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研究生： 黃子耀
Tzu-Yao Huang
論文名稱： 雷射電漿中無碰撞激震波的全域與局域量測
Global and local measurements of collisionless shock waves in laser produced plasmas
指導教授： 朱旭新
Hsu-hsin Chu
藏滿康浩
Yasuhiro Kuramitsu
口試委員:
學位類別： 碩士
Master
系所名稱： 理學院 - 物理學系
Department of Physics
論文出版年： 2018
畢業學年度： 106
語文別： 英文
論文頁數： 55
中文關鍵詞： 無碰撞激震波 、雷射電漿 、實驗室天文學
外文關鍵詞： collisionless shock wave, laser-produced plasma, laboratory astrophysics
相關次數： 點閱：10  下載：0 
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    • 無碰撞激震波在宇宙中扮演著重要的角色。在雷射電漿中無碰撞激震波已被觀
    察。為了觀察激震波馬赫數，我們需要知道激震波速度與上游電漿聲速。藉由
    高強度雷射照射固態靶，我們產生了在雷射電漿中的環境電漿。我們觀察時間
    與空間的電漿演化藉由全域的圖像；而局域電漿溫度、密度與速度由集體的湯
    木森散射系統所量測。從局域電漿溫度與密度，我們可以知道上游電漿聲速及
    計算激震波馬赫數。

    One of the fundamental factors in the universe is collisionless shocks. Collisionless shocks have been observed in laser-produced plasma. To obtain the shock Mach number, we need to know the shock velocity and upstream sound velocity. By irradiating a solid target with the high-power laser pulse, we produced laser-produced plasma in a presence of an ambient plasma. We observed temporal and spatial plasma Evolution with global images. The local temperature, density, and velocity of electrons and ions
    are obtained by collective Thomson scattering(CTS) system. From local temperature and density, we can understand the upstream sound velocity and obtain the shock Mach number.

    1 Introduction 1 2 Shock Waves Produced with 500-ps Laser Pulse 4 2.1 GEKKO XII-HIPER Laser System 4 2.1.1 Experimental Design and Diagnostic System in Osaka University 5 2.1.2 Self-Emission Imaging 8 2.1.3 Shadowgraphy 8 2.1.4 Collective Thomson Scattering 14 2.2 Results in Osaka GEKKO-XII Laser Facility 16 3 Shock Waves Produced with 50-fs Laser Pulse 28 3.1 NCU 100 TW Laser Facility 28 3.1.1 Experimental Setup in NCU 100 TW Laser Facility 29 3.1.2 Mach-Zechnder Interferometer 30 3.1.3 Thomson Parabola 36 3.2 Results in 100 TW Laser Facility in NCU 38 4 Summary and Discussion 41

    [1] Burgess, D.; Möbius, E.; Scholer, M. ”Ion Acceleration at the Earth’s Bow Shock,” Space Science Reviews, Volume 173, Issue 1-4, pp. 5-47 (2012).

    [2] K. Koyama, R. Petre, E. V. Gotthelf, U. Hwang, M. Matsuura, M. Ozaki, and S. S. Holt. ”Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006,” Nature, 378:255-258 (1995).

