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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >FORMOSAT-3/COSMIC observations of seasonal and longitudinalvariations of equatorial ionization anomaly and its interhemisphericasymmetry during the solar minimum period
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FORMOSAT-3/COSMIC observations of seasonal and longitudinalvariations of equatorial ionization anomaly and its interhemisphericasymmetry during the solar minimum period

机译:FORMOSAT-3 / COSMIC观测太阳最短期间赤道电离异常的季节和纵向变化及其半球不对称性

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Using an extremely valuable global data set from Formosa Satellite (FORMOSAT-3)/Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC)radio occultation experiment, a comprehensive study has been carried out on the seasonaland longitudinal variations of equatorial ionization anomaly (EIA) and the temporalvariation in the hemispheric asymmetry of EIA during the low solar activity period fromNovember 2006 to October 2007. The interesting result observed from this investigation isthe local-time-dependent variation in the hemispheric asymmetry of EIA. During thesolstices, it has been consistently observed that the EIA crest in the winter hemisphereappears stronger than that in the summer hemisphere during morning to noon hours. Incontrast to this, during noon to early afternoon hours, the ionization in the winter EIAcrest decreases rapidly, and the crest in the summer hemisphere becomes more intensifiedthan that in the winter hemisphere. Further, this transition of stronger EIA crest fromwinter hemisphere to summer hemisphere occurs around 1200-1300 LT during theDecember solstice months and is delayed by a couple of hours (seen around -4400 LT)during June solstice months. The causative neutral and electrodynamical mechanisms arediscussed in light of relative contributions from the field-aligned plasma transport dueto transequatorial interhemispheric neutral wind, the strength of the equatorial fountainprocess, and the ion drag effects during different local times and seasons. The results fromthe Sami2 is Another Model of the Ionosphere (SAMI2) model simulation also exhibitsimilar local-time-dependent variation in the hemispheric asymmetry of EIA, whichfurther supports our argument. Also, it was observed that the large magnetic declination ofthe field lines and the four-peaked longitudinal structure of EIA can significantly modulatethe interhemispheric asymmetry of EIA even during the equinoxes.
机译:利用福尔摩沙卫星(FORMOSAT-3)/气象,电离层和气候星座观测系统(COSMIC)的无线电掩星实验的极有价值的全球数据集,对赤道电离异常的季节性和纵向变化进行了全面研究( EIA)和2006年11月至2007年10月低太阳活动期间EIA的半球不对称性随时间的变化。从这项调查中观察到的有趣结果是EIA的半球不对称性随时间的变化。在冬至期间,一直观察到,在早晨至中午,冬季半球的EIA波峰比夏季半球的EIA波峰强。与此相反,从中午到下午早些时候,冬季EIAcrest的电离迅速降低,夏季半球的波峰比冬季半球的波峰更强烈。此外,EIA波峰从冬季半球到夏季半球的这种转变发生在冬至的1200-1300 LT左右,而在冬至的几个月则延迟了几个小时(在-4400 LT附近)。讨论了引起中性和电动力学的机制,这是由于跨赤道半球间中性风引起的场定向等离子体传输的相对贡献,赤道喷泉过程的强度以及在不同的本地时间和季节所产生的离子阻力效应。 Sami2的结果是“电离层的另一个模型”(SAMI2),模型仿真也显示了类似的局部时间依赖的EIA半球不对称性变化,这进一步支持了我们的观点。而且,观察到即使在春分期间,磁力线的大磁偏角和EIA的四峰纵向结构也可以显着调节EIA的半球不对称性。

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