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典型大气窗口太赫兹波传输特性和信道分析
引用本文:王玉文,董志伟,李瀚宇,周逊,罗振飞. 典型大气窗口太赫兹波传输特性和信道分析[J]. 物理学报, 2016, 65(13): 134101-134101. DOI: 10.7498/aps.65.134101
作者姓名:王玉文  董志伟  李瀚宇  周逊  罗振飞
作者单位:1. 中国工程物理研究院 研究生院, 北京 100088;2. 北京应用物理与计算数学研究所, 北京 100094;3. 中国工程物理研究院太赫兹研究中心, 绵阳 621900;4. 中国工程物理研究院激光聚变研究中心, 绵阳 621900
基金项目:中国工程物理研究院太赫兹中心(批准号: T2014-06-0209)资助的课题.
摘    要:在已有大气传输模型的基础上,发展了新的太赫兹波大气传输衰减与色散模型,对宽频太赫兹波在真实大气中传输的衰减和色散特性进行了数值模拟研究.改进太赫兹时域光谱技术,对0.3—2.0 THz频段太赫兹波的大气传输特性进行了透射光谱测量,并得到了一组连续吸收参数.比对发现实验窗口区强度和吸收峰的位置都与计算结果符合得很好.据此选取了三个可行的信道:340,410和667 GHz窗口区,利用线性色散理论和无线通信原理分别从物理上精确地计算了这些信道的群速色散参数和信道容量,并分析了影响最大传输数据率的因素-天线增益.研究结果表明:太赫兹波大气传输1 km时,这三个信道群速色散很小,信号不易被展宽;最大传输速率达十几Gbps,高于单模光纤,但需要更高的天线增益.

关 键 词:大气传输  太赫兹时域光谱技术  色散  信道容量
收稿时间:2016-01-21

Atmospheric window characteristic and channel capacity of THz wave propagation
Wang Yu-Wen,Dong Zhi-Wei,Li Han-Yu,Zhou Xun,Luo Zhen-Fei. Atmospheric window characteristic and channel capacity of THz wave propagation[J]. Acta Physica Sinica, 2016, 65(13): 134101-134101. DOI: 10.7498/aps.65.134101
Authors:Wang Yu-Wen  Dong Zhi-Wei  Li Han-Yu  Zhou Xun  Luo Zhen-Fei
Affiliation:1. Graduate School of Chinese Academy of Engineering Physics, Beijing 100088, China;2. Institute of Applied Physics and Computational Mathematics, Beijing 100094, China;3. Terahertz Research Center, Chinese Academy of Engineering Physics, Mianyang 621900, China;4. Research Center of Laser Fusion, Chinese Academy of Engineering Physics, Mianyang 621900, China
Abstract:The increasing demand of unoccupied and unregulated bandwidth for wireless communication systems will inevitably lead to the extension of operation frequencies toward the lower THz frequency range. Since atmospheric transmission windows exist in the lower THz frequency range, it can be realized that carrier frequencies of 300 GHz and beyond will be used for communications once the technology for high bitrate data transmission is available. However, the free-space path-loss and the attenuation due to molecules in the atmosphere can significantly reduce the transmittable data rate in the lower THz frequency range.The main factor affecting the behavior of terahertz band is the absorption by water vapor, which not only attenuates the transmitted signal, but also disperses the signal. A new model of the terahertz wave atmospheric propagation of attenuation and dispersion is developed by using the radiation transmission theory and the empirical continuum absorption based on the HITRAN database. Theoretical aspects of absorption are presented, emphasizing those that deserve special attention as frequency increases. The THz wave atmospheric attenuation experimental results and self- and foreign-continuum coefficients obtained with the improved THz-time domain spectroscopy (THz-TDS) technique are analyzed by this model. The intensities and locations of the observed absorption lines are in good agreement with spectral databases. This model accounts for the group velocity dispersion and the total path loss that a wave in the THz band suffers when propagating 1 km distance. The channel capacity of the THz band is investigated by this model under different conditions including antenna gains, channel bandwidth and transmitter power. In order to keep the considerations as general as possible, the derivations are based on simple assumptions and equations. The special requirement for antenna is also discussed.Three communication channels (340 GHz, 410 GHz and 667 GHz) are obtained in terms of the spectrum. The four parameters of the three channels, i.e., available bandwidth, center frequency, dispersion and transmittable data rate, are summarized and quantized. The signals through the atmosphere for the three communication channels within the corresponding atmospheric windows are not easy to broaden due to the low group velocity dispersion; high data rates of up to 10 Gbps or beyond per 1 GHz bandwidth can be transmitted via these channels if the antennas with high gains are used.
Keywords:atmospheric propagation  terahertz time-domain spectroscopy  dispersion  channel capacity
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