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Evolution of high latitude ionospheric convection associated with substorms: Multiple radar observations.

机译:与亚暴有关的高纬度电离层对流的演变:多次雷达观测。

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摘要

The work presented in this dissertation concerns evolution of the high latitude ionospheric convection and the relevant current systems associated with substorms, with emphasize on these features near the nightside Harang reversal region. Three different types of radars, including the Super Dual Auroral Radar Network (SuperDARN) coherent-scatter radars, the new advanced modular incoherent-scatter radar at Poker Flat (PFISR), and the Sondrestrom incoherent-scatter radar (ISR), have been utilized. Observations from those radars, together with those from complementary instruments, including satellites and other ground-based instruments, have revealed fundamental new understand of the ionospheric electrodynamic properties associated with substorms. By using the SuperDARN and the PFISR radars, we found that the auroral activity at substorm onset is located in the center of the Harang reversal, which represents a key region in the magnetospheric and ionospheric convection and is part of the Region 2 system. We have also shown that nightside convection flows exhibit repeatable, distinct variations at different locations relative to the substorm-related auroral activity. Taking advantage of the simultaneous flow and ionization measurements from PFISR, a current closure relation has been found between the Region 2 and the substorm field-aligned current systems. These observations demonstrate a strong coupling between the Region 2 system and the substorm dynamics. This study sheds new light on the substorm-related magnetosphere-ionosphere coupling and contributes to the building of a holistic picture of the substorm dynamics. The third radar has been used to study the dayside ionospheric convection response to the external soar wind and IMF driving and its role in substorm dynamics. The results have been applied to study substorm triggering and in the future could be used to study the relation between the external driving and the formation of the Harang reversal.
机译:本文提出的工作涉及高纬度电离层对流的演变以及与亚暴有关的相关当前系统,并着重强调了在夜间哈朗逆转区附近的这些特征。使用了三种不同类型的雷达,包括超级双极光雷达网络(SuperDARN)相干散射雷达,Poker Flat的新型先进模块化非相干散射雷达(PFISR)和Sondrestrom非相干散射雷达(ISR)。 。这些雷达以及互补仪器(包括卫星和其他地面仪器)的观测结果揭示了对与亚暴有关的电离层电动力性质的基本新认识。通过使用SuperDARN和PFISR雷达,我们发现亚暴爆发时的极光活动位于哈朗反转的中心,这是磁层和电离层对流的关键区域,是2区系统的一部分。我们还表明,相对于与亚暴有关的极光活动,在不同位置的夜间对流流动表现出可重复的,明显的变化。利用PFISR同时进行的流量和电离测量,发现了2区与亚暴场对准的电流系统之间的电流闭合关系。这些观察结果表明,2区系统与亚风暴动力之间存在强耦合。这项研究为与亚暴有关的磁层-电离层耦合提供了新的思路,并有助于建立亚暴动力学的整体图。第三个雷达已用于研究日间电离层对流对外部飙风和IMF驱动的响应及其在亚暴动力学中的作用。该结果已被用于研究亚暴的触发,将来可用于研究外部驱动与哈朗逆转形成之间的关系。

著录项

  • 作者

    Zou, Shasha.;

  • 作者单位

    University of California, Los Angeles.;

  • 授予单位 University of California, Los Angeles.;
  • 学科 Geophysics.;Atmospheric Sciences.
  • 学位 Ph.D.
  • 年度 2009
  • 页码 189 p.
  • 总页数 189
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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