In this study, the relationship between the neutral components （N2 and 02） in the E-region of the ionosphere （at 110 km altitude） for the Singapore （01.23 N; 103.55 E） station in the equatorial region and the FI...In this study, the relationship between the neutral components （N2 and 02） in the E-region of the ionosphere （at 110 km altitude） for the Singapore （01.23 N; 103.55 E） station in the equatorial region and the FI0.7 solar flux and z-component of Interplanetary Magnetic Field （IMF-Bz） was investigated. This relationship was determined by means of statistical multiple regression model. As a result, it was observed that the changes in F10.7 solar flux and IMF-Bz were inversely proportional to the changes in N2 and 02. 92% and 83% of changes in N2 and O2 were found to be explained by F10.7 solar flux and IMF-Bz, respectively. When the F10.7 solar flux is changed by 1 s.f.u., it causes a decrease of 2.61×10TM m-3 in N2 and 2.96×1014 m-3 in O2. Change of I nT in IMF-Bz causes a decrease of 9.95× 1015 m-3 in N2 and 1.69× 1015 m-3 in O2.展开更多
基于224 MHz欧洲非相干散射甚高频雷达(European incoherent scatter very high frequency radar,EISCAT VHF radar)在2003—2014年间所观测的极区中层冬季回波(polar mesosphere winter echoes,PMWE)数据,分别从出现率、持续时间、高...基于224 MHz欧洲非相干散射甚高频雷达(European incoherent scatter very high frequency radar,EISCAT VHF radar)在2003—2014年间所观测的极区中层冬季回波(polar mesosphere winter echoes,PMWE)数据,分别从出现率、持续时间、高度分布、日变化、季节变化方面分析讨论了PMWE的平均时空特征,并对国际上PMWE与太阳和地磁活动的相关关系理论中存在的一些问题进行了讨论.结果表明:PMWE出现的几率非常低且持续时间普遍较短,其平均出现率为3.26%,每次出现的平均持续时间为67 min;高度分布范围主要在62~70 km,且在66~67 km高度范围内出现率最高;PMWE大多出现在白天,极少出现在夜晚,且11月份的出现率较高,12月份的出现率非常低.本文的研究为解释PMWE形成的物理机制提供了有价值的参考.展开更多
文摘In this study, the relationship between the neutral components （N2 and 02） in the E-region of the ionosphere （at 110 km altitude） for the Singapore （01.23 N; 103.55 E） station in the equatorial region and the FI0.7 solar flux and z-component of Interplanetary Magnetic Field （IMF-Bz） was investigated. This relationship was determined by means of statistical multiple regression model. As a result, it was observed that the changes in F10.7 solar flux and IMF-Bz were inversely proportional to the changes in N2 and 02. 92% and 83% of changes in N2 and O2 were found to be explained by F10.7 solar flux and IMF-Bz, respectively. When the F10.7 solar flux is changed by 1 s.f.u., it causes a decrease of 2.61×10TM m-3 in N2 and 2.96×1014 m-3 in O2. Change of I nT in IMF-Bz causes a decrease of 9.95× 1015 m-3 in N2 and 1.69× 1015 m-3 in O2.
