AERONOMIC RADIO SPECTROMETRY WITH CALIBRATION BY SIGNALS FROM VIRTUAL SOURCES

Q4 Physics and Astronomy Radio Physics and Radio Astronomy Pub Date : 2022-01-01 DOI:10.15407/rpra27.03.219
A. Korolev, Y. Karelin, O. Antyufeyev, V. Shulga, V. Myshenko, D. Chechotkin, D. Shulga, O. Patoka, K. Marynko
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Abstract

Subject and Purpose. The work has been aimed at developing and implementing a novel method of aeronomic observations in the Earth's stratosphere, applicable in the microwave range of the electromagnetic spectrum. The research is centered on a study of the measurement errors arising when the method proposed is employed for observations of the ozone spectral line (142 GHz). Methods and Methodology. The method is based on a simplified calibration procedure, in what concerns the hardware and the technology employed. In contrast to the common calibration techniques using special-purpose sources of the reference signal, we suggest resorting to natural sources, like internal noise of the receiver and the thermal radiation from the Earth's surface and the lower atmospheric layer. The measurement errors (both calculated and evaluated experimentally) have been analyzed within standard mathematical statistics techniques. Results. The tests performed during observations of the spectral line (142 GHz) of atmospheric ozone allow considering the new method as a success. The estimated magnitude of the relative error specific to the observation method proposed does not exceed 1.5%. The experimental estimate accounting for all potential error sources does not exceed 5% (with a 1 hour accumulation period), which result corresponds to the current state of the art. Conclusions. The possibility of an essential simplification of the radio optical part of the spectrometer has been demonstrated. The novel calibration technique, as well as the technical implementation thereof, can be recommended as a basis for prospective spectrometers at microwave frequencies.
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航空无线电光谱与校准的信号从虚拟源
主题和目的。这项工作的目的是发展和实施一种在地球平流层进行航空观测的新方法,适用于电磁波谱的微波范围。本文主要研究了采用该方法对臭氧谱线(142 GHz)进行观测时产生的测量误差。方法和方法论。该方法基于简化的校准程序,涉及硬件和所采用的技术。与使用专用参考信号源的常见校准技术不同,我们建议使用自然信号源,如接收机的内部噪声和来自地球表面和低层大气的热辐射。测量误差(计算和实验评估)已经在标准数理统计技术中进行了分析。结果。在观测大气臭氧谱线(142 GHz)期间进行的试验可以认为新方法是成功的。所提出的观测方法的相对误差估计幅度不超过1.5%。考虑所有潜在误差源的实验估计不超过5%(积累周期为1小时),符合目前的技术水平。结论。证明了对光谱仪的射电光学部分进行基本简化的可能性。这种新的校准技术及其技术实现,可以作为未来微波频率光谱仪的基础。
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来源期刊
Radio Physics and Radio Astronomy
Radio Physics and Radio Astronomy Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
0.60
自引率
0.00%
发文量
18
审稿时长
8 weeks
期刊最新文献
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