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

Gyrokinetic simulations of turbulent energy exchange in a dipole configuration

Not scheduled
20m
EICC, Edinburgh

EICC, Edinburgh

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

Speaker

Ryusuke Numata (University of Hyogo)

Description

Planetary magnetospheres and levitated ring dipole devices represent a unique class of plasma environments where high-temperature plasma is confined by strongly inhomogeneous magnetic fields. A defining feature of these systems is the emergence of "entropy-mode" turbulence—driven by magnetic curvature and density gradients—which is responsible for the "inward pinch" phenomenon, where particles are transported against density gradients to achieve high confinement. Recent work in simplified Z-pinch configurations has revealed a novel, non-intuitive process: thermal equilibration between species without the need for collisions.

This study extends the investigation of turbulent energy exchange from the circular Z-pinch prototype to a comprehensive dipole configuration. In the Z-pinch limit, linear stability analysis and nonlinear gyrokinetic simulations using the GS2 code demonstrate that the roles of electrons and ions in destabilizing the system are interchangeable depending on their temperature ratio, Ti/Te[1]. When Ti/Te is not equal to one, one species carries negative energy due to wave-particle resonances, providing the free energy necessary to drive the entropy mode. This instability facilitates a nonlinear energy exchange (turbulent heating/cooling) that pushes the system toward a state of equal temperatures.

In a more complex dipole geometry, the inclusion of variations along magnetic field lines and the full 3D structure of the dipolar field introduces additional complexities, such as the coupling between electrostatic entropy modes and electromagnetic fluctuations (e.g., Alfvén waves). We present new gyrokinetic simulation results that examine how these geometrical factors influence the efficiency of collisionless thermal equilibration. By characterizing these processes in a dipole field, we aim to provide a more consistent explanation for the global self-organization and observed temperature profiles in magnetospheric plasmas. These findings have significant implications for understanding energy transport in space physics and for the design of compact fusion devices based on the dipole confinement concept.

[1] R. Numata, Mon. Not. Roy. Astron. Soc. Lett. (2025).

Author

Ryusuke Numata (University of Hyogo)

Presentation materials