實驗室模擬行星際磁場所控制 整體性的地球磁層結構

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傅瑋宗(Wei-Tsung Fu) 查詢紙本館藏

畢業系所

太空科學研究所

論文名稱

實驗室模擬行星際磁場所控制整體性的地球磁層結構
(Interplanetary Magnetic Field (IMF) Control over the Global Structures of Laboratory Magnetosphere)

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摘要(中)

藉由實驗室模擬太陽風與地球磁場所耦合的地球磁層結構，並以東西方向和南北方向觀測各種外加行星際磁場Interplanetary Magnetic Field (IMF) 控制下的磁層圖像。當外加南向和北向IMF時，都能觀察到極光，但是外加南向IMF時極光的亮度變得更強。此外，我們也探討了在日側和磁尾部分所產生的磁重聯現象。而當模擬地磁球以20度傾斜，我們除了影像結果也進行了電腦模擬，將其與實驗室模擬中的實驗結果的照片進行比較。應用(NASA’s Community Coordinated Modeling Center，簡稱 CCMC) CCMC上的兩種模擬整體性地球磁層的模式，我們得到電腦模擬與實驗室模擬相較之下，磁力線的曲率無論是模擬地磁球在未傾斜或傾斜，兩者定性上皆能相當匹配吻合。

摘要(英)

Both east - west and north - south view images of magnetosphere for various interplanetary magnetic field (IMF) parameters have been investigated simultaneously in a laboratory experiment of the solar wind - magnetosphere coupling. An aurora is observed for both case of southward and northward IMF but the luminosity becomes stronger for southward IMF. Also, the reconnections are investigated in the front and tail areas. Inserting the 20 - degree terrella tilt, the study of modeling analysis is also processed for comparison with photograph of the experimental results in the laboratory simulation. Applied the models on CCMC overview of the global structure, the comparisons of model and laboratory simulation show the curvatures of the magnetic lines are qualitatively matched for the un-tilted and tilted terrella.

關鍵字(中)

★ 實驗室電漿
★ 地球磁層
★ 行星際磁場
★ 太陽風

關鍵字(英)

論文目次

中文提要 i
英文提要 ii
誌謝 iii
目錄 iv
圖目錄 vi
表目錄 viii
1介紹 1
1.1 太空電漿物理研究…………………………………………………………1
1.2太空電漿物理實驗………………………………………………………… 1
1.3 University of California, Riverside Terrella 1 (UCR-
T1) 實驗設備……… 2
2實驗模擬流程 5
2.1 標度律 (Scaling Laws) 的回顧……………………………………………5
2.2 實驗設備…………………………………………………………………11
3影像結果 19
3.1 地球磁層的整體性 (Global) 結構………………………………………19
3.2 東西向與南北向同時性影像比較………………………………………23
3.3地磁球傾斜20度的整體性 (Global) 結構………………………………27

4 實驗室影像結果討論 30
4.1場致電流 (FAC) 與極光位置……………………………………………30
4.2 赤道部分的明亮區………………………………………………………32
5 整體性的地球磁層電腦模擬 36
5.1 美國的太空天氣模式整合中心 (NASA’s Community
Coordinated Modeling Center) 之大型數值碼………………………36
5.2實驗結果與不同模式的電腦模擬比較……………………………………37
5.2.1 磁傾角0度時的東西向視角影像與模擬結果之比較……………38
5.2.2 磁傾角0度時的南北向視角影像與模擬結果之比較……………39
5.2.3 磁傾角20度時的東西向視角影像與模擬結果之比較…………46
5.2.4 外加北向IMF時的日側影像特性…………………………………46
6 結論與未來展望 50
6.1 論文總結………………………………………………………………………………………………………………50
6.2 Solar wind Magnetosphere Ionosphere Link Explorer
(SMILE) 計畫…………………………………………………………………………………………………51
參考文獻 53

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指導教授

趙吉光

審核日期

2019-7-23

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