| 研究生: |
劉哲宇 Liu, Che-Yu |
|---|---|
| 論文名稱: |
由兩相對電漿噴流對撞產生之滯留電漿密度量測 Density measurement of the stagnated plasma from the collision of two counter propagating plasma jets |
| 指導教授: |
張博宇
Chang, Po-Yu |
| 學位類別: |
碩士 Master |
| 系所名稱: |
理學院 - 太空與電漿科學研究所 Institute of Space and Plasma Sciences |
| 論文出版年: | 2023 |
| 畢業學年度: | 111 |
| 語文別: | 英文 |
| 論文頁數: | 82 |
| 中文關鍵詞: | 錐形導線陣列 、電漿噴流 、正向碰撞 、軸向壓縮 、脈衝功率系統 |
| 外文關鍵詞: | Conical-wire array, Plasma jet, Head-on collision, Z-pinch, Pulsed-power system |
| 相關次數: | 點閱:63 下載:6 |
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本論文中我們研究透過兩正向碰撞的電漿噴流產生的滯留電漿,可以用來模擬銀河系及恆星形成區等大尺度且難以研究的天文物理現象。實驗是使用 1-kJ 的高壓脈衝功率系統,並透過雷射及可見光相機系統進行量測。系統放電時可產生一個峰值約為 123.5 kA 的脈衝電流,且上升時間約為 1592 ns,用於驅動一對彼此相對的錐形導線陣列所組成的雙錐形導線陣列。為了使雷射不會受系統放電所產生的電磁脈衝訊號影響,我們設計了一個八級的高壓脈衝產生器來改善我們用於觸發系統放電的多級高壓觸發系統,改善後的觸發系統的延遲時間為 230±90 ns。最後我們透過分析雷射相機系統所拍攝的影像,得到各時間點上方電漿噴流的長度後,將其長度對應時間做線性擬合,並將線性擬合的斜率定義為平均速度,得到的速值約為 17.2±4 km/s。除此之外,我們透過干涉儀所拍攝的影像,得到因雷射穿過電漿而產生的相位變化圖片,求得各時間點電漿噴流的寬度變化,發現在628.8 ns時上下兩電漿噴流的寬度都減少。透過相位變化的圖片,我們可以得到電漿密度,再將其從上到下分成七個區域觀察電漿密度的變化,發現在約 600 ns後,電漿會開始推積在雙錐形線陣列的中間並形成密度約在 10^{22} 每立方公尺的滯留電漿,因此根據密度的變化以及寬度的變化,意味著電漿噴流會受到軸向壓縮的效應影響,累積在正中心。
In this thesis, we study the stagnated plasma produced by two colliding plasma jets, which can be used to simulate large-scale and difficult-to-study astrophysical phenomena such as the Milky Way and star-forming regions. The experiment was performed using a 1-kJ high-voltage pulsed-power system and measured through a laser and visible light camera system. When the system discharges, it generates a pulse current with a peak value of approximately 123.5 kA and a rise time of approximately 1592 ns, which is used to drive a bi-conical-wire array consisting of a pair of conical-wire arrays facing each other. In order to prevent the laser from being affected by the electromagnetic pulse signal generated by system discharge, we designed an eight-stage high-voltage pulse generator to improve our multi-stage high-voltage trigger system. The delay of the system with the improved triggering system is 230±90 ns. Finally, by analyzing the images captured by the laser camera system, we obtained the length of the plasma jet at different times. Then, we made a linear fitting to the length corresponding to different times. And we defined the slope of the linear fitting as the averaged jet speed. The averaged speed is about 17.2±4 km/s. Through the images taken by the interferometer, we can obtain the time dependent density and the width of the plasma jets. We found that the widths of the top and down plasma jets both decreased after 628.8 ns. In addition, we divide the bi-conical-wire array in seven regions from top to bottom to observe the change of the plasma density. We found that after about 600 ns, the plasma started to pile up in the middle plane of the bi-conical-wire array and formed a stagnanted plasma with a density of about 10^{22} per m^{3}. It suggests that the stagnated plasma not only came from the plasma jets but also from the ablated plasma from the tungsten wires of the bi-conical-wire array.
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