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首页> 外文期刊>Advances in space research >Variability of the bottomside B0 and B1 parameters of ionospheric electron density profile over Cyprus and comparison with IRI-2012 model
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Variability of the bottomside B0 and B1 parameters of ionospheric electron density profile over Cyprus and comparison with IRI-2012 model

机译:塞浦路斯电离层电子密度分布的底面B0和B1参数的变异性以及与IRI-2012模型的比较

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摘要

The bottomside profile thickness (B0) and shape (B1) parameters are investigated for the first time over a lower mid-latitude European digisonde station in Nicosia, Cyprus (Station id. NI135; Geographic 35°N, 33°E), with a set of manually scaled ionograms during the period 2009-2014. We performed a comparative analysis of the digisonde observed B0 and B1 parameters with the predictions of International Reference Ionosphere (IRI-2012), using all bottomside modeling options, during different seasons under low and high solar activity conditions. Observations show significant day-to-day variations in their magnitudes manifesting relatively higher B0 (lower B1) from summer to lower B0 (higher B1) in winter, through the moderate B0 and B1 values during the equinox, the degree of which further depend on the level of solar activity. Considerable discrepancy in the model predictions are noticed with (a) Bil-2000 demonstrating almost no diurnal variability in B0 though the B1 is estimated appreciably, (b) Gul-1987 following the observed diurnal pattern of B0 to manifesting the characteristic pre-sunrise enhancement in spite of its relatively higher magnitudes with its constant B1 replaced by the B1 from Bil-2000 option, and (c) ABT-2009 overestimating observed B0 in all seasons except summer and the estimated B1 following a quasi-similar diurnal pattern to that of observed B1, but with relatively flattened slope of the curves in their diurnal plots in all seasons. It is evident from the present analysis that none of the options in the present version of IRI shows adequate agreement with observed B0 and B1 parameters over Cyprus, which in turn necessitates the inclusion of these datasets in IRI model for better lower mid-latitude predictions. The important extracts from this study may support the international efforts for a comprehensive global climatological representation of the IRI model.
机译:在塞浦路斯尼科西亚的较低中纬度欧洲digisonde台站(台站编号NI135;地理35°N,33°E)下,对底面剖面厚度(B0)和形状(B1)参数进行了首次调查。在2009-2014年期间设置的一组手动缩放的电离图。我们使用所有底部模型选项,在低太阳活动条件和高太阳活动条件下的不同季节中,使用国际参考电离层的预测对洋地黄观测到的B0和B1参数进行了比较分析。观测结果显示,幅度的显着日常变化表明,通过春分期间的中等B0和B1值,夏季到夏季的B0相对较高(B1较低)到冬季的B0较低(B1较高),其程度进一步取决于太阳活动的水平。在模型预测中存在相当大的差异,其中(a)Bil-2000证明了B0几乎没有昼夜变化,尽管对B1的估计是相当大的;(b)Gul-1987遵循观察到的B0的昼夜模式来表现出特征的日出前增强尽管其相对较高的幅度,其常数B1被Bil-2000期权的B1取代,并且(c)ABT-2009高估了除夏季以外的所有季节观测到的B0,并且估计的B1遵循与昼夜模式近似的昼夜模式观察到B1,但在所有季节的日间图中曲线的斜率相对平坦。从目前的分析中可以明显看出,当前版本的IRI中没有任何选项与塞浦路斯的观测到的B0和B1参数显示出足够的一致性,这又有必要将这些数据集包含在IRI模型中,以便更好地进行中低纬度预测。这项研究的重要摘录可能会支持国际上为IRI模式的全球气候综合表示所做的努力。

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