Relativistic MHD Simulations of Jets with Toroidal Magnetic Fields

This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach.     

一种新的共轭增强MUSIC测向算法

提出一种新的测向算法。利用阵列输出的非零时延互相关函数及其共轭形成伪阵列输出,从而得到伪协方差矩阵,对其进行特征分解,利用信号子空间与噪声子空间的正交性,搜索得到的空间谱函数的极大值点对应的角度就是波达方向。仿真实验表明,新算法可对多于阵元数的信号进行测向,其测角精度和分辨力优于MUISC和MUSIC-like算法。     

激光靶斑阵列数据遥测系统传输特性分析

介绍了一种用于激光靶场试验中测量激光靶斑阵列数据的ＷＹＫ２１遥测系统，对该系统的传输特性，包括数据传输误码率，遥测接收灵敏度和系统功率传输裕量进行了分析研究。     

固定容差参数的阵列天线方向图综合法

研究了设计参数具有固定容差的阵列天线方向图综合法;给出了阵列天线方向图容差优化的数学模型;提出了求解容差优化最坏情况问题的离散化方法;建立了直线阵列天线容差区内误差任意分布的物理模型,并采用修正正多面体优化方法对激励幅度具有容差的侧射天线阵进行了综合。当设计参数偏离其标称值时,文中的综合方法可以使天线性能的偏差最小。     

Study on the breakup lengths of free round liquid jets

IntroductionBreakup and atomization of roundliquidjetshad been widely used in internal combustion en-gines,gas turbines,and liquid rocket engines.Recently,with the development of scramjet en-gines and the deepening of fuel atomization re-search,it attract…     

轴对称湍流射流的相似解

本文在相似性条件下,得到了用k-ε模式的轴对称湍流射流的相似方程。利用动量相似方程的近似求解结果作为初值,同时引入变量变换,进行迭代求解。本文的方法收敛速度快,计算简便。     

带有太阳电池阵的卫星电源系统在轨测试方法

根据带有太阳帆板的地球同步卫星在轨测试需求，分析了星上电源系统的组成及技术状态；并以光照区可调节母线为例。给出了卫星电源系统在轨测试方法及相应的计算公式；最后，通过工程验证了该方法的正确性。     

A survey of radio jets with Chandra and HST

Relativistic jets are a common property of radio-loud Active Galactic Nuclei (AGN). Understanding jet physical properties is an essential precursor to understanding the mechanisms of energy transport, and ultimately, how energy is extracted from the central black hole. In this paper, I highlight recent developments from Chandra and HST observations of kpc-scale jets in AGN, with particular emphasis on our survey of 17 radio jets in a sample of FRII radio galaxies. These observations show that (1) X-ray and optical emission is common from kpc-scale jets, (2) a large fraction of the bolometric luminosity is emitted at X-rays, and (3) in most sources, a candidate emission process for the X-rays is inverse Compton scattering of the Cosmic Microwave Background off the relativistic electrons in the jet. If the latter scenario holds, the implication is that jets are still relativistic on kpc scales.     

Study of the variability of blazars gamma-ray emission

The γ-ray emission of blazar jets shows a pronounced variability and this feature provides limits to the size and to the speed of the emitting region. We study the γ-ray variability of bright blazars using data from the first 18 months of activity of the Large Area Telescope on the Fermi Gamma-Ray Space Telescope. From the daily light-curves of the blazars characterized by a remarkable activity, we firstly determine the minimum variability time-scale, giving an upper limit for the size of the emitting region of the sources, assumed to be spheroidal blobs in relativistic motion. These regions must be smaller than ∼10⁻³ parsec. Another interesting time-scale is the duration of the outbursts. We conclude that they cannot correspond to radiation produced by a single blob moving relativistically along the jet, but they are either the signature of emission from a standing shock extracting energy from a modulated jet, or the superposition of a number of flares occurring on a shorter time-scale. We also derive lower limits on the bulk Lorentz factor needed to make the emitting region transparent for gamma-rays interacting through photon–photon collisions.