调频广播主要在甚高频(Very High Frequency,VHF)频段传输。VHF频段具有传播距离远、穿透力强、信号稳定等优势,但易受多种因素影响。基于此,首先介绍VHF频段的基本特点和调频广播信号的技术参数,其次介绍VHF频段调频广播信号传播的测...调频广播主要在甚高频(Very High Frequency,VHF)频段传输。VHF频段具有传播距离远、穿透力强、信号稳定等优势,但易受多种因素影响。基于此,首先介绍VHF频段的基本特点和调频广播信号的技术参数,其次介绍VHF频段调频广播信号传播的测量过程,最后从天线的设计和布置、调制、编码技术的应用等方面,提出改善VHF频段调频广播覆盖效果的策略。展开更多
在超短波通信系统中,经常要求天线具有宽频带与耐受大功率的特性。通过理论上的定性分析,设计了一种对称振子天线。天线阻抗匹配采用套筒式结构、与空气带状线平衡器结构一体设计。根据仿真计算结果,制作了1副天线。测试结果表明,该天线...在超短波通信系统中,经常要求天线具有宽频带与耐受大功率的特性。通过理论上的定性分析,设计了一种对称振子天线。天线阻抗匹配采用套筒式结构、与空气带状线平衡器结构一体设计。根据仿真计算结果,制作了1副天线。测试结果表明,该天线在VHF频段20%带宽内驻波比小于1.3,可以承受5 k W连续波功率要求。该匹配技术也被证明可以用于其他TEM模馈电结构的天线设计。展开更多
Data obtained from the mobile SOUSY VHF radar at And(ya/Norway in summer 1987 have been used to study the nonlinear interactions between planetary waves, tides and gravity waves in the polar mesosphere, and the instab...Data obtained from the mobile SOUSY VHF radar at And(ya/Norway in summer 1987 have been used to study the nonlinear interactions between planetary waves, tides and gravity waves in the polar mesosphere, and the instability of background atmosphere above the mesopause. It is observed that 35-h planetary wave, diurnal, semidiurnal and terdiurnal tides are the prominent perturbations in the Lomb-Scargle spectra of the zonal wind component. By inspecting the frequency combinations, several triads are identified. By bispectral analysis it is shown that most bispectral peaks stand for quadratic coupling between tidal harmonics or between tide and planetary or gravity wave, and the height dependence of bispectral peaks reflects the variation of wave-wave interactions. Above the mesopause, the occurrence heights of the maximum L-S power spectral peaks corresponding to the prominent wave components tend to increase with their frequencies. This may result from the process in which two low frequency waves interact to generate a high frequency wave. Intensities of the planetary wave and tides increase gradually, arrive at their maxima, and then decay quickly in turn with increasing height. This kind of scene correlates with a 'chain' of wave-wave resonant interactions that shifts with height from lower frequency segment to higher frequency segment. By instability analysis, it is observed that above the mesopause, the Richardson number becomes smaller and smaller with height, implying that the turbulent motion grows stronger and stronger and accordingly the background atmosphere more and more instable. It is suggested that the wave-wave sum resonant interaction and the wave dissipation due to instability are two dominant dynamical processes that occur in the mesopause region. The former invokes the energy transfer from lower frequency waves to higher frequency waves. The latter results in the heating of the atmosphere and accelerating of the background flow.展开更多
文摘调频广播主要在甚高频(Very High Frequency,VHF)频段传输。VHF频段具有传播距离远、穿透力强、信号稳定等优势,但易受多种因素影响。基于此,首先介绍VHF频段的基本特点和调频广播信号的技术参数,其次介绍VHF频段调频广播信号传播的测量过程,最后从天线的设计和布置、调制、编码技术的应用等方面,提出改善VHF频段调频广播覆盖效果的策略。
文摘在超短波通信系统中,经常要求天线具有宽频带与耐受大功率的特性。通过理论上的定性分析,设计了一种对称振子天线。天线阻抗匹配采用套筒式结构、与空气带状线平衡器结构一体设计。根据仿真计算结果,制作了1副天线。测试结果表明,该天线在VHF频段20%带宽内驻波比小于1.3,可以承受5 k W连续波功率要求。该匹配技术也被证明可以用于其他TEM模馈电结构的天线设计。
基金the National Natural Science Foundation of China under grant 49625407 and grant 49990450
文摘Data obtained from the mobile SOUSY VHF radar at And(ya/Norway in summer 1987 have been used to study the nonlinear interactions between planetary waves, tides and gravity waves in the polar mesosphere, and the instability of background atmosphere above the mesopause. It is observed that 35-h planetary wave, diurnal, semidiurnal and terdiurnal tides are the prominent perturbations in the Lomb-Scargle spectra of the zonal wind component. By inspecting the frequency combinations, several triads are identified. By bispectral analysis it is shown that most bispectral peaks stand for quadratic coupling between tidal harmonics or between tide and planetary or gravity wave, and the height dependence of bispectral peaks reflects the variation of wave-wave interactions. Above the mesopause, the occurrence heights of the maximum L-S power spectral peaks corresponding to the prominent wave components tend to increase with their frequencies. This may result from the process in which two low frequency waves interact to generate a high frequency wave. Intensities of the planetary wave and tides increase gradually, arrive at their maxima, and then decay quickly in turn with increasing height. This kind of scene correlates with a 'chain' of wave-wave resonant interactions that shifts with height from lower frequency segment to higher frequency segment. By instability analysis, it is observed that above the mesopause, the Richardson number becomes smaller and smaller with height, implying that the turbulent motion grows stronger and stronger and accordingly the background atmosphere more and more instable. It is suggested that the wave-wave sum resonant interaction and the wave dissipation due to instability are two dominant dynamical processes that occur in the mesopause region. The former invokes the energy transfer from lower frequency waves to higher frequency waves. The latter results in the heating of the atmosphere and accelerating of the background flow.
