Longitudinal variation of the equatorial ionosphere: Modeling and experimental results

We describe a new version of the Parameterized Regional Ionospheric Model (PARIM) which has been modified to include the longitudinal dependences. This model has been reconstructed using multidimensional Fourier series. To validate PARIM results, the South America maps of critical frequencies for the E (foE) and F (foF2) regions were compared with the values calculated by Sheffield Plasmasphere-Ionosphere Model (SUPIM) and IRI representations. PARIM presents very good results, the general characteristics of both regions, mainly the presence of the equatorial ionization anomaly, were well reproduced for equinoctial conditions of solar minimum and maximum. The values of foF2 and hmF2 recorded over Jicamarca (12°S; 77°W; dip lat. 1°N; mag. declination 0.3°) and sites of the conjugate point equatorial experiment (COPEX) campaign Boa Vista (2.8°N; 60.7°W; dip lat. 11.4°; mag. declination −13.1°), Cachimbo (9.5°S; 54.8°W; dip lat. −1.8°; mag. declination −15.5°), and Campo Grande (20.4°S; 54.6°W; dip lat. −11.1°; mag. declination −14.0°) have been used in this work. foF2 calculated by PARIM show good agreement with the observations, except during morning over Boa Vista and midnight-morning over Campo Grande. Some discrepancies were also found for the F-region peak height (hmF2) near the geomagnetic equator during times of F₃ layer occurrences. IRI has underestimated both foF2 and hmF2 over equatorial and low latitude sectors during evening-nighttimes, except for Jicamarca where foF2 values were overestimated.     

拦截高速目标的比例与反比例导引捕获区分析

针对拦截高速目标的作战特点,分析了比例导引(PN)与反比例导引(RPN)的捕获区。首先,通过分析拦截弹与目标的相对运动关系,推导得到了顺轨和逆轨的零控拦截条件,此条件由目标和拦截弹的速度前置角以及二者速度比确定;其次,以拦截弹和目标速度前置角为坐标系,推导得到了PN以及RPN捕获区以及各自导航比设置范围。PN的捕获区由逆轨零控拦截条件以及与其相切且斜率为1/(N-1)的两条直线构成,RPN的捕获区由顺轨零控拦截条件以及与其相切且斜率为1/(-N-1)的两条直线构成;然后,利用函数对称性将PN与RPN捕获区转换到同一坐标区间,得到了相同条件下RPN捕获区要大于PN捕获区的结论;最后,开展了四种情形下的仿真,验证了本文捕获区分析的合理性及有效性。     

深冷组合循环发动机吸气模态循环分析与设计可行域研究

为了研究类似SABRE3结构的深冷组合循环发动机,建立了基于部件法的发动机设计点热力学计算模型,提出了发动机氦循环新的循环效率和循环特征参数的定义。考虑发动机参数的物理限制条件及不同工质循环之间的相互影响,求解得到了空气路、氦气路重要参数的设计可行域。在可行域内开展了空气路和氦气路的循环分析,获到了冷却当量比、性能参数等主要参数的分布结果。结果表明:此发动机空气热功转换比ηt2为0.02～0.746。氦循环设计可行域受ηt2及换热器热负荷限制;循环起始温度和热负荷限制确定的情况下,ηt2越低氦循环可行域越窄。降低发动机冷却当量比的关键是:提高换热器1的氦出口温度以降低氦流量;当换热器1和换热器2的氦出口温度同时取得最大值时,冷却当量比取得最小值。换热器1和2的氦出口温度分别取1200K和1300K时,空气路可行域内冷却当量比为0.917～2.64。     

相关进近模式的近距平行跑道尾流危险区域分析

相比于机场一起一降的运行模式,近距平行跑道的相关平行进近运行模式可以最大限度地提升跑道容量.根据尾流在大气中各个阶段的运动特性,得到了以时间为变量的尾流水平侧移距离数学模型.应用Matlab仿真软件得到了侧风及地面效应影响情况下的上海虹桥国际机场实行近距平行跑道相关平行进近的侧向尾流危险区域图,并分析得到了后机不受到前机尾流影响情况下两机需保持26.9 s的最大尾流时间间隔.利用尾流危险区域的特点,可缩短尾流时间间隔,从而大幅度提高机场容量.     

