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 987654321/27505
English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 80990/80990 (100%)
造訪人次 : 42573180      線上人數 : 1710
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: http://ir.lib.ncu.edu.tw/handle/987654321/27505


    題名: The observations of sporadic E irregularities in equatorial anomaly crest zone by using Chung-Li VHF radar
    作者: Chen,YH;Chu,YH;Liu,CH
    貢獻者: 太空科學研究所
    關鍵詞: AURORAL E-REGION;MU-RADAR;E-LAYERS;IONOSPHERIC IRREGULARITIES;COHERENT BACKSCATTER;ASPECT SENSITIVITY;ELECTROJET;WAVES;INSTABILITY;RADIO
    日期: 1996
    上傳時間: 2010-06-29 18:39:53 (UTC+8)
    出版者: 中央大學
    摘要: With employing 52 MHz Chung-Li VHF radar, the ionospheric irregularities embedded in sporadic E layer in equatorial anomaly crest zone are observed. It shows that in general the echoes of sporadic E irregularities in association with plume-like structures are occurred in the height range from 99 km to 122 km and centered at around 108 km, quite consistent with the observations made by local HF ionosonde. Spectrally analysing the radar returns indicates that the low-velocity type 1 (or type 3) and type 2 radar spectra are both observed and may appear simultaneously in the same Doppler spectrum. Their characteristics are estimated and discussed in the text. Differing from those obtained by using VHF radars situated in equatorial and auroral zone, the Doppler velocities of type 1 (or type 3) radar spectra observed here are generally within 95 similar to 115 ms(-1), fairly smaller than the former ones. The typical Doppler velocity and spectral width for type 2 radar spectra are within -150 similar to 160 ms(-1) and 16 similar to 30 Hz, respectively. The average drift velocity of 3-meter irregularities deduced from type 2 spectra is also presented. It displays that the drift is toward the radar at the lower height, while away above approximately 104 km. Moreover, below the altitude of around 108 km the drift velocity varies substantially with height at the gradient of about 10 ms(-1)/km. Above that height, the drift velocity changes slightly with height. The plausible process corresponding to these two distinct behaviors of height variation of drift velocity are also discussed in this article.
    關聯: JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY
    顯示於類別:[太空科學研究所 ] 期刊論文

    文件中的檔案:

    檔案 描述 大小格式瀏覽次數
    index.html0KbHTML485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