3D nonlinear wave heating of coronal loops

The heating of solar coronal loops by the resonant absorption or phase-mixing of incident wave energy is investigated in the framework of 3D nonlinear magnetohydrodynamics (MHD) by means of numerical simulations.     

Transition region line-shifts in the rebound shock spicule model

Spectral emission lines created in the solar chromosphere — corona transition region show net red-shifts. It has been proposed that this may be the result of the return of spicular material. We simulate a spicule numerically using the rebound shock model and find that the resulting hydrodynamic evolution leads to a perceived up-flow in transition region spectral lines even though the average velocity in the line forming region is directed downward. The explanation for this apparent paradox is found in the correlation between density and velocity in the waves generated by the rebound shock spicule.     

气动谐振管加热振荡流动过程数值研究

为了了解气动谐振管加热现象的振荡流动过程，利用显式TVD－MacCormark格式数值求解二维轴对称雷诺平均N－S方程，获得了一个谐振循环中完整的喷嘴－谐振管系统的振荡流动湍流流场，结果表明，欠膨胀声速冲击喷流固有的流场不均匀性和不稳定性是谐振管加热现象产生的内在原因，激波耗散是谐振管主要的加热机理。     

Ni-Cu-Mn-Co高温钎料的工艺钎焊性分析

通过飞机导管高温钎焊时Ni-Cu-Mn-Co钎料传热特征的物理模拟,得到了钎焊间隙的控制要素。在运用经典电磁场理论进行热电磁耦合分析的基础上,制定了安装式感应钎焊工艺。     

Evolution of the Protosolar Nebula and Formation of the Giant Planets

The formation of planetary systems is intimately tied to the question of the evolution of the gas and solid material in the early nebula. Current models of evolution of circumstellar disks are reviewed here with emphasis on the so-called “alpha models” in which angular momentum is transported outward by turbulent viscosity, parameterized by an dimensionless parameter α. A simple 1D model of protoplanetary disks that includes gas and embedded particles is used to introduce key questions on planetesimal formation. This model includes the aerodynamic properties of solid ice and rock grains to calculate their migration and growth. We show that the evolution of the nebula and migration and growth of its solids proceed on timescales that are generally not much longer than the timescale necessary to fully form the star-disk system from the molecular cloud. Contrary to a widely used approach, planet formation therefore can neither be studied in a static nebula nor in a nebula evolving from an arbitrary initial condition. We propose a simple approach to both account for sedimentation from the molecular cloud onto the disk, disk evolution and migration of solids. Giant planets have key roles in the history of the forming Solar System: they formed relatively early, when a significant amount of hydrogen and helium were still present in the nebula, and have a mass that is a sizable fraction of the disk mass at any given time. Their composition is also of interest because when compared to the solar composition, their enrichment in elements other than hydrogen and helium is a witness of sorting processes that occured in the protosolar nebula. We review likely scenarios capable of explaining both the presence of central dense cores in Jupiter, Saturn, Uranus and Neptune and their global composition. This revised version was published online in August 2006 with corrections to the Cover Date.     

多功能CAN节点电路的设计及其应用

介绍一种多功能CAN节点的电路结构及在工业中频感应加热设备控制现场总线中的应用。     

接触焊机理的探索

探讨了接触焊的机理，提出了以电位差选择电极材料的原则，以及焊接处的接触电阻和母材内阻在焊接中有一定作用，而且焊接处的总热能是各种能量产生的热量之和，焊接的总热量也应包括通电加热产生的热量和断电后（锻压时）产生的热量。     

航天飞机防热瓦缝隙气动加热的讨论

本文根据航天飞机防热瓦缝隙流动的特点,从二维定常不可压缩层流的 N-S方程出发,提出了一个简化流动模型,即缝隙的二维流动可近似当作两个准一维沟槽流动的线性迭加,由此给出了缝隙中的热流率与压力、压力梯度和缝隙宽度的变化规律,并利用现有的实验结果作了验证。     

Ⅰ型极值分布的环境因子

本文通过对Ⅰ型极值分布的理论分析和环境因子的二因子法，分别得到了Ⅰ型极大值分布和Ⅰ型极小值分布的环境因子，它们与正态分布的环境因子^[1]具有相同的形式，对Ⅰ型极值分布的环境因子进行了点估计，提出了用环境因子进行数据转换和综合的步骤。     

太阳微波爆发频谱事件

国家天文台1.0-2.0GHz,2.6-3.8GHz太阳射电频谱仪从1994年1月和1996年9月投入观测至2000年4月10日记录到太阳射电爆发分别为297个和316个，取得了高质量的高时间分辨率，高频率分辨率的动态谱资料，为研究耀斑各种尺度的时间及空间演化过程提供了丰富的信息，1998年4月15日的共同事件在时间和频率上显示了丰富的幅度和结构的变化。