中医色诊客观化系统的开发与初步应用(英文)

研制开发了中医色诊客观化研究专用系统。该系统包括硬件和软件两部分。硬件是一个标准光源环境的图像采集装置,主要由色温为5500K的氙灯、漫反射积分球和高分辨率CCD数码相机组成。软件用于图像处理,处理过程分为3步:首先使用灰度阈值将原始图像进行肤色/非肤色分类,然后通过图像分割和坐标排序定位人脸特征,最后应用形态学技术提取与人体五脏对应的色部区域并且计算区域色度值。使用该系统采集和处理了30例年轻人和53例老年人的样本。实验结果表明年轻人和老年人色部数据有显著性差异。初步应用验证了系统在中医色诊客观化研究中的良好性能。     

基于最小总体偏差和区域信息Snake模型的图像分割

提出基于最小总体偏差和区域信息Snake模型的图像分割方法。根据最小总体偏差准则，用包含区域信息的变力替换在气球力Snake模型中的恒定力，并应用于图像分割。实验结果表明，该模型与初始轮廓曲线位置无关，能自动分割模糊边界。对于带椒盐噪声的图像，应用该模型也能取得满意的分割效果。     

海南地区电离层闪烁监测及初步统计分析

为开展赤道区的电离层闪烁形态特性及相关物理过程的研究,空间中心海南台站建立了一套GPS电离层闪烁监测系统．该系统是利用Plessey GPS Builder-2系统开发的,对软件的源码进行了修改,使其能以高采样率(50／s)同时并行记录11个通道GPS信号强度数据．对2003年7—12月间L-波段电离层闪烁事件的初步统计分析结果表明,电离层闪烁主要发生在日落后到午夜附近,其中9—11月较7—8月闪烁发生和结束的时间明显提前;电离层闪烁发生的频率和强度在9—11月较其他月份明显增强,其中10月达到最大;电离层闪烁的逐日变化具有很强的随机性,闪烁的发生在秋分附近9月底到10月中旬的磁静日期间达到最大;太阳和地磁活动的增强通常会抑制电离层闪烁的发生,这种情形在秋分附近尤为明显．     

Response of Hainan GPS ionospheric scintillations to the different strong magnetic storm conditions

Using the GPS ionospheric scintillation data at Hainan station (19.5°N, 109.1°E) in the eastern Asia equatorial regions and relevant ionospheric and geomagnetic data from July 2003 to June 2005, we investigate the response of L-band ionospheric scintillation activity over this region to different strong magnetic storm conditions (Dst < −100 nT) during the descending phase of the solar cycle. These strong storms and corresponding scintillations mainly took place in winter and summer seasons. When the main phase developed rapidly and reached the maximum near 20–21 LT (LT = UT + 8) after sunset, scintillations might occur in the following recovery phase. When the main phase maximum occurred shortly after midnight near 01–02 LT, following the strong scintillations in the pre-midnight main phase, scintillations might also occur in the post-midnight recovery phase. When the main phase maximum took place after 03 LT to the early morning hours no any scintillation could be observed in the latter of the night. Moreover, when the main phase maximum occurred during the daytime hours, scintillations could also hardly be observed in the following nighttime recovery phase, which might last until the end of recovery phase. Occasionally, scintillations also took place in the initial phase of the storm. During those scintillations associated with the nighttime magnetic storms, the height of F layer base (h’F) was evidently increased. However, the increase of F layer base height does not always cause the occurrence of scintillations, which indicates the complex interaction of various disturbance processes in ionosphere and thermosphere systems during the storms.     

太阳宁静区磁漏斗结构的扩展特征

通过对观测的光球纵向磁场进行势场外推, 重构了一个太阳宁静区光球以上的磁场结构. 结果显示, 在20 Mm 以下, 开放磁力线呈现多个明显的小磁漏斗结构, 这些小磁漏斗结构随高度扩展, 并且在20 Mm 左右融合成大的漏斗结构. 通过系统地研究磁漏斗结构横截面积随高度的变化趋势, 发现太阳宁静区磁漏斗结构的截面积随高度近似线性扩展, 磁漏斗结构在较低高度上(<20Mm) 扩展的速度比在较高高度上 (>20Mm) 扩展的速度要快. 这一结果对太阳风起源和磁环中物质流动的二维数值模拟具有重要的意义. 同时还发现, 闭合磁力线的数目随高度以指数函数的形式减少.      

离心压气机转子内近端壁区三维紊流流场

用三维激光多普勒测速系统测量研究了一个离心压气机转子近端壁区三维紊流流场。结果表明,整个叶片通道内叶背角区存在角涡及其伴随涡,叶盆角区存在前缘马蹄涡的叶盆分支,它们的发展、演化较大地影响着附近区域的流动,是造成了所在区域流动阻塞和气流脉动的主要因素。前缘马蹄涡叶背分支沿下游逐渐向叶盆方向发展,与端壁附面层和主流的进一步掺混,并在约 1 /2叶片通道处的叶盆角区与前缘马蹄涡的叶盆分支发生交混,在下游造成一定强度的流动阻塞和紊流脉动带。