中大學術數位典藏-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 987654321/102305
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 94201/94201 (100%)
Visitors : 81663663      Online Users : 3874
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
  • Adv. Search
    HomeLoginUploadHelpAboutAdminister Goto mobile version


    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/102305


    Title: Simulation in the front region of the earth's magnetosphere
    Authors: 趙吉光;Yur, Gung;Cheng, Ching-Chang;Chao, Chi-Kuang;Chao, Jih-Kwin;Rahman, Hafiz-Ur
    Contributors: 地球科學學院太空科學與工程學系
    Keywords: Laboratory simulation;Magnetopause;Magnetosphere
    Date: 2012-02-01
    Issue Date: 2026-04-23 11:05:59 (UTC+8)
    Publisher: Chinese Geoscience Union;Springer
    Abstract: 摘要: A laboratory experiment was conducted to investigate the interaction between a plasma beam and a magnetic dipole, simulating the interaction between the solar wind and magnetized planets. The emphasis in this paper is on the laboratory simulation in the front region of the Earth¡¦s magnetosphere and their variation under different solar wind conditions. The boundary in the front region of the magnetosphere is observed in a space simulation laboratory and the magnetospheric structure is produced by a super-Alfvénic and collisionless plasma beam interacting with terrella field. The boundary of the magnetosphere is determined by the factors that include solar wind parameters, such as magnetic fields, ion current density and magnetospheric structure images. It is interesting to compare the results of laboratory simulations with the empirical model by Shue et al. (1997) and the theoretical model by Cheng (1998) as well for the prediction of magnetopause locations under any solar wind condition. The comparisons show that for the northward IMF, magnetopause locations in the laboratory simulation are consistent with the theoretical model. As the magnitude of northward IMF Bz becomes higher, the subsolar distance and the flank position in laboratory simulations are consistent with the empirical model as well. For a lower southward IMF Bz, magnetopause locations in laboratory simulations are consistent with both the empirical and theoretical models. As the magnitude of the southward IMF Bz becomes higher, the subsolar distance and the flank position in laboratory simulations seem closer to the theoretical model than the empirical model.
    出版者: Springer
    出版日期: 2012-01-01
    出處: TAO : Terrestrial, atmospheric, and oceanic sciences, 2012-01, Vol.23 (1), p.085
    資源來源: Agricultural & Environmental Science Collection
    識別號: ISSN: 1017-0839
    識別號: EISSN: 2311-7680
    識別號: DOI: 10.3319/TAO.2011.06.20.02(AA)
    Appears in Collections:[DEPARTMENT OF SPACE SCIENCE AND ENGINEERING] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML16View/Open


    All items in NCUIR are protected by copyright, with all rights reserved.

    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