Reduced models accounting for parallel magnetic perturbations: gyrofluid and finite Larmor radius–Landau fluid approaches

TOWARD A THEORY OF ASTROPHYSICAL PLASMA TURBULENCE AT SUBPROTON SCALES

(2013) Stanislav Boldyrev et al.   ASTROPHYSICAL JOURNAL

ENHANCED MAGNETIC COMPRESSIBILITY AND ISOTROPIC SCALE INVARIANCE AT SUB-ION LARMOR SCALES IN SOLAR WIND TURBULENCE

(2012) K. H. Kiyani et al.   ASTROPHYSICAL JOURNAL

On the mirror instability in the presence of electron temperature anisotropy

(2012) E. A. Kuznetsov et al.   PHYSICS OF PLASMAS

A compressible Hamiltonian electromagnetic gyrofluid model

(2011) F.L. Waelbroeck et al.   Communications in Nonlinear Science and Numerical Simulation

Hamiltonian four-field model for magnetic reconnection: nonlinear dynamics and extension to three dimensions with externally applied fields

(2010) E. Tassi et al.   NUCLEAR FUSION

ASTROPHYSICAL GYROKINETICS: KINETIC AND FLUID TURBULENT CASCADES IN MAGNETIZED WEAKLY COLLISIONAL PLASMAS

(2009) A. A. Schekochihin et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES