中大機構典藏-NCU Institutional Repository-提供博碩士論文、考古題、期刊論文、研究計畫等下載:Item 987654321/50383
English  |  正體中文  |  简体中文  |  全文笔数/总笔数 : 78818/78818 (100%)
造访人次 : 34717369      在线人数 : 936
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
搜寻范围 查询小技巧:
  • 您可在西文检索词汇前后加上"双引号",以获取较精准的检索结果
  • 若欲以作者姓名搜寻,建议至进阶搜寻限定作者字段,可获得较完整数据
  • 进阶搜寻


    jsp.display-item.identifier=請使用永久網址來引用或連結此文件: http://ir.lib.ncu.edu.tw/handle/987654321/50383


    题名: Magnetopause expansions for quasi-radial interplanetary magnetic field: THEMIS and Geotail observations
    作者: Suvorova,AV;Shue,JH;Dmitriev,AV;Sibeck,DG;McFadden,JP;Hasegawa,H;Ackerson,K;Jelinek,K;Safrankova,J;Nemecek,Z
    贡献者: 太空科學研究所
    关键词: UPSTREAM PRESSURE VARIATIONS;SOLAR-WIND CONDITIONS;BOW SHOCK;MAGNETOSHEATH;PLASMA;MAGNETOSPHERE;PARALLEL;FORESHOCK;MOTION;FLOW
    日期: 2010
    上传时间: 2012-03-27 17:30:33 (UTC+8)
    出版者: 國立中央大學
    摘要: We report Time History of Events and Macroscale Interactions during Substorms (THEMIS) and Geotail observations of prolonged magnetopause (MP) expansions during long-lasting intervals of quasi-radial interplanetary magnetic field (IMF) and nearly constant solar wind dynamic pressure. The expansions were global: The magnetopause was located more than 3 R(E) and similar to 7 R(E) outside its nominal dayside and magnetotail locations, respectively. The expanded states persisted several hours, just as long as the quasi-radial IMF conditions, indicating steady state situations. For an observed solar wind pressure of similar to 1.1-1.3 nPa, the new equilibrium subsolar MP position lay at similar to 14.5 R(E), far beyond its expected location. The equilibrium position was affected by geomagnetic activity. The magnetopause expansions result from significant decreases in the total pressure of the high-beta magnetosheath, which we term the low-pressure magnetosheath (LPM) mode. A prominent LPM mode was observed for upstream conditions characterized by IMF cone angles less than 20 degrees-25 degrees, high Mach numbers and proton plasma beta <= 1.3. The minimum value for the total pressure observed by THEMIS in the magnetosheath adjacent to the magnetopause was 0.16 nPa and the fraction of the solar wind pressure applied to the magnetopause was therefore 0.2, extremely small. The equilibrium location of the magnetopause was modulated by a nearly continuous wavy motion over a wide range of time and space scales.
    關聯: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
    显示于类别:[太空科學研究所 ] 期刊論文

    文件中的档案:

    档案 描述 大小格式浏览次数
    index.html0KbHTML477检视/开启


    在NCUIR中所有的数据项都受到原著作权保护.

    社群 sharing

    ::: Copyright National Central University. | 國立中央大學圖書館版權所有 | 收藏本站 | 設為首頁 | 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - 隱私權政策聲明