The Tien-Shan mountain cosmic ray station of the Ionosphere Institute of Kazakhstan Republic

The mountain cosmic ray (CR) station of the Ionosphere Institute of Kazakhstan Republic (CR station Alma-Ata B, 43.1N latitude, 76.6E longitude, geomagnetic rigidity cutoff 6.69 GV) is a center for an experimental study of the non-stationary processes caused by cosmic rays of different origin in the interplanetary and near-Earth space, so as their influence on the state of the Earth’s magnetosphere and the upper atmosphere layers. This paper summarizes efforts performed over the years by the Almaty CR group till its present status.     

Real-time GLE alert in the ANMODAP Center for December 13, 2006

Within the last years, a real-time system to monitor high energy cosmic rays for space weather use has been operated at Athens cosmic ray station. Neutron monitors and satellite high resolution data in real time are used, making it possible to observe cosmic rays in dual energy range observations. In large solar energetic particle (SEP) events, ground level enhancement (GLE) can provide the earliest alert for the onset of the SEP event. This system watches for count rate increases recorded in real time by 23 neutron monitors, which triggers an alarm if a ground level enhancement (GLE) of cosmic ray intensity is detected.     

Broad-search algorithms for the spacecraft trajectory design of Callisto–Ganymede–Io triple flyby sequences from 2024 to 2040, Part II: Lambert pathfinding and trajectory solutions

Triple-satellite-aided capture employs gravity-assist flybys of three of the Galilean moons of Jupiter in order to decrease the amount of ΔV$\mathrm{\Delta }V$ required to capture a spacecraft into Jupiter orbit. Similarly, triple flybys can be used within a Jupiter satellite tour to rapidly modify the orbital parameters of a Jovicentric orbit, or to increase the number of science flybys. In order to provide a nearly comprehensive search of the solution space of Callisto–Ganymede–Io triple flybys from 2024 to 2040, a third-order, Chebyshev's method variant of the p-iteration solution to Lambert's problem is paired with a second-order, Newton–Raphson method, time of flight iteration solution to the _V∞$V_{\infty }$-matching problem. The iterative solutions of these problems provide the orbital parameters of the Callisto–Ganymede transfer, the Ganymede flyby, and the Ganymede–Io transfer, but the characteristics of the Callisto and Io flybys are unconstrained, so they are permitted to vary in order to produce an even larger number of trajectory solutions. The vast amount of solution data is searched to find the best triple-satellite-aided capture window between 2024 and 2040.     

序列图像中直线边缘快速提取和匹配

针时飞行器视觉导航等实时性较强的应用,给出了一种在航空序列图像中进行直线边缘快速提取和匹配的方案。在提取直线边缘时,运用了当前速度较快的邻接元素标记方法,从而提高了直线边缘提取速度。而在时直线边缘进行匹配时,给出了一种分三步走的方案,并提出了一种能够有效降低噪声影响的度量方式。首先选择3条直线边缘作为参考模型,在直线边缘的方向、位置以及物理特性的约束下构建候选匹配基,然后在基于矢量技术的基础上确定与参考模型基相对应的匹配模型,在此基础上再确定其他直线边缘之间的对应关系。试验结果表明,本文的直线边缘匹配方法比现有的方法速度提高了30倍以上,能够有效地满足一些实时性较强的应用。     

捕捉激波的群速度控制方法

回顾及综述了群速度控制方法基本原理、发展过程及最新进展。群速度控制方法是通过控制色散误差以捕捉间断的一种数值方法。该方法通过在间断两侧采用不同色散类型的格式,将数值波的传播压制在间断附近,避免数值振荡向周围扩散,从而达到抑制数值振荡的效果。该方法主体上采用数值色散抑制振荡,实际使用中仅需补充较低水平的数值耗散就可将振荡压制在可接受的范围内。因而群速度控制格式的总体耗散水平较低,易于实现小尺度波的高分辨率捕捉,是复杂流动高分辨率数值模拟的有效方法。     

发动机进排气系统对飞机气动特性影响的数值研究

为了分析发动机与飞机系统耦合过程中产生的气动力特性,准确获取实际使用条件下的飞机升阻特性,以带动力的某半模飞机模型为研究对象,开展了三维流场数值仿真计算,利用风洞试验数据对计算方法进行了验证,总结了溢流阻力及排气干扰阻力的变化规律,结果表明:发动机状态变化对飞机升阻特性影响明显,在选定的发动机工作参考状态下,溢流阻力在飞机系统升力与阻力方向的分量随捕获面积比的增大分别增大、减小,排气系统实际工作状态偏离选定的参考状态越远,干扰阻力在飞机系统升力和阻力方向分量的绝对值越大。     

飞月轨道引力捕获设计方法研究

利用太阳引力摄动与月球绕飞设计的地月转移轨道（飞月轨道），与霍曼转移相比，虽然飞行时间较长（约三、四个月），但可显著节省速度增量（可达１５０米／秒），对无人月球探测器尤为适合。应用平面圆型限制性四体问题动力学模型，选择从月球出发的初始条件。借助“地心距－时间曲线”，从平面圆型限制性四体问题转换为一般的限制性四体问题。通过典型模拟计算，分析负向积分（从月球轨道出发）初始轨道参数及太阳方位对月球探测器     

全罗盘画面反走样算法的研究和实现

在一定分辨率的屏幕上，用常规画线函数生成的静态罗盘刻度线呈现出锯齿形失真，特别当罗盘作动态旋转时，刻度线扭曲，变形，为消除这一现象，笔者根据线条的反走样原理，提出了一种实用算法，消除了静态的锯齿形失真，并从CRT屏幕上仿真的动态效果来看，罗盘刻度线旋转时不扭曲，不变形，实验证明，在光栅图形显示器中，应用此算法可消除走样，大大增强罗盘刻度线动态显示效果。     

Calculation of the barometric coefficients at the start of the 24th solar activity cycle for particle detectors of Aragats Space Environmental Center

After the major modernization of the data acquisition electronics of the particle detectors operated at Aragats Space Environmental Center (ASEC) calculations of the barometric coefficients of all the monitors were performed in the beginning of the 24th solar activity cycle. The barometric coefficients of particle detectors located at altitudes of 1000 m, 2000 m and 3200 m a.s.l. measuring various secondary cosmic ray fluxes were compared with theoretical expectations and monitors operated on different longitudes and latitudes. The barometric coefficients were also calculated for the several neutron monitors of recently established Eurasian database (NMDB) and SEVAN particle detector networks. The latitude and altitude dependencies of the barometric coefficients were investigated, as well as the dependence of coefficients on energy of the primary particles.     

基于网络信息安全内容审计系统及相关技术研究

伴随着国家信息化不断推进和计算机网络飞速发展,网络信息安全内容审计(CASNI)成为了网络信息安全中不可或缺的重要组成部分.网络信息安全内容审计从网络关键点收集数据包,对其传送的内容进行审计分析,达到网络信息内容可控.本文描述了一种在高速网络环境下分布式、可扩展的高性能网络审计体系结构,分析了Linux(操作系统)捕获数据包的瓶颈,重点论述了使用NAPI (New Application Program Interface)技术和内存映射技术提高数据包捕获,解决审计系统中数据流高速处理的问题.