考虑颗粒湿度和电荷的灰霾事件中厘米波衰减预测经验模型

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-07-11 DOI:10.1016/j.jastp.2024.106296
Tian-Li Bo , Xiao-Hua Yang , Zhi-Mei Huang
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引用次数: 0

摘要

为了确保雾霾天气下无线通信和雷达设备的运行,有必要研究雾霾天气下电磁波衰减系数(α)的定量预测。尺寸分析结果表明,颗粒湿度(Hp)和颗粒电荷质量比(Qm)是影响电磁波传播的两个重要参数。在微观层面,通过核壳结构将这两个参数的影响引入电磁波衰减模型。结果表明,Hp 和 Qm 会增加 α。由于微尺度模型中的物理参数很难通过实验方法获得。因此,本文分析了 Zhang 等人(2020b)的实验数据,发现α的变化可以通过 Hp 来缩放,而 Qm 主要影响α随 Hp 线性变化的斜率项。根据这些发现,提出了一个考虑到 Hp 和 Qm 的 α 经验模型。结果表明,在高湿度的灰霾天气中,Hp 和 Qm 的影响不容忽视。而且,相对湿度对 α 的影响最大,颗粒物充注对 α 的影响次之,颗粒物的一次释放对 α 的影响最小。该模型的优点是不仅形式简单、易于应用,而且所需的输入和模型参数可以通过实验方法测量。
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An empirical model for prediction of centimeter wave attenuation during haze event considering particle humidity and charge

In order to ensure the operation of wireless communication and radar equipment during haze events, it is necessary to study the quantitative prediction of the attenuation coefficient of Electromagnetic wave (α) during haze events. The results of the dimensional analysis show that particle humidity (Hp) and particle charge-to-mass ratio (Qm) are two important parameters that affect the propagation of electromagnetic waves. At the micro level, the influence of two parameters is introduced into the electromagnetic wave attenuation model through the core-shell structure. The results show that the Hp and Qm will increasing α. Due to it being difficult to obtain the physical parameters in the micro-scale model by experimental methods. Therefore, this article analyzes the experimental data of Zhang et al. (2020b) and finds out that the change of α can be scaled by Hp, and Qm mainly affects the slope term of the linear change of α with Hp. Based on these findings, an empirical model of α considering Hp and Qm was proposed. The results show that the influence of Hp and Qm during haze events with high humidity cannot be ignored. And, the relative humidity has the largest contribution to α, the particle charging has the second place, and the primary release of particulate matter has the smallest contribution. The advantage of this model is that it is not only simple in form and easy to apply, but also that the input required and model parameters can be measured with experimental methods.

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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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