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.     

大功率无线电波与低电离层的相互作用

地面入射的大功率无线电波能加热电离层等离子体，引起电离层电子温度和密度的扰动，实现电离层的地面人工变态．本文中，着重考虑电波和电离层相互作用过程中的自吸收，构造一个自治的相互作用模型，在一定功率和频率的加热电波作用下，利用该模型计算了白天低电离层电子温度和由温度的变化而引起的电子密度的变化．计算结果表明，在白天低电离层，电波的自吸收在90km以下比较显著，而最大温度变化在70km高度上，大约增加了2倍．在α复合的假设下，电子密度变化幅度随高度的增加而减少，在70km处，大约增加55％、120km处则为4％左右．     

高频地波雷达抗短波通信干扰的研究

短波通信干扰包括短波通信瞬态干扰和短波通信长干扰两种。在对短波通信干扰的成因进行分析的基础上，利用特征子空间理论，提出了有效抑制短波通信干扰的方法。这种方法不仅能够消除短波通信瞬态干扰，而且对多个瞬态干扰同时存在所形成的长干扰的抑制也非常有效，这是一般抑制瞬态干扰的方法所达不到的。实测数据仿真结果表明了这种算法的有效性和实用性。     

Gravity wave propagation studies using the Indian MST radar observations

The Indian MST radar facility at Gadanki (13.5°N, 79.2°E) has been utilised to study the propagation of gravity waves from the troposphere/lower stratosphere to the mesosphere and their interaction with the radar backscattered signal variations. The main objective is to correlate vertically propagating gravity waves derived from the tropospheric velocity fields with the dynamics of mesospheric scattering centres. The tropospheric wind velocities and signal strengths over the entire height range have been subjected to power spectral and wavelet analysis to determine the predominant wave periods/amplitudes and the coupling between the lower atmosphere and mesosphere. Results show that (a) the gravity waves are clearly detectable near tropopause heights, (b) while relatively higher period gravity waves (20–50 min) interact with mesospheric scattering centres, the lower period waves (<20 min) are absorbed in the troposphere itself, (c) the mesospheric scattering layers are affected by gravity waves of complementary periods.     

短波信道下基于PSWF的非正弦时域正交信号调制解调实现

在对短波信道仿真模型进行了深入分析,并对非正弦时域正交信号的调制解调原理进行研究的基础上,利用Simulink软件对短波信道进行了仿真实现,构建了基于PSWF的非正弦时域正交信号的调制端和解调端。采用一种新的重构方法使小相对带宽PSWF脉冲的产生摆脱了Toeplitz矩阵求解的限制。在3~3.003 MHz频段内,实现了数据流的动态仿真。最后,给出了不同调制路数下的误码率曲线。