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 987654321/27429
English  |  正體中文  |  简体中文  |  全文笔数/总笔数 : 78852/78852 (100%)
造访人次 : 35168800      在线人数 : 1276
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/987654321/27429


    题名: Two-spacecraft observations of an interplanetary slow shock
    作者: Lin,CC;Feng,HQ;Wu,DJ;Chao,JK;Lee,LC;Lyu,LH
    贡献者: 太空科學研究所
    关键词: EARTHS DISTANT MAGNETOTAIL;PLASMA SHEET BOUNDARY;LARGE MAGNETIC SHEAR;MODE SHOCKS;GEOMAGNETIC TAIL;SOLAR-WIND;AMPTE/IRM OBSERVATIONS;MAGNETOPAUSE;RECONNECTION;REVERSE
    日期: 2009
    上传时间: 2010-06-29 18:38:19 (UTC+8)
    出版者: 中央大學
    摘要: Slow-mode shocks in space have been identified via one spacecraft observation by many authors since 1970. However, Feng et al. suggested that the analysis using single-spacecraft observation based only on the Rankine-Hugoniot relations could misinterpret a tangential discontinuity as a slow shock. In this paper, we identify a slow-mode shock using a model fitting based on both the Rankine-Hugoniot relations and intraspacecraft timing. As a result, we found a slow-shock solution that, including the local parameters and propagation time, agrees well with the observations. The slow shock may be associated with an asymmetric reconnection exhaust at a heliospheric current sheet.
    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.html0KbHTML545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