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 987654321/103196
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 94201/94201 (100%)
Visitors : 81608168      Online Users : 5357
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/987654321/103196


    Title: Traveling magnetopause distortion related to a large-scale magnetosheath plasma jet: THEMIS and ground-based observations
    Authors: 蘇亞拉;Dmitriev, A. V.;Suvorova, A. V.
    Contributors: 全球大氣觀測與資料應用研究中心
    Keywords: Atmospheric sciences;Geomagnetic field;interplanetary discontinuities;Kinetic energy;Magnetism;magnetopause;magnetosheath;Plasma;plasma jets;Plasma physics;Solar energy;Space
    Date: 2012-01-01
    Issue Date: 2026-04-23 11:25:22 (UTC+8)
    Publisher: Wiley-Blackwell;Washington, DC: Blackwell Publishing Ltd
    Abstract: 摘要: Here, we present a case study of THEMIS and ground‐based observations of the perturbed dayside magnetopause and the geomagnetic field in relation to the interaction of an interplanetary directional discontinuity (DD) with the magnetosphere on 16 June 2007. The interaction resulted in a large‐scale local magnetopause distortion of an “expansion – compression – expansion” (ECE) sequence that lasted for ∼15 min. The compression was caused by a very dense, cold, and fast high‐βmagnetosheath plasma flow, a so‐called plasma jet, whose kinetic energy was approximately three times higher than the energy of the incident solar wind. The plasma jet resulted in the effective penetration of magnetosheath plasma inside the magnetosphere. A strong distortion of the Chapman‐Ferraro current in the ECE sequence generated a tripolar magnetic pulse “decrease – peak– decrease” (DPD) that was observed at low and middle latitudes by some ground‐based magnetometers of the INTERMAGNET network. The characteristics of the ECE sequence and the spatial‐temporal dynamics of the DPD pulse were found to be very different from any reported patterns of DD interactions with the magnetosphere. The observed features only partially resembled structures such as FTE, hot flow anomalies, and transient density events. Thus, it is difficult to explain them in the context of existing models. Key Points A magnetosheath jet causes a strong distortion of the dayside magnetopause The jet results in intense plasma penetration inside the magnetosphere Ground magnetic variations trace the jet traveling along the magnetopause
    其他題名: J. Geophys. Res
    出版者: Washington, DC: Blackwell Publishing Ltd
    出版日期: 2012-08
    出處: Journal of Geophysical Research: Space Physics, 2012-08, Vol.117 (A8), p.n/a
    資源來源: Wiley Online Library
    版權: 2012. American Geophysical Union. All Rights Reserved.
    版權: 2015 INIST-CNRS
    版權: Copyright American Geophysical Union 2012
    識別號: ISSN: 0148-0227
    識別號: ISSN: 2169-9380
    識別號: EISSN: 2156-2202
    識別號: EISSN: 2169-9402
    識別號: DOI: 10.1029/2011JA016861
    Appears in Collections:[Global Atmosphere Observation and Data Application Research Center] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML22View/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