English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 80990/80990 (100%)
造訪人次 : 42772521      線上人數 : 1240
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/987654321/50467


    題名: The 762 nm emissions of sprites
    作者: Kuo,CL;Chang,SC;Lee,LJ;Huang,TY;Chen,AB;Su,HT;Hsu,RR;Sentman,DD;Frey,HU;Mende,SB;Takahashi,Y;Lee,LC
    貢獻者: 太空科學研究所
    關鍵詞: MOLECULAR NITROGEN;OXYGEN;THERMOSPHERE;PARAMETERS;ATMOSPHERE;SATELLITE;DISCHARGE;AFTERGLOW;O-2;N-2
    日期: 2011
    上傳時間: 2012-03-27 17:32:43 (UTC+8)
    出版者: 國立中央大學
    摘要: We report the 762 nm emissions in sprites recorded by the ISUAL experiment onboard the FORMOSAT-2 satellite. The 762 nm imager filter is centered at 763.3 nm with a 7 nm bandwidth at 50% transmittance. Sprite emissions in this passband include the N(2) first positive (1PN(2)) bands, (2, 0) and (3, 1), the O(2) atmospheric (atm) band (0, 0), and the hydroxyl (4, 0) emissions. Because these mixed emissions cannot be resolved in the 762 nm narrowband filter, a zero-dimensional plasma chemistry model is used to estimate the expected relative intensities of these emission bands in sprites. The computed 1PN(2) brightness in a single streamer is 1.4 MR and 2.6 kR for the O(2) atm band emissions at frame integration times of 30 ms. In the 762 nm passband, the 1PN(2) emissions are the dominant emissions in sprites, and the ratio of 1PN(2) to O(2) atmospheric emissions is similar to 500, while the hydroxyl emissions can be neglected. In this ISUAL 762 nm campaign, the brightest sprite out of the four recorded events has possible O(2) atm band emissions that lasted more than 90 ms, and its observed brightness is consistent with the model prediction. Even though the lightning 762 nm emissions are strongly absorbed by O(2) below 60 km, the ISUAL observed parent lightning emissions in this passband are still more than a factor of two brighter than those from ISUAL observed sprites. Hence for spacecraft nadir TLE detection missions, 762 nm bands may not be used as the sole signature to identify sprites, and auxiliary emission bands are needed.
    關聯: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
    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.html0KbHTML600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