Schaffner, D (University of California, Los Angeles)
Thursday 29 July 2010, 09:00-09:40

Schaffner, D (University of California, Los Angeles) Thursday 29 July 2010, 09:00-09:40

Turbulence and flow in the Large Plasma Device

Perhaps the greatest challenge in plasma science is to understand the multiscale interaction between small-scale fluctuations and large-scale plasma dynamics. This is crucial both in fundamental astrophysical and space physics research (e.g., turbulence in the solar wind) and in more practical terrestrial contexts (e.g., the performance of the international fusion reactor, ITER, will be limited by the transport caused by small-scale fluctuations). Multiscale plasma dynamics also represent a formidable and fascinating mathematical challenge, as new analytical and numerical methods have to be developed in order for major breakthroughs to become possible.

Read more at: http://www.newton.ac.uk/programmes/GYP/

Perhaps the greatest challenge in plasma science is to understand the multiscale interaction between small-scale fluctuations and large-scale plasma dynamics. This is crucial both in fundamental astrophysical and space physics research (e.g., turbulence in the solar wind) and in more practical terrestrial contexts (e.g., the performance of the international fusion reactor, ITER, will be limited by the transport caused by small-scale fluctuations). Multiscale plasma dynamics also represent a formidable and fascinating mathematical challenge, as new analytical and numerical methods have to be developed in order for major breakthroughs to become possible. Read more at: http://www.newton.ac.uk/programmes/GYP/

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Turbulence and flow in the Large Plasma Device

Turbulence and flow in the Large Plasma Device

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