A Class of TVD Type Combined Numerical Scheme for MHD Equations With a Survey About Numerical Methods in Solar Wind Simulations

It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participate in the numerical modelling of atmospheric environments as well as the meteorological conditions at Earth. Space scientists have paid great attention to operational numerical space weather prediction models. To this purpose practical progress has been made in the past years. Here first is reviewed the progress of the numerical methods in solar wind modelling. Then, based on our discussion, a new numerical scheme of total variation diminishing (TVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with MacCormack II scheme for the purpose of developing a combined scheme of quick convergence as well as of TVD property. To verify the validation of the scheme, the propagation of one-dimensional MHD fast and slow shock problem is discussed with the numerical results conforming to the existing results obtained by the piece-wise parabolic method (PPM). Finally, some conclusions are made. This revised version was published online in August 2006 with corrections to the Cover Date.     

一种求解武器--目标分配问题的新方法

提出了一种求解武器-目标分配问题的新方法.阐明了将武器-目标分配问题作为组合优化问题,采用遗传算法进行求解,并针对问题特点,给出了基于系统信息的启发式操作方法及适合的操作算子.仿真结果表明,此方法可以明显提高问题求解的速度及精度.     

平面动力系统的ω（α）极限集的一些性质

本文论述了平面动力系统的ω(α)极限集在轨道有界时的一些性质，并对轨道无界情形下其极限集的结构做了一些初步研究。     

AEDMS工程文件编号的生成算法

工程文件编号生成算法是国航工程文件管理系统（AEDMS）开发的难点。提出的．工程文件编号生成算法包括．工程文件流水号和改版号的指派算法与自动编排算法。前者解决了新旧系统．工程文件编号的兼容问题；后者是一种新的基于关系代数的自动编号算法，其利用元组序号，具有紧凑简单、可靠性好、可维护性好、执行效率高、适用面广的特点。实算结果和AEDMS运行实践表明，此工程文件编号生成算法是可行的。     

天基信息支援对导弹攻防作战的效用分析

分析了空天一体作战天基装备系统——军事卫星,对导弹攻防作战重要的信息支援效用。建立并阐述了天基军事卫星信息系统信息支援下导弹攻防作战过程模型和影响图模型,对模型进行了详细的分析讨论。     

廊坊市大学生生活现状调查及其浅析

青年,尤其是当代大学生是一个国家发展的重要后备力量,他们的健康成长关乎着国家未来和民族的兴衰。通过对廊坊市区内五所高校的部分大学生在大学期间的各项时间分配情况的调查,反映出当前我市大学生具有规律性的一些生活现状。并对此进行认真分析,提出了高校及教育管理部门在大学生教学、教育过程中应注意的问题。     

逻辑无环流系统中逻辑控制器的设计

本文在给出逻辑无环流系统基础上,主要介绍关于DLC设计的有关问题.逻辑控制器DLC是系统的关键部件,必须保证可靠工作.通过实际验收,说明了设计的有效性.     

一种飞船返回舱落点选优算法的设计与实现

设计一种选优算法。算法依据概率论,以寻找落点最密集区域为思路,从已知众多飞船返回舱落点数据中计算产生一个“优秀”落点,即尽可能接近返回舱的实际着陆点。     

Physical characterization of the deep-space debris WT1190F: A testbed for advanced SSA techniques

We report on extensive ${\mathit{BVR}}_c{I}_c$ photometry and low-resolution ($\lambda /\mathrm{\Delta }\lambda ～250$) spectroscopy of the deep-space debris WT1190F, which impacted Earth offshore from Sri Lanka, on 2015 November 13. In spite of its likely artificial origin (as a relic of some past lunar mission), the case offered important points of discussion for its suggestive connection with the envisaged scenario for a (potentially far more dangerous) natural impactor, like an asteroid or a comet.Our observations indicate for WT1190F an absolute magnitude $R_c={32.45}_{\pm 0.31}$, with a flat dependence of reflectance on the phase angle, such as ${\mathit{dR}}_c/d?～{0.007}_{\pm 2}$?mag?deg^?1. The detected short-timescale variability suggests that the body was likely spinning with a period twice the nominal figure of $P_{\mathrm{flash}}={1.4547}_{\pm 0.0005}\mathrm{s}$, as from the observed lightcurve. In the ${\mathit{BVR}}_c{I}_c$ color domain, WT1190F closely resembled the Planck deep-space probe. This match, together with a depressed reflectance around 4000 and 8500 Å may be suggestive of a “grey” (aluminized) surface texture.The spinning pattern remained in place also along the object fiery entry in the atmosphere, a feature that may have partly shielded the body along its fireball phase perhaps leading a large fraction of its mass to survive intact, now lying underwater along a tight ($～1\times 80$?km) strip of sea, at a depth of 1500?m or less.Under the assumption of Lambertian scatter, an inferred size of ${216}_{\pm 30}/\sqrt{\alpha /0.1}$?cm is obtained for WT1190F. By accounting for non-gravitational dynamical perturbations, the Area-to-Mass ratio of the body was in the range $(0.006?\mathit{AMR}?0.011)$?m²?kg^?1.Both these figures resulted compatible with the two prevailing candidates to WT1190F’s identity, namely the Athena II Trans-Lunar Injection Stage of the Lunar Prospector mission, and the ascent stage of the Apollo 10 lunar module, callsign “Snoopy”. Both candidates have been analyzed in some detail here through accurate 3D CAD design mockup modelling and BRDF reflectance rendering to derive the inherent photometric properties to be compared with the observations.     

颈动脉内血流动力学特征受向前加速度影响的数值模拟

人们在日常或某些特殊条件下常会面临方向和大小发生迅速变化的加速度环境,已有研究发现加速度环境会影响心血管系统生理、病理特征。利用计算机模拟方法详细研究了向前加速度环境下人体颈动脉内的血流动力学参数变化规律。结果表明:加速度会对颈动脉内压力、压力梯度、壁面剪切应力等与血管生理、病理现象密切相关的血流动力学参数产生显著影响。研究结果为加速度环境下颈动脉生理、病理研究提供了一定的理论依据,也为航空航天领域加速度环境下人员防护提供参考。