Search NASAโŒ• Search

NASA NTRS ยท 19900061864

The generalized diffusion-convection equation

Abstract

Starting from the Boltzmann equation, a transport equation is derived for energetic particles in a moving magnetized plasma in which the scattering centers that keep the particles quasi-isotropic are moving with a velocity that is not necessarily the same as that of the plasma. The scattering is characterized by three very loose constraints: (1) there is a rest frame for each scatterer in which the particles scatter elastically; (2) in this frame the scattering will not disturb an isotropic distribution; and (3) the momentum transfer in an average collision may be described by a tensor operating on the particles original momentum. Since the strength of the scattering is not specified, the derivation should be as valid for plasma microturbulence as for hard-sphere scattering. The results show clearly which phenomena are responsible for tying the particles to the plasma in the transport equation.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Jones, Frank C.. 1990-09-20. The generalized diffusion-convection equation. https://ntrs.nasa.gov/citations/19900061864

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