Search NASA⌕ Search

NASA NTRS · 19770036157

High-beta turbulence in two-dimensional magnetohydrodynamics

Abstract

Equations of ideal magnetohydrodynamics are used to study incompressible turbulent flows in a specified geometry where all the field quantities vary with only two spatial dimensions. The procedures adopted are basically those of Kraichnan (1967), in which classical equilibrium ensembles are built around constants of the motion identified from the Fourier-transformed equations of motion. Once the constants of the motion are identified, the statistical formulation of the problem is presented in a phase space whose coordinates are the real and imaginary parts of the Fourier coefficients. Canonical ensembles are constructed in this phase space by classical arguments. The theory developed permits isolation of some qualitatively new gross physical effects which have so far not been calculated. One of the more novel physical effects is the appearance of macroscopic structures involving long-wavelength, self-generated, magnetic fields for a wide range of initial parameters.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Fyfe, D., Montgomery, D.. 1976-10-01. High-beta turbulence in two-dimensional magnetohydrodynamics. https://ntrs.nasa.gov/citations/19770036157

Cite the original work for its findings. Save a collection to share your selection of sources.