碳化硅颗粒增强铝基复合材料弹性常数测量

为研究粉末冶金制备的碳化硅颗粒增强铝基复合材料(SiCp/Al)中SiCp含量对材料机械性能的影响,使用弹性波法测量了SiCp含量不同的标准试样的弹性常数矩阵.利用Christoffel方程建立了横观各向同性材料波速与弹性常数之间的关系,介绍了水浸斜入射法测量准横波和准纵波波速的基本原理和测量过程,基于上述原理进行了试验,计算出了被测试件的弹性常数.结果表明,SiCp/Al沿挤压方向的机械性能最高,并且随着SiCp含量的增加,弹性常数变大,材料的强度升高.     

飞船返回舱俯仰振荡的动态稳定性研究

本文研究了以平衡攻角为中心作单自由度俯仰振荡的飞船返回舱,其动态稳定形态随来流M∞的变化.设θ(t)是由平衡攻角起算的俯仰振荡角,Cm是作用在飞船返回舱上的气动俯仰力矩系数,Cμ(θ,)是机械阻尼力矩(自由飞行时为零,实验时要计入其影响),文中给出飞船返回舱在平衡攻角处的俯仰振荡动态稳定性判据,并证明λ=λ(M∞)=(Cm)/()0+Cμ(0,0)1-(Cm)/(O)0是决定动稳定形态的重要参数.如果随M∞的变化,λ(M∞)由λ＜0经过λ=0变化到λ＞0,则飞船返回舱将由稳定的点吸引子形态(即稳定在平衡攻     

数值模拟中的边界处理方法研究

为适应于模拟超声速流场中的一些特殊物理现象,研究了不同物理现象对边界处理的要求.针对激波、旋涡和声波等流场中典型的流动现象,采用常用的外推、特征和缓冲三类边界处理方法分别进行数值模拟.计算结果表明超声速流场边界采用外推技术,只适于计算带有激波的边界.特征方法还能适于旋涡运动的计算.声波的计算只能采用缓冲层技术.     

Evolution of the temporal and the spectral properties in 2010 and 2011 outbursts of H 1743-322

The Galactic black hole candidate H 1743-322 exhibited two X-ray outbursts in rapid succession: one in August 2010 and the other in April 2011. We analyze archival data of this object from the PCA instrument on board RXTE (2–25 keV energy band) to study the evolution of its temporal and spectral characteristics during both the outbursts, and hence to understand the behavioral change of the accretion flow dynamics associated with the evolution of the various X-ray features. We study the evolution of QPO frequencies during the rising and the declining phases of both the outbursts. We successfully fit the variation of QPO frequency using the Propagating Oscillatory Shock (POS) model in each of the outbursts and obtain the accretion flow parameters such as the instantaneous shock locations, the shock velocity and the shock strength. Based on the degree of importance of the thermal (disk black body) and the non-thermal (power-law) components of the spectral fit and properties of the QPO (if present), the entire profiles of the 2010 and 2011 outbursts are subdivided into four different spectral states: hard, hard-intermediate, soft-intermediate and soft. We attempt to explain the nature of the outburst profile (i.e., hardness-intensity diagram) with two different types of mass accretion flow.     

Case studies of height structure of TID propagation characteristics using cross-correlation analysis of incoherent scatter radar and DPS-4 ionosonde data

The height structure of TID characteristics is studied on the base of the electron density profiles measured by two beams of the incoherent scatter radar and DPS-4 ionosonde. The height profiles of the TID propagation characteristics are obtained by means of cross-correlation and spectrum analysis of the radar and ionosonde data. The noticeable height variability of the TID parameters is observed. The variability is explained by interference of several TIDs. The obtained TID propagation characteristics are compared with known results of the TID studies.     

架空线自阻尼的测试方法

自阻尼是导线的基本特性之一。在高压架空导线防振设计中,自阻尼是一个基础数据。本文是介绍对导线自阻尼的三种测试方法。其中的“剪力法”是我们自己研创的新方法。文中不仅介绍了测量技术,还附有在我国第一次测出的 LGJQ-400型导线的自阻尼数据。     

Magneto-gravity Waves Trapped in the Lower Solar Corona

The possibility of trapped magneto-gravity waves in the lower solar corona with an open magnetic field is discussed. Intensity variations and/or Doppler shifts of relevant UV, EUV and x-ray spectral lines in the chromosphere, transition region and lower corona may reveal the existence of such low-frequency modes (with periods longer than ∼ 1.5 hour). The spectrum may be either discrete or continuous depending on the reflection property of the narrow transition region. These modes can be utilized to probe the dynamics of the upper chromosphere, transition region and lower corona; they may also play an important role in coronal heating. This revised version was published online in June 2006 with corrections to the Cover Date.     

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.