一般高速数据总线网络的吞吐量分析

分析了一般高速数据总线网络优先权方案的特性，建立了一般ＨＳＤＢ网络多优先权的平均吞吐量模型，导出了不同优先权的平均吞吐量解析表达式，并通过软件仿真验证了由得到的解析表达式。     

非线性动力响应分析的双θ法

本文在二次加速度插值模式的基础上,提出了动力响应分析的双θ法及加权平均法。这两个方法,加速度的截断误差(精度)是O(△t~(3)),是无条件稳定的,有较好的人工阻尼性质,没有超越现象。比现有的逐步积分法有明显的优点。     

考虑真实气体效应的一维非定常平衡流的随机选取法计算

本文提出一种近似随机选取法,计算一维非定常的高温平衡流动。采用稀疏激波替代等熵稀疏波,选用拟合经验方程计算高温热力学性质,并利用切割迭代方法加快收敛,从而计算大为简化,并有很好精度。     

热力学中最小熵增原理在流体力学中的应用

本文运用非平衡态热力学中最小熵增原理,分析了层流和湍流流动在接近热力学平衡定态时的特性。特别是在湍流流动中,舍弃了以往一些经验性的假设,指出流动处于局部机械平衡时可由最小熵增原理导出速度和温度分布。反之亦揭示了充分发展的湍流遵循最小熵增原理的这一机理。     

临近空间大气中波红外辐射特性的数值分析研究

介绍了临近空间大气环境特点及其非局域热平衡状态的辐射传输计算方法。利用战略高高度辐亮度代码SHARC（Strategic high-altitude radiance code），计算了3—5 μm波段不同观测条件、光学现象及大气环境下的临近空间大气背景辐射。分析结果表明：临近空间中波红外辐射随观测天顶角的增大而增强，随太阳天顶角的增大而减弱；在38 km及75 km附近，临边背景辐射存在极大值；纬度越高，临边背景辐射的季节变化特征越明显。OH夜气辉和极光对背景辐射有重要增强作用。     

场协同原理在高超声速化学非平衡流动中的推广

应用理论分析与数值模拟方法，将对流传热的场协同原理从不可压缩流动推广至高超声速化学非平衡流动中。结果表明，高超声速化学非平衡层流与湍流的热流密度取决于流动的当地单位体积的动量与单位质量总焓梯度的协同。用当地单位体积的动量与单位质量总焓梯度的协同研究高超声速化学非平衡流动的壁面传热问题，对层流流动下的对流传热，不但计及了高超声速化学非平衡流的密度变化对热流密度的影响，而且包括了静焓梯度、压力梯度、边界层内的分子黏性剪切效应对热流密度的作用；对湍流问题，除了上述层流流动各项对热流密度的影响外，还计及了雷诺剪切应力对热流密度的作用。考虑到高超声速化学非平衡流静焓的定义，高超声速化学非平衡层流及湍流的场协同同时计及所有组分的平动能、转动能、振动能及电子能等梯度的贡献。     

Statistical study of the time delay of ionospheric TEC storms to geomagnetic storms in Taoyuan,Taiwan

We have studied the time delay of ionospheric storms to geomagnetic storms at a low latitude station Taoyuan (25.02°N, 121.21°E), Taiwan using the Dst and TEC data during 126 geomagnetic storms from the year 2002 to 2014. In addition to the known local time dependence of the time delay, the statistics show that the time delay has significant seasonal characteristics, which can be explained within the framework of the seasonal characteristics of the ionospheric TEC. The data also show that there is no correlation between the time delay and the intensity of magnetic storms. As for the solar activity dependence of the time delay, the results show that there is no relationship between the time delay of positive storms and the solar activity, whereas the time delay of negative storms has weakly negative dependence on the solar activity, with correlation coefficient −0.41. Especially, there are two kinds of extreme events: pre-storm response events and long-time delay events. All of the pre-storm response events occurred during 15–20 LT, manifesting the Equator Ionospheric Anomaly (EIA) feature at Taoyuan. Moreover, the common features of the pre-storm response events suggest the storm sudden commencement (SSC) and weak geomagnetic disturbance before the main phase onset (MPO) of magnetic storms are two main possible causes of the pre-storm response events. By analyzing the geomagnetic indices during the events with long-time delay, we infer that this kind of events may not be caused by magnetic storms, and they might belong to ionospheric Q-disturbances.     

A theoretical method for solving shock relations coupled with chemical equilibrium and its applications

In this study, a theoretical method is proposed to solve shock relations coupled with chemical equilibrium. Not only shock waves in dissociated flows but also detonation waves in combustive mixtures can be solved. The global iterative solving process is specially designed to mimic the physical and chemical process in reactive shock waves to ensure good stability and fast convergence in the proposed method. Within each global step, the single-variable equations of normal and oblique shock relatio...     

煤油液滴高压蒸发特性

采用真实流体模型描述高压下流体热物理性质的非理想性,并采用状态方程（EoS）法计算多组分高压气-液相平衡及环境气体溶解性,在此基础上建立包含亚临界和超临界两种不同机制的瞬态液滴高压蒸发模型。针对中国新一代高压补燃液氧/煤油发动机,详细研究了煤油液滴在超临界环境下的高压蒸发特性及各因素影响机理。结果表明：高压环境会显著加快液滴温升速率,但弱超临界环境下仍然为相平衡控制的亚临界蒸发状态;只有强超临界环境下才较容易发生扩散控制的超临界蒸发状态。在高压、高温环境下,忽略气相溶解性将导致液滴蒸发速率明显偏小。针对弱超临界环境,温度升高会使液滴蒸发速率单调增加;压力升高则在低温下降低蒸发速率,而在高温下加快蒸发速率。针对强超临界环境,温度升高只提升初始亚临界蒸发阶段的蒸发速率,而超临界蒸发阶段的蒸发速率与环境温度无关;压力升高则同样会提升初始亚临界蒸发阶段的蒸发速率,但会降低超临界蒸发阶段的蒸发速率,此时的总蒸发寿命随压力升高小幅下降。