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Modeling attenuation and phase of radio waves in air at frequencies below 1000 GHz

机译:低于1000 GHz频率的空气中无线电波的衰减和相位建模

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Moist air is characterized for the frequency range 1–1000 GHz as a nonturbulent propagation medium described by meteorological parameters. An adequate spectroscopic data base for air consists of three terms: (1) resonance information for 29 H2O lines up to 1097 GHz and 44 O2 lines up to 834 GHz in the form of intensity coefficients and center frequency for each line; (2) an empirical water vapor continuum spectrum; and (3) a liquid water attenuation term for haze and cloud conditions. This data base is the heart of two computer programs which calculate and plot attenuation rates (in decibels per kilometer), refractivity (in parts per million), and refractive dispersion (in parts per million). The first covers the troposphere and requires pressure, temperature, and relative humidity as input data. The second addresses isolated line behavior in the mesosphere wherein the geomagnetic field strength H is an additional input parameter due to the Zeeman effect of the O2 molecules. Each oxygen line splits proportionally with H into numerous sublines, which are juxtaposed to form Zeeman patterns spread over a megahertz scale. Patterns of three main polarization cases are considered. Various typical examples for a model atmosphere demonstrate the utility of the approach, provide new information, and underline the serious role that water vapor plays above 120 GHz.
机译:作为气象参数描述的非湍流传播介质,潮湿空气的特征是在1–1000 GHz的频率范围内。足够的空气光谱数据库包括三个术语:(1)以每条线的强度系数和中心频率的形式显示最高1097 GHz的29条H2O线和最高834 GHz的44条O2线的共振信息; (2)经验水蒸气连续谱; (3)雾霾条件下的液态水衰减术语。该数据库是两个计算机程序的核心,它们可以计算和绘制衰减率(以每公里分贝为单位),折射率(以百万分之几为单位)和折射色散(以百万分之几为单位)。第一个覆盖对流层,需要压力,温度和相对湿度作为输入数据。第二种方法解决了介球中的孤立线行为,其中由于O2分子的塞曼效应,地磁场强度H是附加的输入参数。每条氧气线都与H成比例地分成许多子线,这些子线并列形成在兆赫兹尺度上分布的Zeeman模式。考虑了三种主要极化情况的模式。模型大气的各种典型示例证明了该方法的实用性,提供了新的信息,并强调了水蒸气在120 GHz以上发挥的重要作用。

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