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Comparative Study of the Geomagnetic Activity Effect on foF2 Variation as Defined by the Two Classification Methods at Dakar Station over Solar Cycle Phases

机译:太阳循环阶段两种分类方法定义了地磁活动对FOF2变异的比较研究

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This paper aims to establish a comparison between both geomagnetic activity classification methods on foF2 diurnal variation over solar cycle phases. It concerns first a comparison of geomagnetic activity occurrences according to both classification methods;and second the geomagnetic effect on foF2 diurnal variation profiles as defined for the equatorial latitudes. The occurrences of the different disturbed geomagnetic activities (recurrent activity (RA), shock activity (SA) and fluctuant activity (FA)) according to both classifications (ancient classification (AC) and new classification (NC)) have been studied at Dakar ionosonde station (Lat: 14.8°N;Long: 342.6°E). Regarding both classifications, the RA occurs more during the decreasing phase. And it’s observed that the RA occurs the most during the increasing phase for the AC and during the minimum phase for the NC. The maximum gap of occurrence () between both classifications is ᆟ.1% (for the negative value which is observed during the increasing phase) and +16.74% (for the positive one which is observed during the decreasing phase). The occurrence of the SA in relation with both classifications is the lowest during the minimum phase and the maximum occurrence is observed during the maximum and decreasing phases, for the AC, with a value close to 37% and for the NC at the maximum phase with a percentage of 54.47%. The maximum gap of occurrence () between both classifications is ᆥ.85% (for the negative value which is observed at maximum phase) and +13.53% (for the positive one which is observed during the decreasing phase). For both classifications, the FA occurs the least during the minimum phase and the most during the maximum phase for the AC and at maximum and decreasing phases with percentage values of occurrence of roughly 37% for the NC. The maximum gap of occurrence () between both classifications is ᆞ% (for the negative value which is observed during the decreasing phase) and +20.11% (for the positive one which is observed during the maximum phase). foF2 diurnal profiles throughout solar cycle phases concerning the AC and the NC have been compared. The FA diurnal profiles don’t present a difference. The RA and the SA present a difference during minimum and increasing phases and the least at maximum and decreasing phases.
机译:本文旨在建立对太阳循环阶段FOF2昼夜变异的地磁活动分类方法的比较。它涉及根据分类方法的热处理活动发生的比较;并第二对FOF2昼夜变化轮廓的几磁体效应,如赤道纬度所定义。根据分类(古代分类(AC)和新分类(NC)研究了根据分类的不同干扰的地磁活动(反复活性(RA),休克活动(SA)和波动活动(FA))已被研究过Dakar Ionosonde站(拉特:14.8°N;长:342.6°E)。关于这两个分类,RA在减少阶段时发生更多。并且观察到,在AC的增加期间和在NC的最小相期间,RA发生最大。两种分类之间的出现()的最大差距是&#4511.1%(对于在增加期间观察到的负值)和+ 16.74%(对于在降低阶段期间观察到的正面)。与两个分类相关的SA发生的是最小相位最低,并且在最大和减小的相位期间观察到的最大发生,其值接近37%,并且在最大相位下为NC的值百分比为54.47%。两种分类之间的出现()的最大间隙是&#4517.85%(在最大相位观察到的负值)和+ 13.53%(对于在降低阶段期间观察到的正面)。对于两个分类,FA在最小阶段期间发生至少在AC的最大阶段和最大阶段和最大和减少阶段,并且对于NC的发生百分比为大约37%。两种分类之间的出现()的最大间隙是&#4510%(对于在降低相期间观察到的阴性值)和+ 20.11%(对于在最大阶段期间观察到的正面)。比较了关于AC和NC的太阳循环阶段的FOF2昼夜曲线。 FA昼夜配置文件不存在差异。 RA和SA在最小和增加期间存在差异,并且最大和阶段的最小值最小。

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