Published May 9, 2018 | Version v1

On the structure of the drifton phase space and its relation to the Rayleigh–Kuo criterion of the zonal-flow stability

  • 1. Princeton University and Princeton Plasma Physics Laboratory
  • 2. Princeton Plasma Physics Laboratory

Description

These are the supplementary data that can be used to generate figure 3, 4, and 5 in the manuscript "On the structure of the drifton phase space and its relation to the Rayleigh--Kuo criterion of the zonal-flow stability". The abstract of this manuscript reads as follows:

The phase space of driftons (drift-wave quanta) is studied within the generalized Hasegawa--Mima collisionless-plasma model in the presence of zonal flows. This phase space is made intricate by the corrections to the drifton ray equations that were recently proposed by Parker [J. Plasma Phys. 82, 595820602 (2016)] and Ruiz et al. [Phys. Plasmas 23, 122304 (2016)]. Contrary to the traditional geometrical-optics (GO) model of the drifton dynamics, it is found that driftons can be not only trapped or passing, but they can also accumulate spatially while experiencing indefinite growth of their momenta. In particular, it is found that the Rayleigh--Kuo threshold known from geophysics corresponds to the regime when such "runaway" trajectories are the only ones possible. On one hand, this analysis helps visualize the development of the zonostrophic instability, particularly its nonlinear stage, which is studied here both analytically and through wave-kinetic simulations. On the other hand, the GO theory predicts that zonal flows above the Rayleigh--Kuo threshold can only grow; hence, the deterioration of intense zonal flows cannot be captured within a GO model. In particular, this means that the so-called tertiary instability of intense zonal flows cannot be adequately described within the quasilinear wave kinetic equation, contrary to some previous studies.

Files

Files (1.3 MB)

Name Size Download all
md5:7573c24fae039a83e257b89018a3c268
420.8 kB Download
md5:4ebf30ee1752db1433234b40a13d9137
418.0 kB Download
md5:2028ba3be64408f9ddddad8eb955b62a
420.8 kB Download

Additional details

Related works

Is cited by
10.1063/1.5039652 (DOI)
arXiv:1805.04086 (arXiv)