60- 1分钟积分时间转换模型的建立及机器学习在热带位置时间序列衰减预测中的应用

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
M.A. Sodunke , J.S. Ojo , F.A. Semire , Y.B. Lawal , O.L. Ojo , G.A. Owolabi , A.I. Olateju
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引用次数: 0

摘要

对1分钟积分时间的本地测量降雨率数据的需求持续增长,因为它在估计降雨引起的衰减方面是准确的。然而,由于购置、维护和测量设备的高成本,当地天文台气象站的短缺导致在大多数地点采用卫星数据。星载雷达覆盖范围广,但分辨率较低,积分时间较高,需要转换为积分时间较低的雷达。本文利用一种新开发的转换模型,将热带降雨测量任务(TRMM)获得的10年(2005-2014)雨率卫星数据从默认的60分钟转换为1分钟的积分时间。研究地点是位于尼日利亚西南部的Akure、Ikole-Ekiti、Ogbomosho和Oshogbo。利用整合时间为1 min的2年(2009-2010年)地面实测雨率数据对所建立的模型进行了验证。与其他模型相比,所建立的60- 1分钟积分时间模型的性能得到了改善,R2为0.92,预测误差为5.8%,均方根误差为5.79%,最小p值为0.005,具有统计学显著性,表明反对原假设的最强证据。将转换后的1 min降雨率数据应用于合成风暴技术(Synthetic Storm technology, SST)降雨衰减模型,生成时间序列雨致衰减。研究区域的互补累积分布函数(CCDF)描述了在0.01%的时间内大于10 dB的衰减值,这可能会威胁到无线电波的传播。通过测试三种预测模型,即SARIMA、ARIMA和SVM,利用机器学习应用了一种预测时间序列衰减的新技术。SVM的R2、MAE、RMSE优于其他模型,置信区间分别为0.89、1.64%、2.14%和[2.4544、5.9273]。研究结果将适用于5G和6G系统的高频移动网络,以及微波点对点等地面通信链路。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Development of 60-min to 1-min integration time conversion model and application of machine learning for time-series attenuation prediction in tropical location
The demand for locally measured rain rate data with 1-min integration time continues to grow due to its accuracy in estimating rain-induced attenuation. However, the scarcity of local observatory weather stations due to the acquisition, maintenance, and the high cost of measuring equipment have resulted in the adoption of satellite data in most locations. Satellite-borne radars provide wide coverage but have low resolutions with higher integration time, hence the need for conversion to lower integration time. In this work, ten years (2005–2014) of rain rate satellite data obtained from the Tropical Rainfall Measuring Mission (TRMM) have been converted from the default 60 min to 1 min of integration time using a newly developed conversion model. The research locations are Akure, Ikole-Ekiti, Ogbomosho, and Oshogbo, located in the southwestern part of Nigeria. The developed model was validated using ground-based measured two years (2009–2010) rain rate data of 1 min integration time. The performance of the developed 60-min to 1-min integration time model when compared with other models showed an improvement with a good R2 of 0.92, a lower prediction error of 5.8 %, a root mean square error of 5.79 %, and a statistically significant smallest p-value of 0.005, indicating the strongest evidence against the null hypothesis. The converted 1-min rainfall rate data was applied to the Synthetic Storm Technique (SST) rain-attenuation model to generate time series rain-induced attenuation. The complimentary cumulative distribution function (CCDF) of the study areas depicted attenuation values greater than 10 dB at 0.01 percent of the time, which could be threatening to radio wave propagation. A further novel technique of predicting time series attenuation was applied by testing three forecasting models, namely SARIMA, ARIMA, and SVM, using machine learning. The SVM outperformed other models with a better R2, MAE, RMSE, and confidence intervals of 0.89, 1.64 %, 2.14 %, and [2.4544, 5.9273], respectively. The results will be found applicable to mobile networks at 5G and 6G systems operating at high frequencies, as well as terrestrial communication links like microwave point-to-point.
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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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