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 987654321/50421
English  |  正體中文  |  简体中文  |  全文笔数/总笔数 : 80990/80990 (100%)
造访人次 : 41639116      在线人数 : 1842
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/987654321/50421


    题名: A predictive model of geosynchronous magnetopause crossings
    作者: Dmitriev,A;Suvorova,A;Chao,JK
    贡献者: 太空科學研究所
    关键词: INTERPLANETARY MAGNETIC-FIELD;STEADY-STATE RESPONSE;LOW-LATITUDE STATIONS;ART. NO. 1341;SOLAR-WIND;GEOMAGNETIC STORMS;RING CURRENT;DAYSIDE MAGNETOPAUSE;SUDDEN IMPULSES;ORBIT
    日期: 2011
    上传时间: 2012-03-27 17:31:28 (UTC+8)
    出版者: 國立中央大學
    摘要: We have developed a model predicting whether or not the magnetopause crosses geosynchronous orbit at a given location for given solar wind pressure P(sw), B(z) component of the interplanetary magnetic field (IMF), and geomagnetic conditions characterized by 1 min SYM-H index. The model is based on more than 300 geosynchronous magnetopause crossings (GMCs) and about 6000 min when geosynchronous satellites of GOES and Los Alamos National Laboratory (LANL) series are located in the magnetosheath (so-called MSh intervals) in 1994-2001. Minimizing of the P(sw) required for GMCs and MSh intervals at various locations, B(z), and SYM-H allows describing both an effect of magnetopause dawn-dusk asymmetry and saturation of B(z) influence for very large southward IMF. The asymmetry is strong for large negative B(z) and almost disappears when B(z) is positive. We found that the larger the amplitude of negative SYM-H, the lower the solar wind pressure required for GMCs. We attribute this effect to a depletion of the dayside magnetic field by a storm time intensification of the cross-tail current. It is also found that the magnitude of threshold for B(z) saturation increases with SYM-H index such that for small negative and positive SYM-H the effect of saturation diminishes. This supports an idea that enhanced thermal pressure of the magnetospheric plasma and ring current particles during magnetic storms results in the saturation of magnetic effect of the IMF B(z) at the dayside magnetopause. A noticeable advantage of the model's prediction capabilities in comparison with other magnetopause models makes the model useful for space weather predictions.
    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.html0KbHTML641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