Gyrokinetics in Laboratory and Astrophysical Plasmas

Gyrokinetics in Laboratory and Astrophysical Plasmas

by

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/

Recent Episodes

  • 2D and 3D kinetic simulations of the MRX reconnection experiment

    14 years ago

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  • Alfvénic turbulence in tokamaks: from micro- to meso-scale fluctuations

    14 years ago

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  • Breaking field lines during reconnection: it's anomalous viscosity not anomalous resistivity

    14 years ago

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  • Dispersive Alfvén-wave turbulence and the role of self-generated temperature anisotropy

    14 years ago

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  • Effects of three-dimensional geometry and radial electric field on ITG turbulence and zonal flows

    14 years ago

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  • Electric field effects in stellarators

    14 years ago

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  • Electrostatic instabilities, turbulence and fast ion interactions in simple magnetised plasmas

    14 years ago

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  • Entropy cascade in 2D-2V Vlasov-hybrid electrostatic model

    14 years ago

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  • Entropy transfer processes in kinetic plasma turbulence and zonal flows

    14 years ago

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  • Experiments on the Propagation of Plasma Filaments in VTF

    14 years ago

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