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 987654321/27426
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 78818/78818 (100%)
Visitors : 34621604      Online Users : 730
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: http://ir.lib.ncu.edu.tw/handle/987654321/27426


    Title: Three-dimensional ionospheric electron density structure of the Weddell Sea Anomaly
    Authors: Lin,CH;Liu,JY;Cheng,CZ;Chen,CH;Liu,CH;Wang,W;Burns,AG;Lei,J
    Contributors: 太空科學研究所
    Date: 2009
    Issue Date: 2010-06-29 18:38:15 (UTC+8)
    Publisher: 中央大學
    Abstract: This paper provides the first three-dimensional description of the ionospheric density structure of the Weddell Sea Anomaly (WSA). The WSA is characterized by a nighttime ionospheric density greater than that in daytime in the Weddell Sea region around the Antarctic Peninsula during the southern hemisphere summer. It was first observed by ground-based ionosondes located in the Antarctica back in the 1950s and was further investigated by two-dimensional maps over the oceans using TEC measurements collected by the TOPEX/Poseidon recently. Although these TEC maps have provided two-dimensional views for tracking the time-evolution and spatial coverage of the WSA, the vertical distribution of this peculiar feature is still unavailable. With the vertical ionospheric density profiles observed by the FORMOSAT-3/COSMIC, three-dimensional density structure of the WSA is presented here for the first time. Meanwhile, a similar WSA signature is observed in the northern and eastern hemisphere during June solstice by both the GPS-TEC and the FORMOSAT-3/COSMIC electron density observations. From the observed altitudinal structure of the WSA during 1800-2400 LT and the similar feature occurred in the opposite hemisphere suggest that the southward offset of the magnetic equator with respect to the geographic equator plays a major role for the WSA formation.
    Relation: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
    Appears in Collections:[Graduate Institute of Space Science] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML635View/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