位于科钦(北纬 10.04°,东经 76.3°)的 CUSAT 205 MHz 平流层-对流层雷达的结构和后向散射特征 - 初步结果

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Radio Science Pub Date : 2024-06-01 DOI:10.1029/2023RS007894
Nabarun Poddar;Siddarth Shankar Das;Veenus Venugopal;S. Abhilash;V. Rakesh
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引用次数: 0

摘要

本文首次利用体积扫描对位于科钦热带站(北纬 10.04°,东经 76.3°)的 205 MHz 平流层-对流层(ST)雷达的面敏感特性进行了观测。最重要的新观测结果是,在某些高度区域,天顶波束和非天顶波束的信噪比几乎相等,表明存在各向同性湍流。信号强度在离天顶 0 至 10 度之间每度下降 0.75 分贝,在离天顶 10 至 20 度之间每度下降 0.9 分贝,在离天顶 20 度以上每度下降 0.3 分贝。根据与面高敏感度相关的各种估计参数,讨论了不同的成因机制。在 12 至 17 千米之间观测到了最大的面敏感性,这表明由于强风切变和大气稳定性而产生的动态不稳定性的存在。当风切变和稳定度参数的平方都高于 0.25 × 10-3 s-2 时,散射体大多成为各向同性。研究还显示了对称波束的功率差异以及方位角依赖性。分析表明,这种不对称是由于开尔文-赫尔姆霍兹不稳定性产生的大气重力波作用下的层倾斜造成的。目前的雷达配置可以让人们更好地了解湍流和不稳定性的三维结构。
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Structures and backscattering characteristics of CUSAT 205 MHz stratosphere-troposphere radar at Cochin (10.04°N, 76.3°E)—first results
This paper presents the first ever observations on aspect-sensitive characteristics of 205 MHz stratosphere-troposphere (ST) radar located at a tropical station Cochin (10.04°N, 76.3°E) using volume scanning. The most significant and new observation is that the signal-to-noise ratio in zenith and off-zenith beams are nearly equal in some height region, indicating the presence of isotropic turbulence. Signal strength decreases by 0.75 dB per degree from 0 to 10 degree off-zenith, 0.9 dB per degree from 10 to 20 degree off-zenith and 0.3 dB per degree beyond 20 degree off-zenith. Different causative mechanisms are discussed on the basis of various estimated parameters associated with aspect sensitivity. Maximum aspect sensitivity is observed between 12 and 17 km, indicating the presence of dynamic instability arising due to strong wind shear and atmospheric stability. When both the square of wind shear and stability parameters are above 0.25 × 10 −3 s −2 , the scatterers become mostly isotropic. The study also shows a power difference in the symmetric beams as well as azimuth angle dependency. Analysis suggests that this asymmetry is due to the tilting of layers by the action of atmospheric gravity waves generated through Kelvin-Helmholtz instability. The present configuration of radar can provide a better understanding of three-dimensional structures of turbulence and instabilities.
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来源期刊
Radio Science
Radio Science 工程技术-地球化学与地球物理
CiteScore
3.30
自引率
12.50%
发文量
112
审稿时长
1 months
期刊介绍: Radio Science (RDS) publishes original scientific contributions on radio-frequency electromagnetic-propagation and its applications. Contributions covering measurement, modelling, prediction and forecasting techniques pertinent to fields and waves - including antennas, signals and systems, the terrestrial and space environment and radio propagation problems in radio astronomy - are welcome. Contributions may address propagation through, interaction with, and remote sensing of structures, geophysical media, plasmas, and materials, as well as the application of radio frequency electromagnetic techniques to remote sensing of the Earth and other bodies in the solar system.
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