一种提高我国空间站中继测控覆盖率的方法

根据中继卫星的定点位置,对我国中继卫星-空间站的几何覆盖率进行了分析,并对提高空间站中继测控覆盖率的途径进行了研究,提出了一种采用不同舱段的2副中继天线融合使用,并通过调整天线安装布局提高中继测控覆盖率的方法。经理论分析和仿真验证,该方法能够有效地提高空间站中继测控覆盖率,可为我国空间站中继天线的安装布局设计提供参考。     

Features of the occurrence of the additional stratification on the bottom-side F region over the equatorial location of Trivandrum

The general features of occurrence of an additional layer on the bottom side of F region, referred to as F0.5 layer in the pre noon period, over the magnetic equatorial location of Trivandrum (8.5° N; 77° E; dip lat of 0.5° N) in India during the period from 2004 to 2007 are presented using ionosonde observations. The F0.5 layer has a June (northern summer) solsticial maximum probability of occurrence with secondary maxima during December (northern winter) solstice. The seasonal as well as the day-to-day variability in the occurrence of F0.5 layer as mentioned in this paper seems to be a result of the variations in the amplitude and phases of the tides and gravity waves, and inventory of the metallic ions of meteoric origin. This study brings out an important manifestation of morning time F layer base region dynamics.     

Stability of the seasonal variations in diurnal and semidiurnal components of mid-latitude F2 layer parameters

We report work utilizing 15-min resolution ionospheric data obtained with DPS-4 digisonde in 2003–2011 to study the seasonal variations in amplitudes and phases of the most powerful spectral components of the F2 layer critical frequency (foF2) and peak height (hmF2) fluctuations over Irkutsk (52.5°N, 104.0°E). We show that fluctuations of both parameters contain quasi-harmonic components with periods of T_n = 24/n h (n = 1–7). The number of distinct spectral peaks varies from 3 in summer to 7 in winter. Amplitude and phase characteristics of the diurnal (n = 1) and semidiurnal (n = 2) components is studied using the data sets extracted from the original data sets with band-pass filter. It has been found that the amplitudes of diurnal/semidiurnal foF2 and diurnal hmF2 components are maximum in winter and minimum in summer. Amplitudes of the diurnal components vary gradually; those of the foF2 semidiurnal one, abruptly, thus forming a narrow winter maximum in November–January. The phase (local time of maximum) of the diurnal foF2 component increases gradually by 4–6 h from winter to summer. The phase of the semidiurnal foF2 component is nearly stable in winter/summer and sharply decreases (increases) by 2–3 h near the spring (autumn) equinox. The phase of the diurnal component of hmF2 (local time of minimum) varies slightly between 1130 and 1300 LT; that of the semidiurnal one decreases (increases) by 4–6 h from January to March (from September to November). The results obtained show that the main features of seasonal variations in the diurnal and semidiurnal components of the mid-latitude F2 layer parameters recur consistently during the solar activity growth and decline phases.     

Investigation of ionospheric response to two moderate geomagnetic storms using GPS–TEC measurements in the South American and African sectors during the ascending phase of solar cycle 24

The responses of the ionospheric F region using GPS–TEC measurements during two moderate geomagnetic storms at equatorial, low-, and mid-latitude regions over the South American and African sectors in May 2010, during the ascending phase of solar cycle 24, are investigated. The first moderate geomagnetic storm studied reached a minimum Dst value of −64 nT at 1500 UT on 02 May 2010 and the second moderate geomagnetic storm reached a minimum Dst value of −85 nT at 1400 UT on 29 May 2010. In this paper, we present vertical total electron content (VTEC) and phase fluctuations (in TECU/min) from Global Positioning System (GPS) observations from the equatorial to mid-latitude regions in the South American and African sectors. Our results obtained during these two moderate geomagnetic storms from both sectors show significant positive ionospheric storms during daytime hours at the equatorial, low-, and mid-latitude regions during the main and recovery phases of the storms. The thermospheric wind circulation change towards the equator is a strong indicator that suggests an important mechanism is responsible for these positive phases at these regions. A pre-storm event that was observed in the African sector from low- to the mid-latitude regions on 01 May 2010 was absent in the South American sector. This study also showed that there was no generation or suppression of ionospheric irregularities by storm events. Therefore, knowledge about the suppression and generation of ionospheric irregularities during moderate geomagnetic storms is still unclear.     

