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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Daytime additional F layer stratification over low-midlatitude station of the Indian sector under geomagnetic disturbed conditions
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Daytime additional F layer stratification over low-midlatitude station of the Indian sector under geomagnetic disturbed conditions

机译:白天额外F层分层low-midlatitude站印度部门在地磁扰动的条件下

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In this paper, the observations of additional F layer stratification are presented in a region which is situated at the outer edge of equatorial ionization anomaly (EIA) zone. The digital ionosonde data observed over Delhi(28.6° N, 77.2° E, dip 42.44° N)during March-April, 2001 has been used to carry out the present work. The observational period was geomagnetically disturbed and represents the high solar activity phase of 23rd solar cycle. The additional transient cusp is frequently observed in the considered months before the noon hours; however, in this paper only five prominent cases are presented. From the analysis of ionograms, it is observed that the transient additional cusp is formed between the pre-existing F_1 and F_2 layer; hence, named as the cusp of F_1.5. Study reveals that the Traveling Atmospheric Disturbances(TADs)along with the vertical expansion of F layer provides the necessary condition for the existence of this transient feature. The intensification of F_1 layer along with increased altitude immediately after the disappearance of additional stratification remains one of the fascinating features of the present results. The present investigation demonstrates that the daytime F_1 and F_2 region over low-midlatitude station is strongly modulated by the passage of TIDs, originating at high latitudes or by atmospheric disturbances of local origin during the high solar activity period. The concurrent presence of TADs and the associated disturbance composition appears to be plausible reason behind the present observations.
机译:本文观察更多的F层分层呈现在一个地区这是位于赤道的外缘吗电离(EIA)异常区。ionosonde数据观察到德里(28.6°N, 77.2°在3 E,下降42.44°N), 2001用来进行目前的工作。观察期间是眼睛打扰,代表了较高的太阳活动23日,太阳活动周期的阶段。瞬态尖端经常被观察到的认为是前几个月的中午时间;在本文中只有五个突出的病例提出了。观察到临时额外的尖端预先存在的f和f₂之间形成的层;揭示了旅游大气随着垂直扰动(TADs)F层提供了必要的扩张这个瞬态存在的条件特性。增加高度后立即额外的分层的消失仍然是一个迷人的特征现在的结果。表明,白天f和f₂地区在强烈low-midlatitude站调制通道的tid,原始高纬度地区的大气扰动当地的起源在高的太阳活动时期。似乎干扰成分有关似是而非的原因目前的观测。

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