Fusion born alpha particle drift simulation with background turbulence by GPU computing
碩士 === 國立成功大學 === 太空天文與電漿科學研究所 === 101 === This thesis investigates the fusion born alpha particle behavior in the presence of drift wave turbulence in toroidal geometry. We employed the guiding center motion and ballooning type drift wave as simulation model to examine the conservation of second ad...
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ndltd-TW-101NCKU50690712015-10-13T22:51:43Z http://ndltd.ncl.edu.tw/handle/57205422709144647809 Fusion born alpha particle drift simulation with background turbulence by GPU computing 以GPU模擬阿伐粒子在背景亂流中的漂移 BOTSZHUANG 黃柏慈 碩士 國立成功大學 太空天文與電漿科學研究所 101 This thesis investigates the fusion born alpha particle behavior in the presence of drift wave turbulence in toroidal geometry. We employed the guiding center motion and ballooning type drift wave as simulation model to examine the conservation of second adiabatic invariant. By the orbit-following code, we are able to control the parameter of particle and turbulence structure, e.g. particle energy and turbulence amplitude. In the analytical work , we found that parallel velocity is related to island width and the shift of island is proportional to ${omega}_{star}/V_{parallel}$. The statistical result is consistent with analytical work. In numerical work, for trapped particles, the second adiabatic does not easily break. Furthermore, the banana tip is sensitive to $E imes B$ drift since the $V_{parallel}$ is near zero. These numerical work are demonstrated by GPU's parallel computation , we can effectively reduce computation time and resource. Yasutaro Nishimura 西村泰太郎 2013 學位論文 ; thesis 46 en_US |
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碩士 === 國立成功大學 === 太空天文與電漿科學研究所 === 101 === This thesis investigates the fusion born alpha particle behavior in the presence of drift wave turbulence in toroidal geometry. We employed the guiding center motion and ballooning type drift wave as simulation model to examine the conservation of second adiabatic invariant. By the orbit-following code, we are able to control the parameter of particle and turbulence structure, e.g. particle energy and turbulence amplitude. In the analytical work , we found that parallel velocity is related to island width and the shift of island is proportional to ${omega}_{star}/V_{parallel}$. The statistical result is consistent with analytical work. In numerical work, for trapped particles, the second adiabatic does not easily break. Furthermore, the banana tip is sensitive to $E imes B$ drift since the $V_{parallel}$ is near zero. These numerical work are demonstrated by GPU's parallel computation , we can effectively reduce computation time and resource.
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Yasutaro Nishimura |
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Yasutaro Nishimura BOTSZHUANG 黃柏慈 |
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BOTSZHUANG 黃柏慈 |
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BOTSZHUANG 黃柏慈 Fusion born alpha particle drift simulation with background turbulence by GPU computing |
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BOTSZHUANG |
title |
Fusion born alpha particle drift simulation with background turbulence by GPU computing |
title_short |
Fusion born alpha particle drift simulation with background turbulence by GPU computing |
title_full |
Fusion born alpha particle drift simulation with background turbulence by GPU computing |
title_fullStr |
Fusion born alpha particle drift simulation with background turbulence by GPU computing |
title_full_unstemmed |
Fusion born alpha particle drift simulation with background turbulence by GPU computing |
title_sort |
fusion born alpha particle drift simulation with background turbulence by gpu computing |
publishDate |
2013 |
url |
http://ndltd.ncl.edu.tw/handle/57205422709144647809 |
work_keys_str_mv |
AT botszhuang fusionbornalphaparticledriftsimulationwithbackgroundturbulencebygpucomputing AT huángbǎicí fusionbornalphaparticledriftsimulationwithbackgroundturbulencebygpucomputing AT botszhuang yǐgpumónǐāfálìzizàibèijǐngluànliúzhōngdepiàoyí AT huángbǎicí yǐgpumónǐāfálìzizàibèijǐngluànliúzhōngdepiàoyí |
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