The Progress of the Taiwan Oscillation Network Project

We describe the present status of the project of the Taiwan Oscillation Network (TON) and discuss a scientific result using the TON data. The TON is a ground-based network to measure solar intensity oscillations for the study of the solar interior. Four telescopes have been installed in appropriate longitudes around the world. The TON telescopes take K-line full-disk solar images of diameter 1000 pixels at a rate of one image per minute. The data has been collected since October of 1993. The TON high-spatial-resolution data are specially suitable for the study of local properties of the Sun. In 1997 we developed a new method, acoustic imaging, to construct the acoustic signals inside the Sun with the acoustic signals measured at the solar surface. From the constructed signals, we can form intensity map and phase-shift map of an active region at various depths. The direct link between these maps and the subsurface wave-speed perturbation suffers from the poor vertical resolution of acoustic imaging. Recently an inversion method has been developed to invert the measured phase travel time perturbation to estimate the distribution of wave-speed perturbation based on the ray approximation. This technique of acoustic imaging has been used to image the far-side of the Sun that could provides information on space weather prediction. The TON Team includes: Antonio Jimenez (Instituto Astrofisica de Canarias, Spain); Guoxiang Ai and Honqi Zhang (Huairou Solar Observing Station, P.R.C.); Philip Goode and William Marquette (Big Bear Solar Observatory, U.S.A.); Shuhrat Ehgamberdiev and Oleg Ladenkov (Ulugh Beg Astronomical Institute, Uzbekistan) This revised version was published online in August 2006 with corrections to the Cover Date.     

基于IPDG方法的嵌套网格技术

在内罚间断伽辽金（IPDG）方法框架内应用嵌套网格技术求解了二维可压缩Navier-Stokes方程。通过把黏性通量作为辅助变量实现了Navier-Stokes方程的降阶,继而用间断有限元方法进行离散得到空间半离散方程。时间推进采用Newton-Krylov隐式方法。利用库埃特流动精确解验证了该方法的精度。在此基础上,对包括有黏NACA0012翼型绕流、定常和非定常的圆柱绕流在内的若干典型测试算例开展数值模拟,进一步验证了该方法的鲁棒性和可靠性。在嵌套网格中应用了h型网格自适应技术用于提高激波分辨率,对NACA0012翼型无黏跨声速绕流开展数值模拟,结果表明：自适应之后的单元数相比无自适应时只增加了8.4%,但是激波分辨率得到了显著提高,激波附近的计算结果也与实验值符合得更好,从而验证了该方法的有效性。     

固体发动机内弹道计算分析中的几个问题

对固体发动机内弹道进行了分析，获得了喷喉面积和燃速的变化规律及燃面到肉厚的关系，同时阐述了内弹道性能计算分析了中有关问题。     

锥柱形装药旋转火箭发动机的零维内弹道计算

介绍了锥柱形装药的旋转固体火箭发动机的零维内弹道计算方法.计算结果与旋转试验结果吻合较好,两种结果均表明锥柱形装药呈现较大的加速度场效应.     

旋转对固体火箭发动机的影响

对旋转对固体火箭发动机的影响进行了初步探讨。给出了旋转对推进剂应力应变的影响、产生的热力学方面的影响及旋转引起的气体动力学的影响等的分析计算模型。并在内弹道计算的基础上,对上述影响引起的发动机性能的变化进行了分析比较,得出了有意义的结论。     

SOHO: The Solar and Heliospheric Observatory

The Solar and Heliospheric Observatory (SOHO), together with the Cluster mission, constitutes ESA's Solar Terrestrial Science Programme (STSP), the first Cornerstone of the Agency's long-term programme Space Science — Horizon 2000. STSP, which is being developed in a strong collaborative effort with NASA, will allow comprehensive studies to be made of the both the Sun's interior and its outer atmosphere, the acceleration and propagation of the solar wind and its interaction with the Earth. This paper gives a brief overview of one part of STSP, the SOHO mission.     

打击复杂地形目标的导弹再入机动弹道设计

建立了再入机动弹道数学模型，给出了气动力系数为速度、迎角、高度的函数拟合式，进行了最佳再入机动弹道设计和仿真计算。结果表明，数学模型正确，计算方法可行，利用再入机动弹道技术可有效地打击复杂地形目标、提高导弹的作战效能和突防能力。     

基于严格成像模型的卫星姿态角系统误差补偿

为消除卫星在轨运动过程中俯仰、偏航、滚动对遥感影像地面定位的影响,建立了卫星姿态角系统误差补偿模型,即在严格成像模型的基础上,对姿态角进行直接调整,以减小定位误差。利用环境减灾-1B（HJ-1B）卫星CCD1相机遥感影像进行分析,在单景影像的定位中,借助于2个地面控制点,将其系统误差减小到原来的1/3,从而验证了模型的有效性,为进一步在轨检校相机内部静态参数提供了前提。     

某型延寿助推器内弹道性能预示

在建立某型延寿助推器翼柱型装药的仿真模型和数学模型的基础上,对该型助推器装药进行了数值模拟,完成了内弹道性能预示,得出了该型延寿助推器燃烧室压强和推力随时间变化的规律,并根据内弹道性能预示结果分析该型延寿助推器继续使用的可能性     

靶场外弹道测量系统最优布站方法研究

外弹道测量系统最优布站是靶场的一项重要工作。描述了布站优化目 标函数和约束条件,阐述了基于遗传算法的求解过程,对距离距离变化率测量系统进行了优 化布站,结果表明该算法可用于外测系统的优化布站设计,为靶场测量系统优化布站提供了 一种新的方法。