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Morphology of pre-noon and post-noon auroras

机译:中午前和中午后极光的形态学

摘要

General characteristics of dayside auroras for quiet and disturbed conditions are examined on the basis of Greenland and Spitzbergen TV data. It is our new finding that characteristics of dayside auroras are quite different between the pre- and post-noon sectors. Namely, corona auroras are seen in the pre-noon sector and band auroras are seen in the post-noon sector. During the quiet period, corona auroras are observed at magnetic latitudes higher than 75° in the pre-noon sector. In the post-noon sector, no remarkable auroras are seen around 75° MLAT. On the other hand, during the disturbed period, corona auroras are observed at latitudes lower than 80° MLAT in the pre-noon sector. Periodic bright band auroras appear in the post-noon sector. The comparison between these auroras and particle precipitation is also examined and the source region of dayside auroras is discussed.
机译:根据格陵兰和Spitzbergen电视数据,研究了安静和干扰条件下的日间极光的一般特征。我们的新发现是,午前和午后之间日间极光的特征完全不同。即,在正午之前可以看到电晕极光,在午后之后可以看到带状极光。在安静时期,在中午之前在高于75°的磁纬度上观测到电晕极光。在午后时段,在MLAT 75°附近没有发现明显的极光。另一方面,在扰动期间,在中午之前在低于80°MLAT的纬度观测到电晕极光。午后时段出现周期性的亮带极光。还检查了这些极光和颗粒降水之间的比较,并讨论了日间极光的来源区域。

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