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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Effects of sporadic E-layer characteristics on spread-F generation in the nighttime midlatitude ionosphere: A climatological study
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Effects of sporadic E-layer characteristics on spread-F generation in the nighttime midlatitude ionosphere: A climatological study

机译:散发e层特征对夜间中间电离层散布生成的影响:气候研究

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The aim of this study is to examine the effects of Es-layer characteristics on spread-F generation in the nighttime midlatitude ionosphere. The Es-layer parameters and spread-F appearance of the 23rd solar cycle (1996-2008) are recorded by the Kokubunji ionosonde. The Es-layer parameters are foEs (critical frequency of Es-layer), fbEs (blanketing frequency of Es-layer), and Delta f (equivalent to foEs-fbEs). In order to completely explore the effects, the pre-midnight and post-midnight data are classified by seasons, solar activities, and geomagnetic conditions. Results show that the spread-F occurs more frequently in post-midnight and in summer. And, the occurrence probabilities of spread-F are greater, when the solar activity is lower. For the occurrence probabilities of spread-F versus foEs and Delta f under geomagnetic quiet conditions, the trend is increasing, when the associated probabilities are significant. These indicate that the spread-F occurrence increases with increasing foEs and/or Delta f. Further, the increasing trends demonstrate that polarization electric fields generated in Es-layer would be helpful to generate spread-F, through the electrodynamical coupling of Es-layer and F-region. Moreover, this electrodynamical coupling is efficient not only under quiet-conditions but under disturbed conditions, since the significant increasing trend can also be found under disturbed-conditions. Regarding the occurrence probabilities of spread-Fversus fbEs, the evident trends are not in the majority. This implies that fbEs might not be a major factor for the spread-F formation.
机译:本研究的目的是研究ES层特征对夜间中间电离层中的展开F代的影响。 23RD太阳能循环(1996-2008)的ES层参数和扩展外观由Kokubunji Ionosonde记录。 ES层参数是FOES(ES层的临界频率),FBES(ES层的次次频率),以及DELTA F(相当于FOES-FBES)。为了完全探索效果,前午夜和午夜后的数据由季节,太阳能活动和地磁条件进行分类。结果表明,在午夜和夏季,普遍发生的频率更频繁地发生。并且,当太阳能活动较低时,散射F的发生概率更大。对于在地磁安静条件下扩散F与敌人和三角洲F的发生概率,当相关概率显着时,趋势正在增加。这些表明,扩散F发生随着敌人和/或三角洲F的增加而增加。此外,越来越多的趋势表明,在ES层中产生的偏振电场通过ES层和F区域的电动耦合来产生扩展F。此外,这种电动偶联不仅有效,不仅在安静条件下,而且在干扰条件下,由于在干扰条件下也可以发现显着的趋势。关于扩散FBE的发生概率,明显的趋势不是大多数。这意味着FBE可能不是扩散F形成的主要因素。

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