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Polar cusp, plasma mantle particles and their relationships to polar rain

机译:极地尖端,等离子体地幔粒子及其与极地雨的关系

摘要

On the basis of low altitude DMSP satellite particle data, characteristics of polar rain, cusp and plasma mantle are examined during the asymmetric polar rain enhancement period. Obtained results are summarized as follows : (1) From the comparison between number flux of cusp and polar rain precipitations, the cusp flux does not increase correlatively with the increasing of polar rain flux. This result suggests that sources of precipitating particles are quite different from each other. (2) Low energy pulsive electrons (plasma mantle) are occasionally observed in the polar rain region. These plasma mantle particles are observed in both hemispheres and the polar rain enhancement shows hemispheric asymmetry. The mixing of polar rain and plasma mantle may be occurred due to the movement of plasma mantle by electric field drift.
机译:根据低空DMSP卫星颗粒数据,在非对称极雨增强期,研究了极雨,尖顶和等离​​子地幔的特征。得到的结果概括如下:(1)从尖峰雨量和极雨降水的通量比较来看,尖峰雨量与极雨通量的增加并没有相关性。该结果表明,沉淀颗粒的来源彼此完全不同。 (2)在极地雨区偶尔观察到低能脉冲电子(等离子地幔)。在两个半球都观察到了这些等离子地幔颗粒,并且极地降雨增强显示出半球不对称。由于电场漂移引起的等离子体罩的运动,可能会导致极性雨和等离子体罩的混合。

著录项

  • 作者

    MakitaKazuo; AyukawaMasaru;

  • 作者单位
  • 年度 1996
  • 总页数
  • 原文格式 PDF
  • 正文语种 ja
  • 中图分类

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