ID 原文 译文
13154 利用2007-2013年的COSMIC掩星数据，分析了E区与F区电离层闪烁的变化特征。 Based on the COSMIC (constellation observing system for meteorology, ionosphere and ciimate) GPS occultation data from 2007 to 2013, the characteristics of ionospheric scintlllation in E and F regions are analyzed.
13155 发现用闪烁出现频次、闪烁发生率以及闪烁强度来表征的电离层闪烁出现规律比较相似。 It is found that the variations of ionospheric scintlllation characterized by its frequency, occurrence or intensity are qute similar.
13156 E区电离层闪烁在夏季半球的中纬地区最强,其次是春秋季的低纬地区和冬季半球。 Ionospherc scintillation in E region is the strongesi in mid-lattudes of summer hemsphere, followed by thai in low lattudes in equmox and wmter hemsphere.
13157 就经度分布来说，春秋季E区电离层闪烁呈 四波结构。 The longtudmal variation of ionospheric scin- tlllaton in E-region presents a four-wave structure in equinox.
13158 对F区电离层闪烁来说：南美-大西洋扇区在12月至点最为显著；非洲和太平洋扇区在6月至点 最为显著；大西洋扇区在春秋分季最为显著。 The ionospheric scintlllation in F region is strongest in South American-Atlantic sector in December solstice, in African and Pacific sector in June solstice and in Atlanta sector in equinox.
13159 极区也出现中等强度的闪烁，尤其在南半球的90°E〜180°E扇区较为显著。 The polar region has a weak contribution to the global ionospheric scintlllation, manly from the 90°E—180°E sector.
13160 高纬E区电离层闪烁强度随太阳活动的增强而增强，而低纬和南半球的中纬E区闪烁随太阳活动的增强而减弱。 The intensity of ionospheric scintillation in region increases wi th solar activities in high latitudes, but decreases in mid-latitude in southern hemisphere and low latitudes.
13161 高纬和低纬F区闪烁随太阳活动的增强而增强，而中纬F区电离层闪烁对太阳活动无显著依赖关系。 The intensity of ionospheric scintillation in F region increases with solar activities in both high and low latitudes, with no significant trends in mid-latitudes.
13162 对于赤道区来说，北半球60°W$60°E经度区闪烁强度随太阳活动的变化最为显著，其次是南半球60°E~210°E附近； In low latitudes, the 60°W—60°E longitude in northern hemsphere has the most sensitive scintlllation effects caused by solar activities, followed by the 60°E—210°E longitude in southern hemsphere.
13163 而对于高纬地区来说!F区闪烁强度随太阳活动的变化最为显著的区域在南半球 60°E〜210E附近・ In high latitudes, the 60°E —210°E longitude in southern hemsphere has the most sensitive scintillation effects caused by solar activities.