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A Comparison of Polarization Jet Characteristics at the Greatly Separated Stations Yakutsk and Podkamennaya Tunguska

机译:雅库茨克和波德卡门纳亚通古斯卡两座极端分离的台站的偏振射流特性比较

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摘要

Characteristics of the polarization jet (PJ) are considered on the basis of measurements made in 1989-1992 at the ionospheric stations Yakutsk (L = 3.0, λ = 129.6°) and Podkamennaya Tunguska (L = 3.0, λ = 90.0°) separated in longitude. Using the data of these stations, the result obtained earlier (that the formation of PJ during disturbances in the near-midnight sector occurs at the expansion phase of a substorm) is confirmed. At isolated magnetic disturbances with AE > 500 nT in the 11:00-16:00 UT interval, the PJ band covers an MLT sector of 3 h between the Yakutsk and Podkamennaya Tunguska stations. The time of the PJ beginning at the Podkamennaya Tunguska station for the majority of events is 45-60 min behind the PJ beginning at the Yakutsk station. This corresponds to the westward motion of a PJ source with a velocity of ~3 MLT h per hour.
机译:根据1989-1992年在雅库茨克(L = 3.0,λ= 129.6°)和Podkamennaya Tunguska(L = 3.0,λ= 90.0°)分离的电离层台站的测量结果来考虑极化射流(PJ)的特性。经度。使用这些台站的数据,可以确认较早获得的结果(在近午夜区域扰动期间PJ的形成发生在亚暴的扩张阶段)。在UT间隔11:00-16:00,在AE> 500 nT的孤立磁干扰下,PJ频带覆盖了雅库茨克站和Podkamennaya Tunguska站之间3 h的MLT扇区。在大多数事件中,PJ在Podkamennaya Tunguska站开始的时间比在Yakutsk站开始的PJ落后45-60分钟。这对应于PJ源的向西运动,速度约为每小时3 MLT h。

著录项

  • 来源
    《Cosmic research》 |2008年第2期|114-119|共6页
  • 作者单位

    Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences, pr. Lenina 31, Yakutsk. 677980 Russia;

    Space Research Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, GSP-7, Moscow, 117810 Russia;

    Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences, pr. Lenina 31, Yakutsk. 677980 Russia;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    ionospheric disturbances and modifications;

    机译:电离层扰动和修正;

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