矩形蜗壳内三维紊流场的热线测量

在3个不同流量工况, 对矩形蜗壳内三维紊流流场进行了测量。结果表明, 在矩形蜗壳进口突变截面两侧壁的角区存在有回流区。在回流区中紊动能和雷诺应力明显大于中间截面主流区中的值。随着试验流量的增加, 回流区减小, 紊动能和雷诺应力很快下降。在同一流量工况, 随着半径增加, 紊动能和雷诺应力减小。在蜗壳圆周方面的不同横截面上存在有大旋涡, 气体在蜗壳中按螺旋管线运动。      

高速滚动轴承弹性流体动力润滑分析

直接采用弹性流体动力润滑（ＥＨＬ）分析方法计算了高速滚动轴承中滚子与内、外套圈接触区的油膜厚度、油膜动压力和润滑油牵引力;分析了载荷、转速及滚子数等参数对轴承打滑损伤的影响。理论分析结果与所作实验结果在较宽的工况范围内吻合较好。     

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.     

航空发动机轴承腔热状态分析模型及温度场计算

分析了轴承腔的主要热源。建立了轴承及石墨密封摩擦热的计算模型、密封热泄漏量的计算模型、对流换热系数的计算模型及温度场的计算模型。用热网络法建立了轴承腔的热平衡方程组,并采用拟牛顿法求解了该方程组。获得了10种不同工况下的温度场计算结果,该结果与本文的测试结果基本吻合。      

某直升机齿轮传动系统的瞬态热分析

提出了传动系统瞬态温度场的分析方法,建立了失去润滑条件下传动系统功率损失及对流换热系数的计算模型,该模型考虑了失去润滑后传动系统热状态参数的时变特征。在稳态热分析的基础上,求解了某直升机齿轮传动系统的瞬态温度场,为该传动系统生存能力的预测提供了理论依据。      

电弧喷射器流场模拟中电场计算的多重网格法

在建立电弧喷射器内等离子体流场电场计算模型以及基本算法基础上,研究了采用多重网格对收敛速度的改进效果。数值计算证实了此方法的有效性尤其对流场电场耦合计算是有利的。     

来流条件对叶片表面附面层转捩影响的数值模拟研究

通过对二维压气机叶栅叶片表面附面层流态的数值模拟分析,研究了在不同来流马赫数和冲角下,叶片表面层流附面层向紊流附面层的转捩过程,转捩区域的大小等。归纳分析了部分来流条件对转捩过程的影响机制。结果表明:来流马赫数和冲角对转捩起始点和结束点的位置,即转捩所占区域的大小有重要影响。研究工作取得的进展不仅为进一步从机理上深刻认识来流条件对叶片表面附面层流态的影响机理提供了一定的科学依据,而且对今后指导叶片表面附面层流态模似实验工作的开展具有重要参考价值。      

Physical processes in the strong magnetic fields of accreting neutron stars

The key radiative processes are discussed, numerical methods of magnetized radiative transfer are presented, and these are considered in their application to X-ray pulsar models.     

Neutron stars: Classification and evolution

The general aproach is considered which describs the evolution of neutron stars in terms of their interaction with surrounding matter. All possible states of neutron stars are classified from this point of view. Classification and evolution of binaries contaning neutron stars are also considered.     

粒子图象电影测速技术

本文介绍一种粒子图象电影测速技术,该技术采用机械调制装置及光学透镜,将连续输出的氩离子激光调制成周期性脉冲片光源序列,并与快速照相枪匹配,可以连续拍摄流场一个截面上随时间发展过程中不同瞬态的一系列两次或多次曝光的粒子图象底片,因而不仅可以取得流动一个截面上的瞬时二维速度场,并且可以获得该流动截面速度场发展的时间历程,为定量研究非定常流动随时间的发展特性提供了一种有效途径。