低轨卫星的北斗反射信号海洋覆盖分析

北斗系统作为我国自行研制的导航系统，具有独特的混合星座特性，其反射事件在海洋上的空间分布和覆盖性能的研究成果较少。针对上述问题，模拟了北斗三号（Beidou System 3，BDS3）以及全球定位系统（Global Positioning System，GPS）空间星座，模拟不同性能参数的低轨接收卫星，在此仿真系统的基础上，计算反射事件在各仿真场景下的海洋覆盖率以及同时发生反射事件的卫星数量。结果表明：BDS3与GPS相比具有更大的反射事件海洋覆盖率，覆盖性能更优；仿真周期7天与1天相比,前者卫星产生的反射事件海洋覆盖率约为后者5倍；低轨道卫星（Low Earth Orbit,LEO）轨道高度越高，天线波束角度越大，反射事件海洋覆盖率越大；3颗LEO卫星下同时发生反射事件卫星数的平均值约为单颗LEO卫星的3倍。可通过设计多星组网来提高反射事件海洋覆盖率。研究结果对星载反射技术海洋遥感应用方面有一定的参考价值。     

Response of the Earth’s lower ionosphere to the Ground Level Enhancement event of December 13, 2006

In this study we analyze the Ground Level Enhancement Event No 70 observed on December 13, 2006, by correlating the observations from two research topics: Cosmic rays and Very Low Frequency (VLF < 30 kHz) wave propagation, as two ground based techniques for the detection of solar proton events, and their impact on the lower ionosphere. The observations have been endorsed from recordings of worldwide network ground based Neutron Monitors as well as by satellite data from the satellites GOES 12 (www.swpc.noaa.gov) and Pamela (www.pamela.roma2infn.it).     

叶片外物损伤的实验模拟及其疲劳强度的研究

研究了空气炮法模拟外物损伤叶片的可行性,分析了外物损伤对模拟叶片疲劳强度的影响规律。用空气炮发射以300m/s左右速度发射直径1~4mm的钢珠,冲击模拟叶片,空气炮法在发射速度控制和撞击缺口深度方面具有较强的可控性及可重复性。采用光学和扫描电子显微镜对外物损伤的宏观和微观特征进行了观察,冲击损伤处具有材料丢失、塑性变形、剪切撕裂、应力集中、微裂纹、空穴结构和材料的折叠等特征。采用步进法对部分外物损伤模拟叶片进行了高周疲劳强度测试,试验结果比较分散,且冲击损伤引起的高周疲劳强度下降不随缺口深度的增加而单调变化,表明物损伤模拟叶片的疲劳强度是受缺口的宏观特征、微观特征等综合因素的影响。     

高负荷离心压气机扩压器叶片前缘结构分析

为拓宽离心压气机稳定工作范围,以某高负荷离心压气机为研究对象,对径向扩压器叶片前缘进行盘侧开槽处理,借助数值模拟手段,探讨了开槽处理对离心压气机性能和稳定工作范围的影响,并对开槽结构进行了参数化研究,确定了主要开槽参数对离心压气机的影响.数值计算表明,径向扩压器前缘盘侧开槽能够在一定程度上提高离心压气机的稳定工作裕度,但同时伴随着压气机性能的降低.详细对比分析了开槽结构引人前后离心压气机内部流场结构,揭示了径向扩压器叶片前缘开槽提高离心压气机稳定工作裕度机理.     

"伊春空难"对航空运输上市公司股价的影响

用事件研究方法就伊春空难对航空运输板块上市公司股价的影响进行了实证分析。实证结果表明,伊春空难的发生对航空运输板块上市公司的股价造成了短暂的下跌,其原因可归结为航空运输股受宏观环境影响较大,但事件发生后社会各方积极采取补救措施,从而将该事件的负面影响降至最低。航空运输业的安全需要国家有关部门严格规范的管理,也需要航空公司从硬件和人员两方面进行改进。     

风扇叶片脱落机匣包容性仿真并行计算一致性研究

风扇叶片脱落并行计算结果的一致性非常重要。在共享内存并行(SMP)模式下,由于计算随机误差和误差累积现象的存在,计算结果可能不一致。针对该问题,对某型大涵道比涡扇发动机简化的三叶片模型进行并行仿真计算,分析造成计算结果不一致的误差来源,提出四种控制策略,研究表明,通过计算方法的改进和计算平台的选择可以有效避免误差累积现象,提高并行计算精度。     

太阳微波脉冲事件的时变特性

本文利用瑞士Berne大学1988年1月-1989年12月发布的15个太阳微波脉冲事件的观测资料，分析其时间轮廓的3个主要特征：脉冲度、不对称性和半功率宽度频率响应．这些特性，可以定性地用非热电子的连续注入模，和不均匀的源模型给出较合理的解释．     

巧用Creat（）和SyntaxFromSQL（）函数创建动态数据窗口

本文以两个实例介绍了在PB环境下，利用Creat()和SyntaxfromSQL()函数创建动态数据窗口的设计方法。     

Study on solar sources and polar cap absorption events recorded in Antarctica

Particularly intense events occurred on the Sun in a period around minimum of solar activity during cycle 23. We investigated the characteristics of September 2005 and December 2006 events and the properties of the correlated observations of ionospheric absorption, obtained by a 30 MHz riometer installed at Mario Zucchelli Station (MZS-Antarctica), and of geomagnetic activity recorded at Scott Base (Antarctica). Solar events are studied using the characteristics of CMEs measured with SoHO/LASCO coronagraphs and the temporal evolution of solar energetic protons in different energy ranges measured by GOES 11 spacecraft.     

Physics of ion acceleration in the solar flare on 2005 September 7 determines γ-ray and neutron production

Relativistic neutrons were observed by the neutron monitors at Mt. Chacaltaya and Mexico City and by the solar neutron telescopes at Chacaltaya and Mt. Sierra Negra in association with an X17.0 flare on 2005 September 7. The neutron signal continued for more than 20 min with high statistical significance. Intense emissions of γ-rays were also registered by INTEGRAL, and during the decay phase by RHESSI. We analyzed these data using the solar-flare magnetic-loop transport and interaction model of Hua et al. [Hua, X.-M., Kozlovsky, B., Lingenfelter, R.E. et al. Angular and energy-dependent neutron emission from solar flare magnetic loops, Astrophys. J. Suppl. Ser. 140, 563–579, 2002], and found that the model could successfully fit the data with intermediate values of loop magnetic convergence and pitch-angle scattering parameters. These results indicate that solar neutrons were produced at the same time as the γ-ray line emission and that ions were continuously accelerated at the emission site.