模式化分析F区电离层赤道异常槽

利用二维低纬电离层理论时变模式模拟低纬电离层演化，考察影响赤道异常槽位置的物理因素．计算结果显示赤道槽有明显的季节、地方时和经度变化．以１１０°Ｅ为例，北半球夏季期间赤道槽一般在磁倾赤道北侧，最北达３°-３．５°Ｎ，而在北半球冬季期间一般位于磁倾赤道南侧，最南可达４°－５°Ｓ．进一步分析发现，赤道槽季节变化中光化电离率季节改变的影响很小，主要由水平中性风季节变化贡献．计算以８３天为例，白天赤道槽在地理经度１００°Ｅ附近最南，２８５°Ｅ附近最北，与观测特征基本一致．主要是背景大气水平风场的经度差异导致赤道槽位置的经度变化，而非前人认为直接由磁偏角控制的．     

Responses of the African equatorial ionization anomaly (EIA) to some selected intense geomagnetic storms during the maximum phase of solar cycle 24

This study investigates the morphology of the GPS TEC responses in the African Equatorial Ionization Anomaly (EIA) region to intense geomagnetic storms during the ascending and maximum phases of solar cycle 24 (2012–2014). Specifically, eight intense geomagnetic storms with Dst ≤ ?100 nT were considered in this investigation using TEC data obtained from 13 GNSS receivers in the East African region within 36–42°E geographic longitude; 29°N–10°S geographic latitude; ± 20°N magnetic latitude. The storm-time behavior of TEC shows clear positive and negative phases relative to the non-storm (median) behavior, with amplitudes being dependent on the time of sudden commencement of the storm and location. When a storm starts in the morning period, total electron content increases for all stations while a decrease in total electron content is manifested for a storm that had its sudden commencement in the afternoon period. The TEC and the EIA crest during the main phase of the storm is significantly impacted by the geomagnetic storm, which experiences an increase in the intensity of TEC while the location and spread of the crest usually manifest a poleward expansion.     

基于图像化变差函数的性能数据异常明别

为提升发动机性能监控的智能化水平,实现性能数据的高效利用,提出了基于图像化变差函数的发动机性能数据异常 判别方法。 通过研究发动机性能数据的标准化修正方法和图像转化方法,将数值型表示的发动机性能数据转化为发动机性能图像。 通过引入变差函数理论,采用 4 方向的变差函数值表示性能特征值,融合不同时刻不同参数的性能数据。 在提取发动机性能图像关 键特征点的基础上,定义性能图像间的差异距离,实现基于变差函数的发动机性能图像异常判别方法,从而实现对发动机性能状态 的判别。 选用若干组实际发动机性能数据对方法进行验证O 验证结果表明:该方法运算高效,实现了高维性能数据的降维和对性能 图像运行状态的分类,从而判别发动机性能数据的运行状态。     

考虑地球扁率的大椭圆轨道编队飞行优化设计

大椭圆轨道上卫星编队的相对运动特性及其所受摄动力的影响给编队轨道设计者提出了新的挑战.本文总结了大椭圆轨道卫星编队的五种基本形式,利用数值积分法计算了主星轨道倾角、近地点角和平近点角初值对地球扁率作用下基本编队形式相对位置极值点漂移量的影响规律.结合零J2项摄动条件,提出基于主星平近点角初值的J2项编队相对轨道优化设计方法,进而获得瞬时根数描述的编队初始条件.仿真算例表明：优化设计结果可以明显降低大椭圆轨道编队卫星的相对漂移量,与平根数描述的编队初始条件的设计结果相比,相对距离极大值点的漂移量降低约81.8681%,验证了基于主星平近点角初值的大椭圆轨道编队优化设计方法的可行性.     

Beacon Monitoring: Reducing the Cost of Nominal Spacecraft Operations

Beacon monitoring is an architecture for augmenting on-board health assessment software with the following elements: a transmitter that periodically broadcasts this health assessment to the ground, a network of globally distributed low-cost monitoring stations that relays the health assessment to mission control, and an automated mission control system for notifying on-call operators and initiating appropriate response actions. While beacon monitoring is often cited as a means of lowering nominal monitoring costs for particular missions, these claims have typically been qualitative and undiscriminating in nature. This study introduces modeling and experimentation as means of providing a more fundamental validation of the cost-effectiveness of beacon monitoring. Results include simple quantitative estimates of first-order performance metrics, experimental data that verifies predicted performance and validates the use of beacon monitoring for a test mission, and a method for assessing the value of beacon monitoring for general satellites missions.     

无线传感网中能量优化的异常检测算法

基于网内数据处理技术和网络动态分簇技术,提出一种能量优化的异常检测算法。算法首先利用节点协作计算获取相关性信息,然后根据节点相关性和节点能量信息进行动态网络分簇,最后利用簇内相关与簇间相关性进行能量有效性的异常检测。相关测试结果表明,本文算法既保证了传感网异常检测精度又提高了网络能量利用效率。     

磁探仪应召搜潜建模与仿真

依据经典的磁探仪应召搜潜方法,以某型反潜巡逻机为背景,建立了反潜巡逻机利用磁探仪执行平行航线、扩展矩形和螺旋形搜潜模型.对3种方法的搜潜概率进行分析,仿真了相同潜艇运动模型条件下,潜艇初始位置散布、初始距离、潜艇经济航速和海洋环境磁噪声对搜潜概率的影响.实验结果表明:相同条件下,螺旋形搜潜效能最高;潜艇只进行航速机动时...     

Vertical TEC variations and model during low solar activity at a low latitude station,Xiamen

GPS-derived vertical TEC recorded at Xiamen (24.5°N, 118.1°E, geomagnetic latitude 13.2°N), China, during year 2006 is analyzed for the first time and compared to that predicted by ionosphere model SPIM recommend by ISO. A manifest seasonal anomaly is found with the high value during equinoctial season and low value during summer and winter season. Relative standard deviation for VTEC shows high value at around midnight and before sunrise. The correlation analysis exhibits that the variation of VTEC has a very weak relation with geomagnetic and solar activities (Dst, AP, SSN and F10.7). Comparative results reveal that the SPIM overestimates the observed VTEC at most of the time.     

IRI-2007预测TEC在广州地区的适用性分析

利用广州站(23.2°N, 113.3°E) GPS双频接收机监测的电离层TEC数据和IRI-2007模型不同电离层输入参数计算得到的TEC预测值, 对比分析了太阳活动低年(2008年)广州地区TEC的变化特征. 结果表明, TEC观测值周日变化在16:00LT左右达到最大值, 而IRI-TEC最大值出现时间较GPS-TEC提前1h左右. TEC季节变化在春秋分较高, 两至季节较低, 表现出明显的半年特性和季节依赖性, 并出现冬季异常现象. IRI-TEC与GPS-TEC在白天具有较好的一致性, 夜间偏差较大. 不同电离层输入参数得到的TEC预测值也相差较大, 选用顶部电子密度参数NeQuick、底部厚度参数B0 Table并用URSI系数计算F₂层峰值参数时, 能较好地反映TEC观测值的变化特征. 在对磁暴的响应上, 预测值无明显变化, 观测值则有比较明显的表现. 通过对比, 初步分析了利用IRI-2007模型预测TEC在广州地区的适用性, 并给出了合理的参数选择方案.