorms (deep convection) are one of the major sources of gravity waves in the tropical region, capable of generating waves with a wide range of frequencies and scales and significantly affecting the existing waves. Previous numerical studies have characterised the wave properties that are generated from thunderstorms, but there are no statistically quantified studies. In this paper, we have modelled the relationship between the latent heat generated inside a thunderstorm and the gravity wave properties at the geo-collocated points. Gravity waves are identified over Singapore radiosonde station (with data available until 30?km altitude with 12?h temporal resolution) in the stratosphere using wavelet studies. Based on the GROGRAT ray tracing methods to identify the thunderstorm locations, and RAMS cloud-resolving models simulations to obtain the latent heating of the thunderstorm, a regression analysis is performed using 200 cases of gravity waves. Furthermore, cloud-top momentum flux analysis is performed for various cases latent heat. This study is expected to provide more quantified and concrete information on the coupling between the thunderstorm and gravity wave which includes the variance in these relationships due to wave frequency spectrum and generation mechanisms.     

空气动力二阶核函数辨识方法

采用截断三阶Volterra级数模型来研究空气动力二阶核函数的辨识问题,选取一簇正交化的切比雪夫多项式对二阶核函数进行参数化处理,并将非参数辨识问题转化成参数辨识问题。相比于其他方法,本文模型能有效降低对激励信号幅值的敏感程度,保证辨识出的核函数具有较好的保真度;只针对三阶Volterra降阶模型中的一阶、二阶核函数进行辨识,即可提升原系统一阶、二阶核函数的辨识精度,却不会显著增加辨识过程的工作量;参数化辨识方法属于整体性辨识,根据已有的部分数据对(输入、输出数据)就能完成系统辨识,且能达到较好的辨识精度,从而有效地减少了执行计算流体力学(CFD)代码程序的总次数,节约了大量的时间成本。算例表明,与目前流行的非参数化方法相比,本文提出的切比雪夫函数辨识方法,精度上达到预期要求,辨识过程消耗的CFD总时间量至少可降低一个数量级。     

用激光散斑测微小位移及应用

本文介绍了散斑测微小位移原理及在普通物理实验中的应用。     

振动系统特征值和特征向量的—阶导数

本文主要解决两个问题:(1)频率集聚时,如何计算特征值(固有频率的平方)和特征向量(振型)的一阶导数,(2)如果仅获得了少数的低阶模态,如何改进已有的模态展开法,使其能用于计算低阶特征向量的一阶导数。     

Magnetospheric and ionospheric manifestations of interplanetary foreshocks

The geometry of a typical interplanetary shock front in the vicinity of the Earth’s orbit predicts that the leading edge of the foreshock region comes into contact with the magnetosphere a few hours ahead of geomagnetic sudden impulses (SI). There is reason to believe that the interaction of the magnetosphere with the foreshock leads to magnetic and ionospheric disturbances, which can be detected by ground-based instruments. We searched for specific precursors of SIs in data from the Scandinavian riometer network and in the short period geomagnetic pulsation data from mid-latitude magnetometers. We found that SIs were preceded by the following three features: (1) an increase in riometric absorption, (2) excitation of Pcl magnetic pulsations and (3) a spectral broadening of the Pc3 magnetic pulsations. Our observations may be useful for the study of acceleration processes in the solar wind. These observations are also of potential forecasting interest.     

Dissipative Solitary Kinetic Alfvén Waves and Electron Acceleration in the Solar Corona

Nonthermal electrons play a major role during solar flares since not only they contain a large amount of the released energy but also they provide important information of the flaring physics through their nonthermal radiation in radio and hard X-ray bands. In a recent work Wu (Phys. Plasmas 10 (2003) 1364) proposed that dissipative solitary kinetic Alfvén wave (DSKAW) with a local shock-like structure could provide an efficient acceleration mechanism for energetic electrons in a low-β plasma. In the present paper dynamical characteristics of the DSKAW acceleration mechanism in solar coronal plasmas are studied and its application to the acceleration of flaring electrons is discussed.     

圆锥激波的反解法

给出了超音速圆锥激波的一种反解法，该方法由假定的激波处向锥面推算，具有计算效率高，适于计算机处理等特点。     

复合材料模具技术

复合材料模具以其热膨胀系数小、质量轻、热容小等优点在国外航空航天领域应用广泛并且形成产业.分析了该技术的优缺点,研究了复合材料模具制造工艺的关键问题,总结了复合材料模具技术的发展动向.     

玻璃纤维增强酚醛基复合材料平均线胀系数测试影响因素

研究了保温时间、升温速率、预处理温度等对玻璃纤维增强酚醛基复合材料线胀系数测试的影响。结果表明,玻璃纤维增强酚醛基复合材料在加热条件下进一步固化,造成样品收缩与样品受热膨胀相抵消,升温曲线出现平台。因此,测试前应对样品进行预处理,处理温度高于试样最终的测试温度,低于样品固化温度,以免材料内部结构发生变化;设置合适的升温速率,升温速率低,增加了时间成本,升温速率太高,测温热电偶引入的误差增加,且不均匀的加热使试样产生热应力,影响试验结果。