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作 者:张红波[1] 盛冬生[1] 刘玉梅[1] 孙树计[1] 徐彤[1]
机构地区:[1]中国电波传播研究所电波环境特性及模化技术重点实验室,青岛266107
出 处:《空间科学学报》2016年第2期167-174,共8页Chinese Journal of Space Science
摘 要:基于中国海口站(20.00°N,110.33°E)获取的2013全年UHF频段电离层闪烁信号强度数据,利用Welch算法,分析给出了四类典型电离层闪烁强度功率谱.利用功率谱时序图分析方法,发现电离层不均匀体存在东西向水平周期性变化结构.提取全年功率谱指数p,通过统计分析发现谱指数p存在规律变化,据此建立一个谱指数经验模型,该谱指数模型已用于中国低纬区域电离层闪烁发生预报概率模型(CMSOP),进而对海口站UHF频段电离层闪烁发生概率观测数据和预报结果进行了对比分析.The amplitude data of UHF-band ionospheric scintillations were recorded at a lowlatitude station of China,Haikou station(geographic:20.00°N,110.33°E),during the high sunspot activity year of 2013.Based on these data,the Welch algorithm of the Fast Fourier Transform methods was used to analyze the scintillation intensity power spectra,and four types of typical intensity power spectra were found and presented.A nearly sinusoidal fluctuation in the east-west horizontal direction was found in the irregularity structure by analyzing the contour map of spectral density as a function of local time and spatial scale.The spectral index p of the ionospheric amplitude scintillations was extracted for the year of 2013,and the variation of the spectral index p was analyzed by statistical method and an empirical model of the spectral index p over Haikou station was put forward,which was applied in the empirical Climatological Model of Scintillation Occurrence Probability(CMSOP) over the low-latitude of China.Finally the prediction of ionospheric scintillation occurrence over Haikou station from CMSOP is compared with the observations.
关 键 词:电离层闪烁 不均匀体 谱指数模型 CMSOP模型 概率预报
分 类 号:P352[天文地球—空间物理学]
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