English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 64745/64745 (100%)
造訪人次 : 20420536      線上人數 : 331
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/987654321/5184


    題名: 利用台灣日震觀測網的太陽影像資料研究 太陽差動自轉的變化情形;A Study of Solar Differential Rotation Based on Solar Images Obtained From Taiwan Oscillation Network
    作者: 余秀珊;Hsiu-Shan Yu
    貢獻者: 太空科學研究所
    關鍵詞: 太陽差動自轉;日震學;solar differential rotation;helioseismology or solar seismology
    日期: 2004-06-16
    上傳時間: 2009-09-22 09:46:39 (UTC+8)
    出版者: 國立中央大學圖書館
    摘要: 太陽的差動自轉(solar differential rotation)可將原本南北方向的磁 偶極場(poloidal field)拉成東西方向(toroidal field)。因此太陽差動自轉 在太陽磁場的週期變化中,扮演著很重要的角色。早期科學家從追踨 太陽黑子(sunspots)的運動所得到的太陽差動自轉模式受到太陽黑子 分佈情形的限制,在時空解析度上,很難再進一步提升。台灣日震觀 測網(Taiwan Oscillation Network, TON)提供一分鐘一張高時空解析度 的broadband K-line image。這些K-line 影像圖中除了太陽黑子與明亮 的譜斑(plages) 外還有超米粒組織的明亮邊界(supergranulation boundaries,SGB),都可以作為研究太陽差動自轉的追蹤標記。由於 超米粒組織的明亮邊界的緯度分佈甚廣且數量不受太陽週期的影 響,因此藉著分析TON K-line image 可得高時空解析度之太陽表面差 動自轉的情形。 在本論文的研究中,我們從1994 年起,每年分析數日已經 remapped 的TON 資料來研究太陽差動自轉隨太陽週期的變化情形。 初步的結果發現,在1994~2000 年間,太陽的轉速在北半球,有逐年 減慢的趨勢,但在南半球,則是逐年的增快。但是進一步的檢驗 remapped 的資料後,發現有一部分的南北不對稱性是受到不正確的 remapped 影像的影響。因此本論文在太陽差動自轉隨太陽週期變化 方面的研究仍未成功。但是在本研究中,我們設計了一種只要半天的 資料量,就可以很快的求得太陽在不同緯度的自轉角速率。我們同時 找到一種檢驗remapped 結果是否正確的方法。相信我們所研發的這 兩項資料分析方法,將對未來利用TON 資料做日震分析的研究有很 大的幫助。 i Solar latitudinal differential rotation, which can generate toroidal magnetic field from a poloidal magnetic field, plays an important role on solar dynamo and formation of solar cycle. Solar differential rotation was first found by tracing sunspots' motion. The well-known solar differential rotation formula obtained from sunspots' motion is only applicable to the middle- and lower- latitude regions and has a poor latitudinal resolution during solar minimum. Supergranulations, or chromosphere networks, or plages are excellent targets for studying solar differential rotation in all latitudes and during different phases of solar cycle. The one-minute broadband K-line images obtained from Taiwan Oscillation Network (TON) provide an opportunity to study differential rotation of supergranulations or plages up to very high latitude. Our preliminary results show that weak north-south asymmetry on solar differential rotation is found during years 1994~1997. Strong north-south asymmetry on solar differential rotation is found during years 1998~2000. According to our preliminary study, solar rotation rate decreases with time in northern hemisphere, but increases with time in southern hemisphere during years 1994~2000. However, further study indicates that the strong north-south asymmetry on solar differential rotation may partially due to incorrect mapping of the TON data sets we used in this thesis. Thus, our study of solar cycle dependence on solar differential rotation is not fully successful. But, in this thesis we have developed a very efficient way to obtain solar rotation rate at different latitude. We have also found a simple way to check and to improve the accuracy of a remapped image. Therefore, using the techniques developed in this thesis can provide accurate remapped images and real-time solar differential rotation information for future solar seismology study using TON data sets.
    顯示於類別:[太空科學研究所 ] 博碩士論文

    文件中的檔案:

    檔案 大小格式瀏覽次數
    0KbUnknown508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 ©   - 回饋  - 隱私權政策聲明