Aspect sensitivity measurement of backscattering radar echoes from 205 MHz Stratosphere–Troposphere radar at a tropical coastal station

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Dhanya R. , Anju Pradeep , Rakesh V. , Abhilash S. , K. Mohankumar , Sivan C. , Rejoy Rebello , Prabhath H. Kurup
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Abstract

Aspect sensitivity in VHF radar refers to the extent to which the power and spectrum width of echoes vary with changes in the zenith angle, which is related to the backscattering process. The scattering of clear air signals is primarily caused by Fresnel reflection, anisotropic scattering, and isotropic scattering. The aspect sensitivity and accuracy of moment and wind estimation in clear air radars are influenced by the beam width, beam pointing angle from zenith, and atmospheric conditions. This study proposes a method to determine the sensitivity of the recently developed Stratosphere–Troposphere (ST) wind profile Radar in Cochin, India (10.04°N, 76.33°E). The radar operates at a distinct frequency of 205 MHz in the far VHF band. The experiment is conducted at an altitude of 5 to 20 km above the ground by adjusting the beam’s orientation with a resolution of 2°in both the east–west and north-south directions. The estimation of wind components is subject to uncertainty due to the varying aspect angles caused by the distinct dispersion properties in this height range. The study found that power variance is lowest between 6 and 12 km in both north-south and east–west directions, while daily fluctuations in aspect-sensitive echoes complicate wind component estimation. Correlation length (ζ) ranges from 0.5 to 15 m, indicating various air scattering processes. Notably, θs is smaller near the zenith and increases with tilt angles, exceeding 20°up to 14 km before declining at higher altitudes, indicating significant anisotropy at elevated levels. The wide range of R factor values (0.1 to 0.9) across different heights causes significant ambiguity in wind estimation. In this study, the impact of various aspect sensitivity parameters on wind estimation on days with clear air has been analyzed.
在热带海岸站测量 205 MHz 平流层-对流层雷达反向散射雷达回波的高宽比灵敏度
甚高频雷达的频谱灵敏度是指回波的功率和频谱宽度随天顶角变化而变化的程度,这与后向散射过程有关。晴空信号的散射主要由菲涅尔反射、各向异性散射和各向同性散射引起。晴空雷达的方位灵敏度和时刻及风估算精度受波束宽度、波束与天顶的指向角和大气条件的影响。本研究提出了一种方法来确定最近在印度科钦(北纬 10.04°,东经 76.33°)开发的平流层-对流层(ST)风廓线雷达的灵敏度。该雷达的工作频率为 205 兆赫,属于远甚高频波段。实验在离地面 5 至 20 千米的高度进行,通过调整波束的方向,东西和南北方向的分辨率均为 2°。在这一高度范围内,由于不同的频散特性造成了不同的纵横角,因此对风分量的估算存在不确定性。研究发现,南北向和东西向 6 至 12 千米范围内的功率方差最小,而纵横向敏感回波的日波动使风分量估算复杂化。相关长度(ζ)从 0.5 米到 15 米不等,表明存在各种空气散射过程。值得注意的是,θs 在天顶附近较小,并随倾斜角的增大而增大,在 14 千米以内超过 20°,然后在更高的高度下降,这表明在高空有明显的各向异性。不同高度的 R 因子值范围很广(0.1 至 0.9),导致风力估算非常模糊。在这项研究中,分析了各种高程灵敏度参数对晴朗天气风力估算的影响。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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