English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 78852/78852 (100%)
造訪人次 : 37999112      線上人數 : 829
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/987654321/27433


    題名: An investigation of 19.5 GHz sky noise temperature over Taiwan area
    作者: Chu,YH;Shih,SP
    貢獻者: 太空科學研究所
    關鍵詞: LI VHF RADAR;ECHO POWER;RAIN;ATTENUATION
    日期: 1999
    上傳時間: 2010-06-29 18:38:24 (UTC+8)
    出版者: 中央大學
    摘要: A number of ground-based instruments, including 19.5 GHz radiometer, optical raingauge, portable weather station, and high resolution disdrometer, were set up to conduct the Ka band propagation experiment of the Experimental Communication Payload (ECP) for ROCSAT-1. In this article, 19.5 GHz background sky noise temperatures measured at Chung-Li and Tainan sites are presented and investigated. Long-term statistics of the 19.5 GHz background sky noise temperature observed by a vertically pointed radiometer in precipitation-free condition over the Taiwan area shows that the percentages of time that the sky noise temperature exceeds 20 K, 30 K, 40 K and 50 K are, respectively, 98%, 85%, 53%, and 27%. However, in precipitating environments, statistics shows that the percentage of time that the sky noise temperature exceeds 55 K, 100 K, 150 K, and 200 K are, respectively, 22%, 13%, 4.5%, and 2%. The statistics of sky noise temperatures observed at different zenith angles under environments without precipitation is also made. The results show that 80% of the observed sky noise temperatures at zenith angles of 100, 300, 500 and 70 degrees are, respectively, in the ranges of 92 - 180 K, 39 - 52 K, 26 - 33 K, and 21 - 27 K. In addition, a comparison between surface rainfall rate recorded by the optical raingauge and sky noise temperature measured by 19.5 GHz radiometer shows that the former lags behind the latter by about 5 minutes, implying non-uniform and inhomogeneous distribution of precipitation in the air. In order to measure the precipitation aloft, the Chung-Li VHF radar was operated simultaneously. Champaign observation shows that there is no latency between sky noise temperature and VHF backscatter from precipitation. This result implies that the VHF backscatter from precipitation can be employed to validate the observed sky noise temperature. In addition, we also find that the sky noise temperature may be as high as 155 K (corresponding to 3.6 dB attenuation) under an environment without surface precipitation. This feature is attributed to the dense water vapor and heavy cloud.
    關聯: TERRESTRIAL ATMOSPHERIC AND OCEANIC SCIENCES
    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.html0KbHTML438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