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 987654321/56225
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 80990/80990 (100%)
Visitors : 42691496      Online Users : 1520
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: http://ir.lib.ncu.edu.tw/handle/987654321/56225


    Title: 中華衛星一號在上午時段所觀測之全球離子溫度分布;Global Distribution of Ion Temperature Observed by Rocsat-1 Satellite in the Morning Sector
    Authors: 趙吉光
    Contributors: 中央大學太空科學研究所
    Keywords: 大氣科學類
    Date: 2008-09-01
    Issue Date: 2012-10-01 11:48:22 (UTC+8)
    Publisher: 行政院國家科學委員會
    Abstract: 我國華衛一號(現已更名為福衛一號)上的電離層電漿電動效應儀,自1999 年起,已觀測五年多在電離層頂部的離子資料。透過這豐富的資料庫,我們已建立隨時間、季節與太陽週期變化的全球離子溫度分布。在2004 年,我們曾探究早晨時段離子溫度脊與溫度谷之觀測結果。但在那時候,我們沒有模式可進行精細的研究。僅能用其他觀測資料進行粗略的解釋,認為氧離子的絕熱壓縮與膨漲是其主因。但也有其他人認為,此分布完全是由電子溫度分布所決定,氧離子的對流效應並不重要。日前我們發現SAMI2 模式所產生的離子分布與目前我們所量測的結果相去甚遠。就我們所知,模式所給予的太陽輻射量過高,也許需要作一修正才可得到與觀測相近之結果。此外,我們會使用 HINOTORI 衛星的電子溫度量測,來驗證我們的推論與SAMI2 模式的正確性。透過一系列的比較,我們希望能進一步改良SAMI2 模式,使其能釐清產生早晨時段離子溫度脊與溫度谷之物理機制。 ; Ion temperature has been measured with the Ionospheric Plasma and Electrodynamics Instrument (IPEI) onboard the first satellite of Republic of China (ROCSAT-1) at 600 km altitude for 5.3 years. Global distributions of ion temperature have been constructed and investigated for different local times, seasons and solar variability. In 2004, we have published an article to discuss the possible causes to produce temperature crests and troughs in the morning sector. The adiabatic compression and expansion are expected to produce these distributions. However, some people thought that the heating from electrons should be the main cause. The convective motion seems play a minor role in these distributions. Meanwhile, we found that the SAMI2 model can not reproduce temperature crests and troughs in the morning sector. Currently we know that the amount of solar radiation is too high given in the model and it would result in insignificant adiabatic heating and cooling processes to produce the temperature crests and troughs in the morning sector. Furthermore, electron temperature distribution from HINOTORI satellite would be also used to check the correctness of the SAMI2 model and our explanation. We hope that this study can help improve the SAMI2 model and clarify the physical mechanisms to produce the temperature crests and troughs in the morning sector. ; 研究期間 9708 ~ 9807
    Relation: 財團法人國家實驗研究院科技政策研究與資訊中心
    Appears in Collections:[Graduate Institute of Space Science] Research Project

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML275View/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