Visualization of turbulent flows is a powerful tool to help understand the turbulence dynamics and induced transport. However, it does not provide a quantitative description of the observed structures. In this paper, an approach to characterize quantitatively the topology of the flows is given. The technique, which can be applied to any type of turbulence dynamics, is illustrated through the example of resistive ballooning instabilities.
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Department of Astrophysical Sciences, Princeton Plasma Physics Laboratory, NJ,08543, United StatesDepartment of Astrophysical Sciences, Princeton Plasma Physics Laboratory, NJ,08543, United States
Huang, Yi-Min
Zhou, Yao
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School of Physics and Astronomy, Institute of Natural Sciences, MOE-LSC, Shanghai Jiao Tong University, Shanghai,200240, ChinaDepartment of Astrophysical Sciences, Princeton Plasma Physics Laboratory, NJ,08543, United States
Zhou, Yao
Loizu, Joaquim
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École Polytechnique Fédérale de Lausanne, Swiss Plasma Center, Lausanne,CH-1015, SwitzerlandDepartment of Astrophysical Sciences, Princeton Plasma Physics Laboratory, NJ,08543, United States
Loizu, Joaquim
Hudson, Stuart
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Princeton Plasma Physics Laboratory, New Jersey,08543, United StatesDepartment of Astrophysical Sciences, Princeton Plasma Physics Laboratory, NJ,08543, United States
Hudson, Stuart
Bhattacharjee, Amitava
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Department of Astrophysical Sciences, Princeton Plasma Physics Laboratory, NJ,08543, United StatesDepartment of Astrophysical Sciences, Princeton Plasma Physics Laboratory, NJ,08543, United States