The role of parametric instabilities in turbulence generation and proton heating: Hybrid simulations of parallel propagating Alfv\'en waves
C.A. Gonz\'alez, A. Tenerani, M. Velli, P. Hellinger

TL;DR
This study uses multi-dimensional hybrid simulations to explore how parametric instabilities of large-amplitude Alfvén waves lead to turbulence and proton heating, revealing persistent decay processes at high plasma beta and their role in plasma heating.
Contribution
It demonstrates that decay processes in Alfvén waves persist in multi-dimensions at high plasma beta, unlike in 1D, and links these processes to turbulence development and proton heating mechanisms.
Findings
Decay persists at high plasma beta in multi-dimensions
Decay triggers perpendicular turbulent cascade
Saturated state shows field-aligned proton beams and increased temperatures
Abstract
Large amplitude Alfv\'en waves tend to be unstable to parametric instabilities which result in a decay process of the initial wave into different daughter waves depending upon the amplitude of the fluctuations and the plasma beta. The propagation angle with respect to the mean magnetic field of the daughter waves plays an important role in determining the type of decay. In this paper, we revisit this problem by means of multi-dimensional hybrid simulations. In particular, we study the decay and the subsequent nonlinear evolution of large-amplitude Alfv\'en waves by investigating the saturation mechanism of the instability and its final nonlinear state reached for different wave amplitudes and plasma beta conditions. As opposed to one-dimensional simulations where the Decay instability is suppressed for increasing plasma beta values, we find that the decay process in multi-dimensions…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Ocean Waves and Remote Sensing
