Method of the HF wave absorption evaluation based on GIRO network data

High frequency (HF) communication is strongly dependent on the state of the ionosphere, which specifies the mode structure of the radio wave propagating in ionosphere. Another core factor defining the strength of the HF signal at the receiving site is the ionospheric absorption. Accurate modelling the effect of absorption is an essential part of many studies of the HF propagation in the ionosphere.This paper proposes a method for estimating the absorption. The method is based on analysis of vertical sounding ionograms. The main idea of the approach is to compare the main parameters retrieved from measured and simulated ionograms. The combination of Global Ionospheric Radio Observatory (GIRO, http://giro.uml.edu) data and ionograms modelling allows for developing the empiric absorption model available at near real-time. The ionogram simulation taking into account absorption utilizes the NIM-RT (North Ionospheric Model and Ray Tracing) software. As a result, the proposed technique provides more reliable and accurate evaluation of minimum frequency at which echoes are observed in vertical incidence ionosonde soundings. The values of these frequencies should be used in the following simulation to optimize parameters in the empirical formulae for defining absorption HF wave in ionosphere.The ultimate objective of this work is the designing the method, which allows the simulating of HF radio channel accounting for regular absorption due to UV radiation of the Sun. Eventually it could be considered as some kind of the HF propagation forecasting.     

光学材料亚表面损伤深度破坏性测量技术的实验研究

基于差动原理对HF酸恒定化学蚀刻速率法进行改进,以降低环境(温度、HF酸浓度等)变化对测量结果的影响,从而提高测量效率和测量准确性。并将在新方法测量实验后的结果与理论估计值进行了比较分析。     

短波返回探测最小时延曲线的反演

提出一个利用短波扫频返回探测最小时延导出电离层结构参数的方法。这个方法不必引入辅助参数,只需给出二个频率点的最小时延数据和相应的斜率数据,即可导出电离层参数。      

1984年4月份兰州地区电离层行波扰动的观测结果及初析

１９８４年４月份兰州地区电离层行波扰动的观测结果及初析张秀菊（中国电波传播研究所,新乡,４５３００３）关键词高频返回探测,多普勒频率,电离层行波扰动１９８４年４月我们利用高频返回探测系统在新乡一西北（反射点在兰州地区）电路上多次测到电离Ｆ层的行波扰动...     

基于扩频体制的短波时号发播新方案及可行性分析

短波授时系统采用扩频信号将有助于提高其授时服务质量。顾及到短波信道的复杂性和系统带宽的有限性,本文提出了一种基于两个扩频信号之间的相对发播时间间隔实现短波时号发播的新方案,并对其可行性进行了分析。阐述了所提方案的基本技术思路,并通过理论分析与比较,验证了所提方案相比于常规方案能够显著降低接收机的时号检测错误概率,可更好地实现协调世界时UTC和世界时UT1两种短波时号的兼容发播,为基于扩频体制的短波时号调制技术的进一步研究提供一种有效途径。     

L波段有源冷噪声源研究

本文介绍了有源冷噪声源的应用背景及发展现状。根据微波场效应晶体管常温下输出稳定低噪声的特性,以Avago公司的两种典型pHEMT晶体管为核心器件进行了ADS仿真设计,研制出两款有源冷噪声源。给出了对设计的两款器件的技术指标进行验证的L波段周期定标辐射计设计框图。仿真结果表明,以pHEMT型晶体管为核心器件设计成的L波段有源冷噪声源能输出稳定低噪声。     

GJB5000 A与DO-178 B／C的综合应用研究

针对软件研制单位目前存在的型号软件研制必须同时满足GJB5000 A与适航软件研制标准的要求,通过对GJB5000 A与DO-178 B／C的对比分析,提出一种将GJB5000 A与DO-178 B／C相互融合的方法,并对方法实际工程实践时应注意的问题进行了说明。     

短波地空通信多普勒频移对DTMF信号解码影响

DTMF信号具有优良的抗干扰性能和一定的抗多普勒频移的能力,广泛应用于语音信道的低速数据通信。文中分析了地-空短波通信的多普勒频移、基于Goertzel算法的DTMF信号解码基本原理和基本过程;在语音噪声背景下,基于Goertzel算法,解算了16个频点的信号幅值,对地—空短波通信的多普勒频移对DTMF信号解码性能的影响进行了仿真,得出了在语音和多普勒频移干扰的背景下,信噪比高于9dB时,基本可实现DTMF信号的高可靠检测的结论。     

波音737飞机垂尾高频天线前缘风蚀的预防与修理

波音737飞机垂直尾翼前缘高频天线风蚀是该机型日常维护中的常见故障,本文分析了风蚀的预防以及修理的原理和方法,通过安装聚亚安酯防风蚀膜和喷涂FP-200防风蚀涂层,可有效避免飞机AOG停场,减少运行维护成本以及保障高频天线的通信正常。     

HF wave activity in the low and middle-altitude polar cusp

We reported the results of our investigations of wave activity in high-frequency range performed on board CLUSTER spacecraft in the middle-altitude cusp region, around 5 R_E during August and September 2002. Our analysis was mainly based on the registration gathered by the WHISPER instrument (Waves of HIgh frequency and Sounder for Probing of Electron density by Relaxation). For a better understanding of the processes of wave-particle interaction and in order to understand the general plasma conditions in the cusp region, we also included in our analysis the data registered by the STAFF (Spatio-Temporal Analysis of Field Fluctuation experiment) instrument and the CIS (Ion Spectrometry experiment) instrument. These observations were carried out during different geomagnetic activity; under quiet conditions and during magnetic storm period. The space plasma is characterised by the ratio of plasma frequency to electron gyrofrequency, in this case, the local plasma frequency was, mainly, a little greater than the electron plasma, but it was also frequently observed that these two characteristic frequencies were not very different from one another. The whistler waves, electron-cyclotron waves, electron-acoustic waves and Langmuir waves have been detected when the spacecraft was crossing the middle-altitude cusp region. We suggested that the majority of those waves were generated by electron beams. For a better understanding the plasma conditions in the low and middle-altitude cusp region the past FREJA wave data results are used to describe typical wave activity detected in the low-altitude cusp region. The aim of this paper is to discuss, on the basis of a few chosen representative examples, the property of typical high wave activity detected in the lower part of cusp region.