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引用次数: 15

摘要

根据最常见的定义,“极帽”是指以平均或统计极光椭圆为界的区域。综述了行星际磁场对各种高层大气现象影响的研究。南极地区和北极地区是进行这种调查的一个地区。本文特别注意在高纬度地区的观测,这些观测提供了有关磁层内部结构相应变化的一些信息。本文考虑了极帽的定义和工作定义以及国际货币基金组织和磁层模型、太阳高能电子的进入、关于极光的统计研究、个别事件、极帽弧、极光尖峰、极光电子降水、对流、电离层电流和场向电流、电离层、热层、极雨、极风和重离子的跳跃运动。
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The polar caps
According to the most common definition, the 'polar cap' is the region bounded by the average or statistical auroral oval. Studies of the effects of the interplanetary magnetic field (IMF) on various upper atmospheric phenomena are reviewed. The Antarctic region and the Arctic region represent an area for such investigations. Particular attention is given in this paper to those observations in the highest latitude region which provide some information concerning corresponding changes of the internal structure of the magnetosphere. A definition and working definition of the polar cap are considered along with the IMF and magnetospheric models, the entry of solar energetic electrons, statistical studies regarding the aurora, individual events, polar cap arcs, the cusp aurora, auroral electron precipitation, convection, ionospheric currents and field-aligned currents, the ionosphere, the thermosphere, polar rain, polar wind, and hopping motions of heavy ions.
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Polar vortex meandering and stratospheric aerosol distribution: Lidar measurements at Fairbanks, Alaska (scientific paper) The polar caps A Special Ozone Observation at Syowa Station, Antarctica from February 1982 to January 1983 Interlinking of physical and biological processes in the Antarctic Ocean (abstract) Precambrian of the African Continent
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