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 987654321/102091
English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 94274/94274 (100%)
造訪人次 : 82858564      線上人數 : 1580
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
搜尋範圍 查詢小技巧:
  • 您可在西文檢索詞彙前後加上"雙引號",以獲取較精準的檢索結果
  • 若欲以作者姓名搜尋,建議至進階搜尋限定作者欄位,可獲得較完整資料
  • 進階搜尋


    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/102091


    題名: A comparison of a model using the FORMOSAT-3/COSMIC data with the IRI model
    作者: 劉正彥;Kakinami, Yoshihiro;Liu, Jann-Yenq;Tsai, Lung-Chih
    貢獻者: 地球科學學院太空科學與工程學系
    關鍵詞: Altitude;Earth and Environmental Science;Earth Sciences;Equator;Geology;Geophysics/Geodesy;Ionosphere
    日期: 2012-01-01
    上傳時間: 2026-04-23 11:02:44 (UTC+8)
    出版者: Springer International Publishing AG;Berlin/Heidelberg: Springer Berlin Heidelberg
    摘要: 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
    顯示於類別:[太空科學與工程學系] 期刊論文

    文件中的檔案:

    檔案 描述 大小格式瀏覽次數
    index.html0KbHTML32檢視/開啟


    在NCUIR中所有的資料項目都受到原著作權保護.

    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