TY - JOUR

T1 - Collisionless distribution functions for force-free current sheets: using a pressure transformation to lower the plasma beta

AU - Wilson, F.

AU - Neukirch, T.

AU - Allanson, O.

PY - 2018/6

Y1 - 2018/6

N2 - So far, only one distribution function giving rise to a collisionless nonlinear force-free current sheet equilibrium allowing for a plasma beta less than one is known (Allanson et al., Phys. Plasmas, vol. 22 (10), 2015, 102116; Allanson et al., J. Plasma Phys., vol. 82 (3), 2016a, 905820306). This distribution function can only be expressed as an infinite series of Hermite functions with very slow convergence and this makes its practical use cumbersome. It is the purpose of this paper to present a general method that allows us to find distribution functions consisting of a finite number of terms (therefore easier to use in practice), but which still allow for current sheet equilibria that can, in principle, have an arbitrarily low plasma beta. The method involves using known solutions and transforming them into new solutions using transformations based on taking integer powers ( N ) of one component of the pressure tensor. The plasma beta of the current sheet corresponding to the transformed distribution functions can then, in principle, have values as low as 1/N . We present the general form of the distribution functions for arbitrary N and then, as a specific example, discuss the case for N=2 in detail.

AB - So far, only one distribution function giving rise to a collisionless nonlinear force-free current sheet equilibrium allowing for a plasma beta less than one is known (Allanson et al., Phys. Plasmas, vol. 22 (10), 2015, 102116; Allanson et al., J. Plasma Phys., vol. 82 (3), 2016a, 905820306). This distribution function can only be expressed as an infinite series of Hermite functions with very slow convergence and this makes its practical use cumbersome. It is the purpose of this paper to present a general method that allows us to find distribution functions consisting of a finite number of terms (therefore easier to use in practice), but which still allow for current sheet equilibria that can, in principle, have an arbitrarily low plasma beta. The method involves using known solutions and transforming them into new solutions using transformations based on taking integer powers ( N ) of one component of the pressure tensor. The plasma beta of the current sheet corresponding to the transformed distribution functions can then, in principle, have values as low as 1/N . We present the general form of the distribution functions for arbitrary N and then, as a specific example, discuss the case for N=2 in detail.

KW - astrophysical plasmas

KW - space plasma physics

U2 - 10.1017/S0022377818000570

DO - 10.1017/S0022377818000570

M3 - Article

SN - 0022-3778

VL - 84

JO - Journal of Plasma Physics

JF - Journal of Plasma Physics

IS - 3

M1 - 905840309

ER -