地球同步轨道高能电子增强事件预报方法

分析了地球同步轨道高能电子通量增强事件的发生规律及其与太阳风和行星际磁场参数的关系，并在此基础上建立了基于人工神经网络的高能电子增强事件模式，经实测数据检验，预报模式可以对未来1天的高能电子通量进行预报，误差为8．2％，达到了较高水平．     

基于等高线图与小波变换的3D地形匹配算法研究

提出一种新的基于边缘的3D地形匹配算法。在算法中，一种结构紧凑的特征“等高线图”，用于表示参考高程图(DEM)及从实时数据恢复的高程图，这样3D地形匹配转化为基于等高线的匹配，即边缘(平面曲线)匹配问题。在边缘匹配过程中，首先用一种具有平移，旋转，尺度不变性的规范化小波描述子描述边缘。其次提出了一种基于小波系数域的快速边缘匹配算法，并分析了运算复杂性。由匹配成功的边缘对提取控制点的坐标。讨论了图像变换模型及基于最小均方根误差准则的图像变换参数估计方法。用真实地形实验表明该算法匹配精度高，计算速度快。最显著的特点是该算法抗噪声能力强。     

一种快速有效的雷达目标识别方法

基于核的学习算法提出一种快速有效的雷达目标识别方法。首先利用核的主分量分析方法对雷达目标的一维距离像进行特征提取,可以有效地提取出其中的非线性特征;然后基于一种新型的支撑矢量机——近似支撑矢量机作为分类器对所提取的特征进行识别。实验结果表明,所提出的识别方法其正确识别率与标准支撑矢量机相当,但在计算速度上却有很大的提高,并对噪声具有较好的抑制作用。     

Launch and commissioning of the PAMELA experiment on board the Resurs-DK1 satellite

PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature in a wide energy range (protons: 80 MeV–700 GeV, electrons 50 MeV–400 GeV). Main objective is the study of the antimatter component: antiprotons (80 MeV–190 GeV), positrons (50 MeV–270 GeV) and search for antimatter (with a precision of the order of 10⁻⁸). The experiment, housed on board the Russian Resurs-DK1 satellite, was launched on June, 15th 2006 in a 350 × 600 km orbit with an inclination of 70°. The detector consists of a permanent magnet spectrometer core to provide rigidity and charge sign information, a Time-of-Flight system for velocity and charge information, a silicon–tungsten calorimeter and a neutron detector for lepton/hadron identification. An anticounter system is used off-line to reject false triggers coming from the satellite. In self-trigger mode the calorimeter, the neutron detector and a shower tail catcher are capable of an independent measure of the lepton (e⁺ + e⁻) component up to 2 TeV. In this work we focus on the first months of operations of the experiment during the commissioning phase.     

Dark matter search with the CALET detector on-board ISS

The CALorimetric Electron Telescope, CALET, mission is proposed for the observation of high-energy electrons and gamma-rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe the electrons (without separation between e⁺ and e⁻) in 1 GeV–10 TeV and the gamma-rays in 20 MeV–several TeV with a high-energy resolution of 2% at 100 GeV, a good angular resolution of 0.06 degree at 100 GeV, and a high proton-rejection power of nearly 10⁶. The CALET has a geometrical factor of 1 m²sr, and the observation period is expected for more than three years. The very precise measurement of electrons enables us to detect a distinctive feature in the energy spectrum caused from WIMP dark matter in the Galactic halo. The excellent energy resolution of CALET, which is much better than GLAST or air Cherenkov telescopes over 10 GeV, enables us to detect gamma-ray lines in the sub-TeV region from WIMP dark matter annihilations. The CALET has, therefore, a unique capability to search for WIMP dark matter by the hybrid observations of electrons and gamma-rays.     

论高校医院与全科医学

摘 要 保证高校教职工、大学生的身心健康，是高校医院义不容辞的责任。为此，应探索一条更适合高校实际情况的医疗模式。本文就高校医院应如何为师生员工提供全方位的医疗保健服务进行了初步探讨。