GALAXY FORMATION WITHOUT PRIMORDIAL TURBULENCE - MECHANISMS FOR GENERATING COSMIC VORTICITY

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 168:1 (1974) 73-92

A solvable model of Vlasov-kinetic plasma turbulence in Fourier-Hermite phase space

Journal of Plasma Physics Cambridge University Press

Authors:

T Adkins, AA Schekochihin

Abstract:

A class of simple kinetic systems is considered, described by the 1D Vlasov--Landau equation with Poisson or Boltzmann electrostatic response and an energy source. Assuming a stochastic electric field, a solvable model is constructed for the phase-space turbulence of the particle distribution. The model is a kinetic analog of the Kraichnan--Batchelor model of chaotic advection. The solution of the model is found in Fourier--Hermite space and shows that the free-energy flux from low to high Hermite moments is suppressed, with phase mixing cancelled on average by anti-phase-mixing (stochastic plasma echo). This implies that Landau damping is an ineffective dissipation channel at wave numbers below a certain cut off (analog of Kolmogorov scale), which increases with the amplitude of the stochastic electric field and scales as inverse square of the collision rate. The full Fourier--Hermite spectrum is derived. Its asymptotics are $m^{-3/2}$ at low wave numbers and high Hermite moments ($m$) and $m^{-1/2}k^{-2}$ at low Hermite moments and high wave numbers ($k$). The energy distribution and flows in phase space are a simple and, therefore, useful example of competition between phase mixing and nonlinear dynamics in kinetic turbulence, reminiscent of more realistic but more complicated multi-dimensional systems that have not so far been amenable to complete analytical solution.

An analytical theory for the resolution attainable using eclipse mapping of exoplanets

Monthly Notices of the Royal Astronomical Society 528:1 (2024) 596鈥�607

Authors:

Sasha Boone, David Grant, Mark Hammond

Abstract:

We present an analytical theory for the resolution attainable via eclipse mapping of exoplanets, based on the Fourier components of the brightness distribution on the planetary disc. We find that the impact parameter determines which features can and cannot be seen, via the angle of the stellar edge relative to the axis of the orbit during the eclipse. We estimate the signal-to-noise ratio as a function of mapping resolution, and use this to determine the attainable resolution for a given star鈥損lanet system. We test this theory against numerical simulations and find good agreement; in particular, our predictions for the resolution as a function of stellar edge angle are accurate to the simulated data to within 10 per鈥塩ent over a wide range of angles. Our prediction for the number of spatial modes that can be constrained given a light-curve error is similarly accurate. Finally, we give a list of exoplanets with the best expected resolution for observations with the NIRISS SOSS, NIRSpec G395H, and MIRI LRS instruments on JWST.

CoRoT 223992193: Investigating the variability in a low-mass, pre-main sequence eclipsing binary with evidence of a circumbinary disk

Astronomy and Astrophysics Springer Verlag

Authors:

E Gillen, S Aigrain, Caroline Terquem, J Bouvier, SHP Alencar, D Gandolfi, J Stauffer, A Cody, L Venuti, PV Almeida, G Micela, F Favata, HJ Deeg

Collisionality scaling of the electron heat flux in ETG turbulence

Plasma Physics and Controlled Fusion IOP Publishing: Hybrid Open Access

Authors:

GJ Colyer, AA Schekochihin, FI Parra, CM Roach, MA Barnes, Y-C Ghim, W Dorland

Abstract:

In electrostatic simulations of MAST plasma at electron-gyroradius scales, using the local flux-tube gyrokinetic code GS2 with adiabatic ions, we find that the long-time saturated electron heat flux (the level most relevant to energy transport) decreases as the electron collisionality decreases. At early simulation times, the heat flux "quasi-saturates" without any strong dependence on collisionality, and with the turbulence dominated by streamer-like radially elongated structures. However, the zonal fluctuation component continues to grow slowly until much later times, eventually leading to a new saturated state dominated by zonal modes and with the heat flux proportional to the collision rate, in approximate agreement with the experimentally observed collisionality scaling of the energy confinement in MAST. We outline an explanation of this effect based on a model of ETG turbulence dominated by zonal-nonzonal interactions and on an analytically derived scaling of the zonal-mode damping rate with the electron-ion collisionality. Improved energy confinement with decreasing collisionality is favourable towards the performance of future, hotter devices.