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A high-sensitivity laboratory system for measuring the microwave properties of gases under simulated conditions for planetary atmospheres

机译:一种高灵敏度实验室系统,用于在模拟条件下测量行星大气中气体的微波特性

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摘要

A system for measuring the microwave properties of gases under simulated conditions for planetary atmospheres has been under continuous development at Georgia Tech for over 2 decades (see, e.g., DeBoer and Steffes, 1996). The measurements from this system form the basis for accurately modeling the microwave properties of gases under various planetary conditions, which are essential in determining the presence and concentration of such gases through various microwave remote sensing techniques. This system consists of two independent configurations, one capable of measuring gas mixtures up to pressures of 3 bars at frequencies from 22 to 40 GHz, and another capable of pressures up to 12 bars over the frequency range from 1.5 to 24.1 GHz. The former configuration exhibits maximum 2-σ sensitivities in absorptivity of 0.25 dB/km and in refractivity of 2.0, while the latter configuration exhibits maximum 2-σ sensitivities in absorptivity ranging from 0.01 dB/km at 1.5 GHz (20 cm) to 1.0 dB/km at 24.1 GHz (1.25 cm) and in refractivity from 0.05 at 1.5 GHz to 3.13 at 24.1 GHz.
机译:佐治亚理工学院已经持续开发了一种在模拟大气条件下测量气体在大气中的微波特性的系统,该系统已有20多年的历史(例如,参见DeBoer和Steffes,1996)。该系统的测量结果构成了在各种行星条件下准确模拟气体微波特性的基础,这对于通过各种微波遥感技术确定此类气体的存在和浓度至关重要。该系统由两个独立的配置组成,一种能够在22至40 GHz的频率下测量高达3 bar压力的气体混合物,另一种能够在1.5到24.1 GHz的频率范围内测量高达12 bar的压力。前一种配置在0.25 dB / km的吸收率中表现出最大的2-σ灵敏度,在折射率2.0时表现出最大吸收率,从1.5 GHz(20 cm)到0.01 dB / km到1.0 dB的吸收率中表现出最大2-σ灵敏度。 / km在24.1 GHz(1.25 cm)时,折射率从1.5 GHz的0.05到24.1 GHz的3.13。

著录项

  • 来源
    《Radio Science 》 |2007年第6期| p.RS6010.1-RS6010.12| 共12页
  • 作者单位

    School of Electrical and Computer Engineering, Georgia Institute of Technology, 777 Atlantic Drive, Atlanta, GA 30332-0250, USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 无线电电子学、电信技术 ;
  • 关键词

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