skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Kinetic and thermodynamic properties of a convecting plasma in a two-dimensional dipole field

Journal Article · · Journal of Geophysical Research
DOI:https://doi.org/10.1029/94JA01452· OSTI ID:166259
 [1];  [2]
  1. Prairie View A&M Univ., TX (United States)
  2. NASA Goddard Space Flight Center, Greenbelt, MD (United States)

Charged particle guiding center motion is considered in the magnetic field of a two-dimensional (`line`) dipole on which is superimposed a small, static, perpendicular electric field. The parallel equation of motion is that of a simple harmonic oscillator for cos{theta}, the cosine of magnetic colatitude. Equations for the perpendicular electric and magnetic drifts are derived as well as their bounce-averaged forms. The latter are solved to yield a bounce-averaged guiding center trajectory, which is the same as that obtained from conservation of magnetic moment {mu}, longitudinal invariant J, and total (kinetic plus electrostatic) energy K. The algebraic simplicity of the trajectory equations is also manifest in the forms of the invariants. An interesting result is that guiding centers drift in such a way that they preserve the values of their equatorial pitch angles and (equivalently) mirror latitudes. The most general Maxwellian form of the equilibrium one-particle distribution function f is constructed from the invariants, and spatially varying density and pressure moments, parallel and perpendicular to the magnetic field, are identified. Much of the paper deals with the more restricted problem in which f is specified as a bi-Maxwellian over a straight line of finite length in the equatorial plane of the dipole and perpendicular to field lines. This might be thought of as specifying a cross-tail ion injection source; the authors formalism then describes the subsequent spatial development. The distribution away from the source is a scaled bi-Maxwellian but one that is cut off at large and small kinetic energies, which depend on position. Density and pressure components are reduced from the values they would have if the total content of individual flux tubes convected intact. The equatorial and meridional variations of density and pressure components are examined and compared systematically for the isotropic and highly anisotropic situations. 22 refs., 10 figs.

OSTI ID:
166259
Journal Information:
Journal of Geophysical Research, Vol. 99, Issue A9; Other Information: PBD: 1 Sep 1994
Country of Publication:
United States
Language:
English

Similar Records

Bounce-averaged Hamiltonian for charged particles in an axisymmetric but nondipolar model magnetosphere
Journal Article · Sat Apr 01 00:00:00 EST 1995 · Journal of Geophysical Research · OSTI ID:166259

Adiabatic particle motion in a nearly drift-free magnetic field: application to the geomagnetic tail
Journal Article · Wed Mar 01 00:00:00 EST 1978 · J. Geophys. Res.; (United States) · OSTI ID:166259

The effects of pressure anisotropy on Birkeland currents in dipole and stretched magnetospheres
Journal Article · Wed Apr 01 00:00:00 EST 1992 · Journal of Geophysical Research; (United States) · OSTI ID:166259