English  |  正體中文  |  简体中文  |  Items with full text/Total items : 94274/94274 (100%)
Visitors : 82850725      Online Users : 1452
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/987654321/102091


    Title: A comparison of a model using the FORMOSAT-3/COSMIC data with the IRI model
    Authors: 劉正彥;Kakinami, Yoshihiro;Liu, Jann-Yenq;Tsai, Lung-Chih
    Contributors: 地球科學學院太空科學與工程學系
    Keywords: Altitude;Earth and Environmental Science;Earth Sciences;Equator;Geology;Geophysics/Geodesy;Ionosphere
    Date: 2012-01-01
    Issue Date: 2026-04-23 11:02:44 (UTC+8)
    Publisher: Springer International Publishing AG;Berlin/Heidelberg: Springer Berlin Heidelberg
    Abstract: 摘要: In this study, an empirical model constructed using data of FORMOSAT3/COSMIC (F3/C) from 29 June, 2006, to 17 October, 2009, retrieves altitude profiles of electron density ( N e ). The model derives global N e profiles from 150 to 590 km altitude as functions of the solar EUV flux, day of year, local time and location under geomagnetically quiet conditions ( K p < 4). N e profiles derived by the model are further compared with those of the International Reference Ionosphere (IRI). Results show that the F 2 peak altitude h m F 2 and the electron density N m F 2 , as well as the electron density above, derived by the model are lower than those of the IRI model. The F3/C model reproduces observations of F3/C well at 410-km altitude while the IRI model overestimates them. The overestimation of the IRI model becomes large with decrease of EUV flux. It is found that the topside vertical scale height of the F3/C model shows high values not only magnetic dip equator but also middle latitude. The results differ significantly from those of IRI, but agree with those observed by topside sounders, Alouette and ISIS satellites.
    其他題名: Earth Planet Sp
    出版者: Berlin/Heidelberg: Springer Berlin Heidelberg
    出版日期: 2012-01-01
    出處: Earth, planets, and space, 2012-01, Vol.64 (6), p.545-551
    資源來源: Publicly available content database
    版權: The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences; TERRAPUB. 2012
    版權: The Society of Geomagnetism and Earth, Planetary and Space Sciences, The Seismological Society of Japan 2012
    識別號: ISSN: 1343-8832
    識別號: ISSN: 1880-5981
    識別號: EISSN: 1880-5981
    識別號: DOI: 10.5047/eps.2011.10.017
    Appears in Collections:[DEPARTMENT OF SPACE SCIENCE AND ENGINEERING] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML32View/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