过冷状态下二维枝晶生长的相场方法模拟

通过相场理论建立了纯物质镍在过冷溶液中枝晶生长的相场模型。把相场方程和温度场方程进行耦合,建立了相对应的相场模型。该模型以熵增加函数为基础,通过熵增加函数推导出热力学一致性的相场控制方程。利用上述的模型和方法在计算机上编制二维组织凝固模拟程序得出结论,各向异性强度影响枝晶尖端生长速度,过冷度决定凝固速度的快慢。     

一种用于光传飞控系统的光纤温度传感器研究

利用半导体光吸收原理，设计出一种光纤温度传感器，它可实现强电磁干扰下高空无人机内的环境温度测量，具有体积小，结构简单的特点。该测试仪用GaAs晶片作为温度敏感元件，采用透射式结构，利用双光束补偿原理消除了光路扰动产生的误差。实验结果表明该传感器在-20-85℃的范围内有良好的温度响应。     

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.     

超高强度钢300M含碳量,等温组织与力学行为的关系

研究了四种含碳量、三种等温温度与力学行为的关系，并与淬火回火３００Ｍ钢进行比较得出，３００Ｍ钢在Ｍｓ点以下温度等温获得Ｍ＋Ｂ＿下＋Ａ＿Ｒ混合组织、超高强度和优良的韧性。断裂韧性对含碳量不敏感，冲击韧性随含碳量升高而降低。较高温度等温时，钢的冲击韧性和断裂韧性显著提高且对含碳量不敏感。     

Energy conversion of the flare due to direct electric fields from the sheared reconnection

In this paper we present a new mechanism of the main energy conversion of the solar flare. Since a flare inducing prominence (flux tube) rises V_z ? 300 km s⁻¹, the plasmas below it cannot continuously eject with Alfvén speeds of V_A = 3000 km s⁻¹ but probably with V_z ≈ ±100 km s⁻¹. Plasma up and downflows with V_A will within a short duration be blocked between the chromosphere where reconnected flux tubes are piling up, and the slowly rising flux rope. Hence the Petschek slow shock mechanism is difficult to be realized as a major energy converting mechanism.     

计算机模拟高温下温度波动对简化环氧分子结构参数的影响

对４００Ｋ下简化环氧分子结构的键长、键角、四原子扭转角及非键合原子间距离等结构参数在微小温度波动时进行动态模拟，分析了这些结构参数在该条件下的变形刚性。     

链子崖危岩体防治工程的DDA模拟

阐述了二维非连续变形分析方法（DDA）与锚杆数值模型的基本原理，开发了考虑锚杆单元的DDA程序。针对链子崖危岩体及其防治工程的特点。建立了相应的DDA数值模型，计算得出了不稳定块体的位移趋势图。计算结果与实际监测结果较为吻合．证明了此方法的有效性及其在工程应用中的可行性．拓宽了DDA的工程应用领域。     

电磁场作用下包晶合金定向凝固过程传输模型的建立

建立了二元包晶合金在电磁场作用下定向凝固过程中多场耦合的数学模型,并根据包晶转变不同阶段的特点,提出了包晶转变中固相分数的计算办法。该模型可以计算电磁场作用下包晶合金定向凝固中的流动、传热、传质的过程,为电磁场作用下包晶合金定向凝固过程的数值计算及对实验结果的分析提供理论依据。     

高超声速复杂气动问题数值方法研究进展

高超声速流场具有复杂流动特征,其中真实气体效应、磁流体干扰效应和力热结构耦合效应等对气动力分析产生了重要影响。将流体力学研究扩展到分子动力学、电磁流体力学以及流固耦合等交叉学科领域,这给数值模拟方法带来了巨大挑战。针对高超声速气动力/热分析的热点问题,重点关注高温效应与低密度流动效应、磁流体干扰效应和力热结构耦合效应等,结合算例分析了相应的数值求解技术;在气动热方面主要比较了3类求解方法(纯工程方法、纯数值方法和基于Prandtl边界层理论的方法),并给出了相应算例;对于气动力/热/结构耦合问题,从耦合模型及耦合计算方法两方面开展了分析。最后指出了高超声速复杂气动问题数值求解技术未来需重点关注的几个方面。     

高超声速飞行器表面温度分布与气动热耦合数值研究

针对高超声速飞行器热防护设计中的高温气体非平衡效应问题和气动热环境精确预测问题,基于流场的非平衡Navier-Stokes方程、表面的能量守恒方程和内部的热传导方程,考虑流场的非平衡效应、表面的热辐射效应、催化效应和烧蚀效应以及热防护层内部的热传导效应,建立了初步的表面温度分布与气动热的耦合计算方法,完善了高超声速飞行器气动物理流场计算软件(AEROPH_Flow)。在表面材料为碳-碳(C-C)条件下,对飞行高度为65km和飞行速度为8,10km/s的半球以及飞行高度为50km和飞行速度为8km/s的球锥模型,开展了表面温度分布与气动热的耦合计算,验证了计算方法和计算软件,分析了表面温度分布对气动热环境的影响。研究结果表明:表面温度分布对气动热的计算结果有较大影响,在气动热环境的预测中,不仅要考虑热化学非平衡效应和表面催化效应的影响,还要考虑表面温度分布的影响,最好是采用表面温度分布与气动热耦合计算的方法,以减小表面温度分布对气动热计算结果的影响。为此,需要发展完善非平衡流场/表面催化和烧蚀/热传导温度场(气/表/固)的计算模型、耦合求解技术和计算软件,实现对高超声速飞行器的真实飞行条件下高温气体非平衡效应和气动热环境的精确模拟。