PPT-Gyrokinetic simulation of electron turbulence spectrum
Author : finley | Published Date : 2023-10-27
Chika Kawai 12 Shinya Maeyama 2 Yasuhiro Idomura 2 Yuichi Ogawa 1 1 GSFSUniv Tokyo 2JAEA This work was carried out using the HELIOS supercomputer system at Computational
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Gyrokinetic simulation of electron turbulence spectrum: Transcript
Chika Kawai 12 Shinya Maeyama 2 Yasuhiro Idomura 2 Yuichi Ogawa 1 1 GSFSUniv Tokyo 2JAEA This work was carried out using the HELIOS supercomputer system at Computational Simulation Centre of International Fusion Energy Research Centre IFERCCSC Aomori Japan under the Broader Approach collaboration between . Ye Zhao. , . Zhi. Yuan and Fan Chen. Kent State University, Ohio, USA. Turbulent Fluid. “Turbulence is an irregular motion which in general makes its appearance in fluids, gaseous or liquid”. Taylor and von . http://turb.seas.ucla.edu/~jkim/sciam/turbulence.html Turbulence ? Why do the skin of sharks have groves ? Related Links But what exactly is turbulence? A few everyday examples may be illuminati Kenji Yoshida. 1. , Shoji Torii. 2. . on behalf of . the PPB-BETS collaboration. 1. Shibaura Institute of Technology, Japan. 2. Waseda University, Japan. March 3, 2010. 2. HEAD 2010. Side view of the detector. Radial . Localization of Alfven Eigenmodes . and . Zonal Field Generation. Z. Lin. University of California, . Irvine. Fusion Simulation Center, Peking . University. Z. X. . Wang. , W. . W. Heidbrink, I. . CSDMS Annual Meeting 2016: Capturing Climate Change (May 17-19, 2016). Zhen Cheng. 1. (Charlie. ), . Tian-Jian. . Hsu. 1. . (Tom. ), . Julien. Chauchat. 2. ,. . Thibaud. Revil-. Baudard. 3. 1. University of Delaware, Newark, DE, 19716, USA. in a Developing Turbulence. . Shuichi M. ATSUKIYO. . ESST Kyushu Univ.. Collaborator : T. . Hada. Outline . Background. -- motivation. -- acceleration processes in turbulent plasmas. -- parametric instability (PI). Bas van de . Wiel. , . Ivo. van . Hooijdonk. & Judith . Donda. in collaboration with:. Fred . Bosveld. , Peter Baas, . Arnold . Moene. , Harm . Jonker. , . Jielun. Sun, Herman Clercx, . e.a. .. He Zhang. MEIC Collaboration Meeting, 10/06/2015. He Zhang. ---. 2. ---. Outline. Staged cooling scheme. Numerical simulation. Cooling with correlated electron beam. Simulation code development. Summary. Light is an electromagnetic wave*.. Wave Characteristics. Frequency (. ν. ). : number of waves that pass a point in a given period of time. Total . energy. is proportional to amplitude and frequency of waves. . Katsuaki. Asano. (. ICRR, U. Tokyo. ). Collaborators:. Yuto. . Teraki. (YITP, Kyoto), Masaaki. . Hayashida. (ICRR),. Fumio . Takahara. (Osaka) etc.. Non-thermal Emission. Supernova Remnant SN1006. Siming. Liu. University of Glasgow. Collaborators. Vahe. ’ . Petrosian. , . Yanwei. Jiang: Stanford University. Zhonghui. Fan: Yunnan University. Oct. 2008 Krakow, Poland . Outline. I: Observations: Distribution. S. Ku et al.. A fast edge turbulence bifurcation achieved in XGC1 when heat accumulation ~P. L-H. in the edge layer. in an L-mode diverted C-Mod edge geometry. with neutral particle recycling (R=0.99). Yang . Ren. Walter Guttenfelder. Gregory W. Hammett. for the NSTX-U Research Team. NSTX-U PAC-33 Meeting. PPPL – B318. February 19-21, 2013. NSTX-U. Supported by . Culham Sci Ctr. York U. Chubu U. ionospheric. anomalies and how they affect our understanding of coupling. Jean-Pierre St-Maurice. ISAS, U of Saskatchewan. Background. A look back at some intriguing problems I tackled over the years.
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