29 June 2026 to 3 July 2026
EICC, Edinburgh
Europe/London timezone

Stationary power-law solutions of weak kinetic-Alfvenic turbulence

Not scheduled
20m
EICC, Edinburgh

EICC, Edinburgh

150 Morrison St, Edinburgh EH3 8EE
Poster Presentation Fundamental Plasma Physics - Theory (BSAP)

Description

Based on nonlinear gyrokinetic theory which captures the ion gyroscale, we proposed the wave-kinetic description of weak kinetic-Alfvénic turbulence in a low-β uniform plasma of axisymmetry, which conserves energy (generalized free-energy) and parallel-momentum (generalized helicity). We calculated the stationary power-law solutions corresponding to energy and parallel-momentum cascades using the conformal Zakharov transformation, in both long-wavelength and short-wavelength limits, for both counter-propagating and co-propagating cases. The cascade directions of stationary solutions were identified and further verified by numerical calculations of the wave kinetic equation. Discussions about the relevance of such predictions to the imbalanced solar wind turbulence, the formation of the transition range, and cascade behaviors of helical kinetic-Alfvénic turbulence are given.
Reference: Shen K., Cheng Z. and Qiu Z., arXiv:2508.03478

Author

Mr Kexun Shen (Institute for Fusion Theory and Simulation, School of Physics, Zhejiang University, Hangzhou, People’s Republic of China)

Co-author

Zhiyong Qiu (Institute of Plasma Physics, Chinese Academy of Sciences)

Presentation materials