“火星快车”的三程多普勒观测

利用中国VLBI网无线电天线和数字信号采集系统跟踪测量了欧洲航天局的＂火星快车＂（MEX）探测器,并研发了相应的三程多普勒信号提取算法和软件。对探测器8.4GHz下行载波1s采样的最终结果显示,多普勒数据随机噪声为1mm/s,这些数据已成功应用于对火星探测器的轨道确定。     

Metric radio bursts and fine structures observed on 17 January, 2005

A complex radio event was observed on January 17, 2005 with the radio-spectrograph ARTEMIS-IV, operating at Thermopylae, Greece; it was associated with an X3.8 SXR flare and two fast Halo CMEs in close succession. We present dynamic spectra of this event; the high time resolution (1/100 s) of the data in the 450–270 MHz range, makes possible the detection and analysis of the fine structure which this major radio event exhibits. The fine structure was found to match, almost, the comprehensive Ondrejov Catalogue which it refers to the spectral range 0.8–2 GHz, yet seems to produce similar fine structure with the metric range.     

高升阻比乘波体外形设计及气动特性计算研究

采用数值模拟方法研究在设计点(马赫数6,迎角0°)锥导乘波体气动外形的设计方法及其基本气动特性,以及在非设计点时该乘波体的气动特性,即各个气动系数随迎角和马赫数的变化特性.研究表明:基于无粘锥形流的乘波体气动外形的反设计方法是成功的;在设计点附近选取合适的半基准圆锥激波角并考虑粘性影响时,可得到乘波体最大升阻比为3.36;给出了采用这一布局的单级入轨运载器的可行的飞行控制方案;分析提出了进一步提高该乘波体气动布局升阻比的有效途径.      

无线定位扩展卡尔曼滤波算法的优化

设计了一种蜂窝系统无线定位中使用的扩展卡尔曼滤波(EKF)算法,对其性能进行了仿真. 通过仿真结果分析,寻找出算法优化方法. 优化方法综合了到达时间(TOA)信号测量方差和雅可比矩阵计算出预测误差,然后对算法估计出的用户位置进行修正. 仿真结果显示,优化后定位估计性能比优化前的算法性能有显著改善.      

空间环境对无线电波传播的影响综述

文章研究了空间环境对无线电通信的影响,主要体现在多种因素制约下的等离子体环境对电波传播的影响。首先介绍了几种典型的电离层模型,接着详细讲述了工程实用电离层模型;随后给出了电磁波在等离子体环境中的传播路径和等离子体介质在磁场环境下对电磁波影响的定量分析,并建议将空间等离子体环境（包括星际等离子体环境和电离层等离子体环境等）作为一个整体进行研究,来考虑地磁场对等离子体电磁特性的影响;最后基于目前理论的不足与实际需求的矛盾,探讨未来的研究方向。     

A study on radio-loud interacting/non-interacting CMEs-associated SEPs and solar flares

We have established a data set of 58 major hybrid SEP events associated with meter-to-decahectometer wavelength (m-to-DH) type II bursts, solar flares, and radio-load CMEs during the period of 1997–2014. The main focus of our study is to address the following two questions: Does the interaction of CMEs play a role in the enhancement of SEP intensity? Is there any difference in the seed population, and parent eruptions in the SEP events with and without CME interactions? Hence, the sample of 58 events is classified into two sets: (i) 35 non-interacting-CME-associated SEP events; (ii) 23 interacting-CME-associated SEP events. All the characteristics of SEPs, their associated CMEs/flares and the relationships between them are statistically analyzed and compared. Some of the basic attributes and relative elemental abundances (Fe/O ratios) of the both the sets are also compared. The results indicate that the seed particles in non-interacting-CME-associated SEP events are mostly from solar wind/coronal materials. But in the case of interacting-CME-associated SEP events, it may be associated with both flare material from preceding flares and coronal materials from solar wind/preceding CMEs. The correlation studies reveal that there are clear correlations between logarithmic peak intensity of SEP events and properties of CMEs (space speed: cc?=?0.56) and solar flares (peak intensity: cc?=?0.40; integrated flux: cc?=?0.52) for non-interacting-CME-associated SEP events. But these correlations are absent for the interacting-CME-associated events. In addition, the results suggest that interaction of primary CMEs with their preceding CMEs plays an important role in the enhancement of peak intensity of SEPs at least for a set of m-to-DH type II bursts associated SEP events.     

Estimated errors in a global gravity wave climatology from GPS radio occultation temperature profiles

In a previous paper by Schmidt et al. (2008), from CHAllenging Minisatellite Payload (CHAMP) Global Positioning System (GPS) radio occultation data, a comparison was made between a Gaussian filter applied to the “complete” temperature profile and to its “separate” tropospheric and stratospheric height intervals, for gravity wave analyses. It was found that the separate filtering method considerably reduces a wave activity artificial enhancement near the tropopause, presumably due to the isolation process of the wave component. We now propose a simple approach to estimate the uncertainty in the calculation of the mean specific wave potential energy content, due exclusively to the filtering process of vertical temperature profiles, independently of the experimental origin of the data. The approach is developed through a statistical simulation, built up from the superposition of synthetic wave perturbations. These are adjusted by a recent gravity wave (GW) climatology and temperature profiles from reanalyses. A systematic overestimation of the mean specific wave potential energy content is detected and its variability with latitude, altitude, season and averaging height interval is highlighted.     

Observations of HF propagation on a path aligned along the mid-latitude trough

Observations of the direction of arrival and time of flight of HF signals propagating on a 1400 km path oriented along the mid-latitude trough are presented. At night, the signal commonly arrives from directions offset from the great circle bearing by up to 80° and these events have been categorised into five main types. Statistics indicating how often these categories of propagation were observed in the period August 2006 to September 2007 are presented. The physical mechanisms which result in the off great circle propagation are also discussed.     

复合材料电搭接分析

电搭接是指用金属编织线或金属片将机载设备的外壳与飞机基本结构连接起来,使两者处于一个共同的电位点。飞机上采用复合材料后,由于复合材料与金属之间电性能的差异,在GJB358-87中规定的搭接电阻值就不完全适用。本文在研究了大量国内外资料的基础上,根据国内目前的技术水平,对安装在复合材料结构上的机载设备,按不同的电搭接功能要求,提出了合适的搭接电阻值。     

Length scales for September 14, 2005 solar noise storm

Source length scales are estimated for the September 14, 2005 solar noise storm from the spectral and temporal observed characteristics of the background continuum fluctuations and clusters of Type I bursts. The characteristic height of the magnetic structure where the noise storm source is located and the size of the source where Type I bursts clustering takes place were calculated. A lower limit for the height of the magnetic structure supporting the noise storm at 237 MHz was estimated too.