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Characteristics of the large-scale traveling atmospheric disturbances during geomagnetically quiet and disturbed periods simulated by a whole atmosphere general circulation model

机译:大气整体环流模式模拟的地磁静寂和扰动期间大规模旅行大气扰动的特征

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We have investigated characteristics of the large-scale traveling atmospheric disturbances (LS-TADs) generated during geomagnetically quiet and disturbed periods using a whole atmosphere general circulation model (GCM). The GCM simulations show that various TADs appear in association with passages of regions with large temperature gradients near the solar terminator, midnight temperature anomaly, and auroral oval which move with the Earth's rotation. These TADs, which are superimposed on each other, appear even when a geomagnetically quiet period. The TADs generated during a geomagnetically quiet period show structures extending in the longitudinal direction at high-latitude and in the latitudinal direction at mid- and low-latitude. These structures disappear after their short-range propagations. The TADs generated during a geomagnetically disturbed period show structures extending widely in the longitudinal direction and propagate from high- to low-latitude. These simulation results suggest the different generation mechanisms and features between the TADs generated during geomagnetically quiet and disturbed periods.
机译:我们使用整体大气总环流模型(GCM)研究了在地磁安静和扰动期间产生的大规模旅行大气扰动(LS-TAD)的特征。 GCM模拟显示,各种TAD伴随着太阳终结者附近具有大温度梯度的区域,午夜温度异常和极光椭圆随着地球自转而移动时出现。这些TAD相互叠加,即使在地磁静默期也出现。在地磁静默期产生的TAD显示出在高纬度时沿纵向延伸而在中纬度时沿纬度延伸的结构。这些结构在短距离传播后消失。在地磁干扰期间产生的TAD显示出在纵向上广泛分布并从高纬度传播到低纬度的结构。这些模拟结果表明,在地磁静默和受干扰时期产生的TAD之间存在不同的生成机制和特征。

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