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作 者:欧阳新艳[1] 张学民[1] 申旭辉[1] 刘静[1] 钱家栋[1] 蔡晋安[1] 赵庶凡[1]
机构地区:[1]中国地震局地震预测研究所,中国北京100036
出 处:《地震学报》2008年第4期424-436,共13页Acta Seismologica Sinica
基 金:中国地震局地震预测研究所基本科研业务经费(0207690221);国家科技支撑项目联合资助
摘 要:挑选普洱地震前邻近地震震中的3条轨道的电子密度(Ne)数据,分析其1年内的所有重访轨道,并提取了这次地震前的Ne前兆异常.结果表明:①夜间电离层Ne存在明显的季节变化,4个季节呈现了各自不同的变化形态;②Ne的主要变化形态有3种,即单峰、马鞍和平缓状,这些形态在各个季节都可能出现,但每个季节有相对集中的形态;③Ne空间图象在震前30天内在震中区附近形成高值,异常信息在空间和时间上都与地震分布有很好的相关性,反映空间出现的异常信息确与本次地震有关;④Ne重访轨道曲线形态有一定的相似性,可以为识别判定地震异常提供背景信息.Selecting three half orbits near the epicenter of 2007 Ms6.4 Pu' er earthquake, we analyzed the No data recorded on their revisited orbit during a year before this earthquake, and extracted Ne precursors. The results show that: ①There are significant seasonal variations of ionospheric No in night time, with different varying style in the four seasons;②There are three main types of Ne variation: single-peak, saddle-shaped, even-shaped, all of which may occur in four seasons, but each season has its relatively typical variation style;③Spatial images of No showed high values near the epicenter for 30 days before the earthquake, and there is a good correlation between anomaly and distribution of earthquakes in space and time, implying that these spatial anomalies were indeed associated with the earthquake;④The Ne variation curves show a certain similarity among revisited orbit. This similarity may provide background information for distinguishing and identifying seismic anomaly.
关 键 词:普洱地震 DEMETER卫星 电子密度(Ne) 季节变化 地震异常
分 类 号:P318.63[天文地球—固体地球物理学]
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