一种确定模拟的行星际MHD激波局地参数的新方法

简要阐述了分析模拟的行星际磁流体力学（MHD）激波的局部性质时，采用无厚度局部平面激波这一假设的合理性，说明了在激波未扰动区域（激波上游），物理量在几个小时内的变化很小这一事实，利用平面激波的分析方法，提出了分析模拟的行星际MHD激波的新方法，包括激波位置的确定，上下游状态参数的选择，激波局部参数的计算以及激波的分类，最后应用这种方法对一个二维的MHD模拟结果进行了分析。结果证实了过去文献关于磁流体力学混合激波空间连接和时间演化的链式规则，而且说明位于太阳赤道附近的慢激波和中间激波最终会发展为快激波。     

三元流叶轮的电弧铣削与机械铣削组合加工

首先介绍了一种实现电弧与铣削组合的加工方法及装备。其次,为验证电弧加工在航空部件生产方面的能力及其对后续精加工工艺的友好性,利用自研的高速电弧放电与机械铣削组合加工专用机床,以具有复杂曲面特征的三元流叶轮样件为例进行五轴电弧铣削与机械铣削组合加工试验研究。结果表明,合理安排电弧加工工序,可以在实现材料高效去除的同时,取得较优的表面质量,电弧铣削中最大材料去除率达14500mm^3/min,小能量电弧加工完成后的样件表面粗糙度R_a为12.5μm,硬度为69.4HRB,较基体硬度未有明显变化,可以很好地适应切削加工要求。后续机械铣削加工过程中,刀具磨损小、加工状态稳定,最终获得粗糙度R_a1.2μm的加工表面,且由于切削余量小,有效抑制了加工变形,样件加工结果达到设计要求,充分展现了该组合加工工艺应用于具有复杂形貌特征的航空发动机零部件制造方面的可行性。     

Nanoflares and current sheet dissipation

Energy must be continually supplied to the solar corona to maintain both its average temperature and its high energy manifestations. The energy is supplied by photospheric motions and the magnetic field acts both to transmit this energy to the corona and as the furnace in which the energy is stored. The means by which the energy is dissipated and transformed into the actual forms we observe is the activation of current sheets. We conjecture here the properties of such current sheets as derived by both energetical arguments and numerical evidence of the self-organization of a system of currents in a highly turbulent medium. The consequences of the appearance of spatial and temporal intermittency on the different aspects of solar acitvity are also discussed.     

Low frequency turbulence and energy dissipation in the Solar Wind

The possibility to perform in-situ measurements of velocity, magnetic field, density and temperature fluctuations in the Solar Wind has greatly improved our knoweledge of MHD turbulence not only from the point of view of space physics but also from the more general point of view of plasma physics.These fluctuations on the one hand extend over a wide range of frequencies (about 5 decades), a fact which seems to be the signature of turbulent non-linear energy cascade, on the other hand display, mainly in the trailing edge of high speed streams, a number of striking features: (i) a high degree of correlation between magnetic and velocity field fluctuations, (ii) a very low level of fluctuations in mass density and magnetic field intensity, (iii) a considerable anisotropy revealed by minimum variance analysis of the magnetic field correlation tensor. More recently it has been stressed that MHD turbulence in the Solar Wind displays a clear intermittent character.The picture which emerges from the most recent analytical theories and numerical simulations is presented. In particular the observations which give us informations about the dissipation mechanism, which remains yet largely unknown, are discussed.     

有限元三维网格自动生成

讨论了为提高有限元法求解流动问题的精度和效率而寻求自动生成三维网格的方法。给出了利用代数变换、输入极少量区域边界数据即可插值生成三维网格的方法。最后举出了自动生成三维网格的例子。     

太阳色球层-日冕中扰动的传播(Ⅱ)

首先讨论了磁流波传播的线性特征，然后构造了球坐标中-自治的非等温，非均匀等离子体初态，应用二维时变可压缩磁流体动力学模拟，数值研究了色球层底部压力脉冲所引起扰动的全球传播过程，结果表明，在极区，压力脉冲导致的扰动传播可以区分成两类不同模式的波动，快磁声波与慢磁声波，而在赤道附近，传播扰动是快模磁声波，在源区附近还存在一非传播的扰动，模拟结果的特征有助于解释SOHO/EIT观测到的波动事件。     

Absolute and Convective Instabilities of Circularly Polarized Alfvén Waves

We discuss the recent progress in studying the absolute and convective instabilities of circularly polarized Alfvén waves (pump waves) propagating along an ambient magnetic field in the approximation of ideal magnetohydrodynamics (MHD). We present analytical results obtained for pump waves with small dimensionless amplitude a, and compare them with numerical results valid for arbitrary a. The type of instability, absolute or convective, depends on the velocity U of the reference frame where the pump wave is observed with respect to the rest plasma. One of the main results of our analysis is that the instability is absolute when U _l < U < U _r and convective otherwise. We study the dependences of U _l and U _r on a and the ratio of the sound speed to the Alfvén speed b. We also present the results of calculation of the increment of the absolute instability on U for different values of a and b. When the instability is convective (U < U _l or U > U _r) we consider the signalling problem, and show that spatially amplifying waves exist only when the signalling frequency is in two symmetric frequency bands. Then, we write down the analytical expressions determining the boundaries of these frequency bands and discuss how they agree with numerically calculated values. We also present the dependences of the maximum spatial amplification rate on U calculated both analytically and numerically. The implication of the obtained results on the interpretation of observational data from space missions is discussed. In particular, it is shown that circularly polarized Alfvén waves propagating in the solar wind are convectively unstable in a reference frame of any realistic spacecraft.     

MKDVB and CKB Shock Waves

This review presents results from MKDVB and CKB systems to illustrate the properties of magnetohydrodynamics intermediate shock waves. The intermediate shocks can have a family of shock structures; the shock structure and the evolution are related. Furthermore, there exists a class of time-dependent intermediate shocks. This revised version was published online in August 2006 with corrections to the Cover Date.     

涡轮流量计转子内完全三元流场的变域变分有限元解

三、涡轮流量计仪表特性曲线的计算由动量矩原理可知,当转子处于平衡时,可得到力矩平衡方程 T_d=∑T_i=T_h T_b T_t T_m T_P T_f下面分别讨论各力矩的大小。     

BUAA-SID1.0空间目标图像数据库

随着太空竞争的加剧,空间目标监视及目标识别受到越来越多国家的重视。而空间目标图像数据库的缺乏直接影响了空间目标识别技术的研究进展。针对这一问题,建立了BUAA-SID1.0空间目标图像数据库。文章在分析空间目标图像数据库建立的背景和意义的基础上,介绍了数据库的建立方法,指出了数据库共享版本BUAA-SID-share1.0的内容,给出了两种识别算法在共享数据库上的测试结果。