船载测控设备远程测试标校系统设计与实现

远洋航天测控事业的不断发展,对测控设备的远程测试标校和故障诊断提出更高的要求。目前。船载测控设备配备了大量的智能测试仪器,为建立船载测控设备自动化测试标校系统提供了有利条件。此外基于PXI总线的虚拟仪器技术的广泛应用,也为未来航天测控设备的自动化测试提供了新途径。本文主要探讨了船载测控设备远程测试标校系统的主要设计思想和实现方式。     

卫星测控应用中心远程容灾系统方案设计

随着航天技术的发展,各种卫星如综合侦察卫星、气象与海洋监视卫星、数据与中继卫星等,其数据的信息速率存储、处理的数据量越来越大,对卫星测控应用中心大容量、高速率数据的安全性、可靠性要求也越来越高。在自然灾害,如地震、洪水;人为破坏,如恐怖活动、战争等条件下,确保卫星测控应用中心的安全与快速恢复能力,将非常重要。本文从原理上设计了一套远程数据容灾系统方案,以保证卫星测控应用中心在自然灾害或人为破坏后能够快速恢复其基本功能。分析表明,该方案具有很好的可靠性、安全性。     

单音干扰下扩频测控信号伪码跟踪性能研究

扩频测控信号的伪码跟踪性能直接关系到测控系统的测距精度。以伪码跟踪环中鉴相曲线平衡点的过零偏移为研究对象,推导了音频干扰条件下扩频测控信号伪码跟踪的干扰最大误差;并针对干扰最大误差需考虑具体鉴相算法的特点,提出基于相关曲线主瓣的二阶中心矩扩展因子的性能评价方法。该方法利用伪码相关曲线主瓣在干扰前后的畸变情况,反映干扰对伪码跟踪性能的影响。仿真分析表明,干扰最大误差的理论及仿真结果和二阶中心矩扩展因子所得结论一致,从而验证了干扰最大误差理论的正确性以及所提性能指标的有效性。     

基于多活性代理的多星测控调度方法

多星测控调度问题是一个具有多时间窗口、多资源约束的优化问题,其中多星测控任务调度的建模和求解算法是关键。在多活性代理理论的基础上,引入任务调度活性度概念及多活性代理活性保持的协调协商机制,建立基于活性度的多星测控调度模型,并给出一种多活性代理协调协商遗传算法。最后给出实验示例对所提出的算法进行仿真验证。仿真实验表明,所提出的基于多活性代理协商协调的模型及算法能够更好地解决多星测控任务调度问题。     

船载测控系统遥控小环误码分析与解决方案

针对某型船载测控系统中遥控设备存在遥控小环比对误码故障,在分析遥控小环接收解调机理基础上,通过模拟仿真和试验研究,建立了遥控副载波收发相位延迟与数据解调间的关系模型,提出了解决遥控小环设备误码问题的设计方案。试验结果表明,该方案对于解决船载测控系统中遥控小环比对误码问题是有效的、可靠的,降低了遥控指令小环比对错误的虚、漏概率,确保了遥控指令发送状态信息的实时监视。     

2007-2009谷年期间高热层大气密度的变化

在第23至第24太阳活动周的峰年之间,太阳活动谷年具有持续时间长,极低F_10.7太阳辐射通量（低至65）和超长期的零太阳黑子数记录等特点,因此是观测和研究在这种特殊背景下热层大气变化的极好机会.尤其是能充分理解和掌握在宁静环境下热层大气密度对弱太阳活动和小地磁扰动的响应特性.本文利用高度650 km以上星载大气密度探测器2007—2009年的连续探测数据进行分析,结果表明,在太阳辐射通量F_10.7极低值期间,较高热层大气密度对F_10.7的起伏具有更显著的响应变化.当F_10.7由70降至65时,日均大气密度会有4～5倍的显著降变,远大于通常大气模式中的降变值.同样在F_10.7极低值期间,较高热层大气密度对小地磁扰动也具有显著的响应增变,当日K_p指数之和由23增至30时,较高热层大气密度则会有80%～160%的强增变.