真空绝热板阻隔膜PA/ VMPET/ Al/ PE 热封工艺

真空绝热板阻隔膜PA/ VMPET/ Al/ PE 是一种多层复合阻隔膜,是真空绝热板的重要候选膜材。 通过实验研究了热封温度、时间、压力对其强度的影响,同时采用Matlab 软件对热封工艺参数进行优化,得出 最佳的热封工艺。利用DSC 对PA/ VMPET/ Al/ PE 进行热分析。实验结果表明:热封温度是影响热封强度的 最显著因素,当热封温度为160 ~170℃,热封时间为1. 0 ~2. 0 s,热封压力为0. 2 ~0. 4 MPa 时,热封边的热封 强度良好。Matlab 软件优化最佳热封工艺参数值为:热封温度167℃,热封时间1. 80 s,热封压力0. 34 MPa,该 模拟优化热封工艺参数与实验值一致。     

基于面板数据模型的中西部地区加工贸易升级研究

我国经济高速发展,劳动力、土地等要素随之发生转变,加工贸易从东部地区向中西部地区转移,中西部地区加工贸易急需升级以适应发展。利用2001-2011年中西部地区部分省份的面板数据建立计量模型,通过检验对混合估计模型、固定效应模型和随机效应模型进行选择,并对选定模型的估计结果进行具体分析,提出中西部地区加工贸易升级的对策及建议。     

舰面效应对直升机操纵的影响

舰面效应对直升机的配平操纵和姿态角有很大的影响。基于三维面元法建立了直升机舰面效应模型,可有效用于分析部分地效和倾斜甲板。最后以某型机舰配合为例,分析了舰面效应对直升机配平操纵和姿态角的影响。     

The Modulation of Galactic Cosmic Rays in the Heliosphere: Theory and Models

Almost all theoretical and numerical models for the modulation of cosmic ray in the heliosphere are based on Parker's transport equation which contains all the important basic physical processes. The relative importance of the various mechanisms is however not established and may vary significantly over 22 years. The simultaneous measurements of solar wind parameters, heliospheric magnetic field properties and cosmic rays over a wide range of energies and positions in the heliosphere have brought the realization that modulation is much more complicated than what the original drift models predicted. In the process the sophistication of models based on solving Parker's equation has increased by orders of magnitude. A short review of the global modulation of cosmic rays is given from a theoretical and modelling point of view.     

大型太阳帆板展开状态动态特性研究

利用有限元技术及自编的 FORTRAN程序计算了单翼太阳帆板约束模态的振型和频率 ,计算结果和实验结果比较表明 ,计算精度在工程上是可以接受的。在此基础上 ,以飞船带有双翼对称太阳帆板为模型 ,计算了太阳帆板在转动和不转动情况下非约束模态的振型和频率。上述计算结果为研究带有挠性太阳帆板的航天器的动力学与控制问题打下了基础     

上市公司信息披露质量的影响因素——深圳股市面板数据的实证研究

以深圳股票市场2001-2004年的1958家上市公司的面板数据为研究样本，运用实证分析的方法，检验上市公司信息披露质量的影响因素。实证结果显示：信息披露质量与第一大股东持股比例、资产规模、净资产收益率以及审计意见正相关，而与资产负债率负相关；设立审计委员会的公司的信息披露质量较高。     

AN IMPROVEMENT FOR LOWER－ORDER PANEL METHOD BASED ON THE DIRICHLET BOUNDARY CONDITION

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X-Ray Emission from Flare Collapsing Trap

An acceleration process in the collapsing magnetic trap, formed in the flare with cusp magnetic field topology, is described. Computations show that high-energy electrons are accumulated in the central part of the collapsing magnetic trap due to an increase of their pitch angles. The effect explains in a natural way the formation of X-ray loop-top sources. Then, using the model with the collapsing trap and considering only the adiabatic heating process, a possible explanation for the motion of the X-ray loop-top source observed at the beginning of some cusp-type flares is presented.     

Oxygen Isotopes in the Solar System

The oxygen three-isotope system has major advantages over the two-isotope systems of hydrogen, carbon, and nitrogen because different fractionation laws govern intraplanetary and interplanetary processes. This permits discriminating between solar nebular processes and parent-body processes. Oxygen isotopes also serve as a sensitive natural tracer for meteorite classification. This revised version was published online in August 2006 with corrections to the Cover Date.     

Thermal cyclotron radiation from a hot coronal loop with helical magnetic field

The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field.