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首页> 外文期刊>Annales Geophysicae >Day-to-day thermosphere parameter variation as deduced from Millstone Hill incoherent scatter radar observations during March 16-22, 1990 magnetic storm period
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Day-to-day thermosphere parameter variation as deduced from Millstone Hill incoherent scatter radar observations during March 16-22, 1990 magnetic storm period

机译:从1990年3月16日至22日磁暴期间的Millstone Hill非相干散射雷达观测结果推导出的日常热层参数变化

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摘要

A self-consistent method for day-timeF2-region modelling was applied to the analysis of Millstone Hill incoherentscatter observations during the storm period of March 16-22, 1990. The methodallows us to calculate in a self-consistent way neutral composition, temperatureand meridional wind as well as the ionized species height distribution.Theoretically calculated Ne(h) profiles fit the observeddaytime ones with great accuracy in the whole range of heights above 150 km forboth quiet and disturbed days. The overall increase in Tex by270 K from March 16 to March 22 reflects the increase of solar activity levelduring the period in question. A 30% decrease in [O] and a two-fold increase in[N2] are calculated for the disturbed day of March 22 relativeto quiet time prestorm conditions. Only a small reaction to the firstgeomagnetic disturbance on March 18 and the initial phase of the second storm onMarch 20 was found in [O] and [N2] variations. The meridionalneutral wind inferred from plasma vertical drift clearly demonstrates thedependence on the geomagnetic activity level being more equatorward on disturbeddays. Small positive F2-layer storm effects on March 18 and 20 are totallyattributed to the decrease in the northward neutral wind but not to changes inneutral composition. A moderate (by a factor of 1.5) O/N2ratio decrease relative to the MSIS-83 model prediction is required to describethe observed NmF2 decrease on the most disturbed day of March22, but virtually no change of this ratio is needed for March 21.
机译:在1990年3月16日至22日的暴风雨期间对Millstone Hill非相干散射观测值进行分析时,采用了一种自洽的白天F2区域建模方法。该方法使我们能够以自洽的方式计算中性成分,温度和子午线理论上计算出的 N e (h)剖面在白天都非常安静,在150 km以上的整个高度范围内都非常安静和不安的日子。从3月16日到3月22日, T ex 整体增加了270 K,反映了在此期间太阳活动水平的增加。相对于安静时间的暴风雨前天气,3月22日的干扰天[O]降低30%,[ N 2 ]增长两倍。在[O]和[ N 2 ]变化中,仅发现对3月18日的第一次地磁扰动和3月20日的第二次风暴的初始反应很小。由等离子垂直漂移推断出的子午线中性风清楚地表明,在干扰日,对地磁活动水平的依赖性更加赤道。 3月18日和20日的F2层小正风暴效应完全归因于向北的中性风的减少,而不是中性成分的变化。相对于MSIS-83模型预测,O / N 2 比率的中度(降低1.5倍)需要描述观察到的 N m F 2在最受干扰的3月22日减少,但实际上3月21日不需要更改此比率。

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