    [3] F. A. Aharonian, A. G. Akhperjanian, K.-M. Aye, A. R. Bazer-Bachi, M. Beilicke, W. Benbow, D. Berge, P. Berghaus, K. Bernlöhr, O. Bolz, C. Boisson, C. Borgmeier, F. Breitling, A. M. Brown, J. Bussons Gordo, P. M. Chadwick, V. R. Chitnis, L.-M. Chounet, R. Cornils, L. Costamante, B. Degrange, A. Djannati-Ataï, L. O'C. Drury, T. Ergin, P. Espigat, F. Feinstein, P. Fleury, G. Fontaine, S. Funk, Y. A. Gallant, B. Giebels, S. Gillessen, P. Goret, J. Guy, C. Hadjichristidis, M. Hauser, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, W. Hofmann, M. Holleran, D. Horns, O. C. de Jager, I. Jung, B. Khélifi, Nu. Komin, A. Konopelko, I. J. Latham, R. Le Gallou, M. Lemoine, A. Lemière, N. Leroy, T. Lohse, A. Marcowith, C. Masterson, T. J. L. McComb, M. de Naurois, S. J. Nolan, A. Noutsos, K. J. Orford, J. L. Osborne, M. Ouchrif, M. Panter, G. Pelletier, S. Pita, M. Pohl, G. Pühlhofer, M. Punch, B. C. Raubenheimer, M. Raue, J. Raux, S. M. Rayner, I. Redondo, A. Reimer, O. Reimer, J. Ripken, M. Rivoal, L. Rob, L. Rolland, G. Rowell, V. Sahakian, L. Saugé, S. Schlenker, R. Schlickeiser, C. Schuster, U. Schwanke, M. Siewert, H. Sol, R. Steenkamp, C. Stegmann, J.-P. Tavernet, C. G. Théoret, M. Tluczykont, D. J. van der Walt, G. Vasileiadis, P. Vincent, B. Visser, H. J. Völk & S. J. Wagner ”High-Energy particle acceleration in the shell of a supernova remnant,” Nature, 432:75-77 (2004).

    [4] E. A. Helder, J. Vink, C. G. Bassa, A. Bamba, J. A. M. Bleeker, S. Funk, P. Ghavamian, K. J. van der Heyden, F. Verbunt, and R. Yamazaki. ”Measuring the Cosmic-Ray Acceleration Efficiency of a Supernova Remnant,” Science,
    325:719,(2009).

    [5] Y. Kuramitsu, Y. Sakawa, T. Morita, C. D. Gregory, J. N. Waugh, S. Dono, H. Aoki, H. Tanji, M. Koenig, N. Woolsey, H. Takabe. ”Time Evolution of Collisionless Shock in Counterstreaming Laser-Produced Plasmas,” Phys. Rev. Lett. 106, 175002 (2011).

    [6] N. Miyanaga, M. Nakatsuka, H. Azechi, H. Shiraga, T. Kanabe, H. Asahara, H. Daido, H. Fujita, K. Fujita, Y. Izawa, T. Jitsuno, T. Kawasaki, H. Kitamura, S. Matsuo, K. Mima, N. Morio, M. Nakai, S. Nakai, K. Nishihara, H. Nishimura, T. Sakamoto, K. Shigemori, K. Sueda, K. Suzuki, K. Tsubakimoto, H. Takabe, S. Urushihara, H. Yoshida, T. Yamanaka and C. Yamanaka. ”The GEKKO XII-HIPER (High Intensity Plasma Experimental Research) System Relevant to Ignition Targets,” in Proceedings of the 18th International Conference on Fusion Energy (IAEA, Vienna, 2000), Paper No. IFP/14(R), IAEA-CN-77.

    [7] M. C. Richardson, C.-S. Koay, K. Takenoshita, C. Keyser, B. Bernath, S. A. George, and S. Teerawattanasook, Proc. SPIE https://doi.org/10.1117/12.597349 5580, 434 (2005).

    [8] J. N. Waugh. D. Gregory L. A. WilsonB. Loupias E. BrambrinkM. Koenig Y. Sakawa Y. Kuramitsu H. Takabe R. Kodama N. C. Woolsey. ”A jet production experiment using the high-repetition rate Astra laser,” Astrophysics and Space Science, Volume 322, Issue 1–4, pp 31–35 (2009).

    [9] T.-S. Hung, C.-H. Yang, J. Wang, S.-y. Chen, J.-Y. Lin, and H.-h. Chu. ”A 110-TW multiple-beam laser system with a 5-TW wavelength-tunable auxiliary beam for versatile control of laser-plasma interaction,” Appl. Phys. B 117, 1189 (2014).

    [10] Kelly WarnerGary, M.Hieftje. ”Thomson scattering from analytical plasmas” Spectrochimica Acta Part B: Atomic Spectroscopy, Volume 57, Issue 2, 201-241 (2002).

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