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

Title: Extending the radial diffusion model of Falthammar to non-dipole background field

Technical Report ·
DOI:https://doi.org/10.2172/1182627· OSTI ID:1182627
 [1]
  1. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

A model for radial diffusion caused by electromagnetic disturbances was published by Falthammar (1965) using a two-parameter model of the disturbance perturbing a background dipole magnetic field. Schulz and Lanzerotti (1974) extended this model by recognizing the two parameter perturbation as the leading (non--dipole) terms of the Mead Williams magnetic field model. They emphasized that the magnetic perturbation in such a model induces an electric ield that can be calculated from the motion of field lines on which the particles are ‘frozen’. Roederer and Zhang (2014) describe how the field lines on which the particles are frozen can be calculated by tracing the unperturbed field lines from the minimum-B location to the ionospheric footpoint, and then tracing the perturbed field (which shares the same ionospheric footpoint due to the frozen -in condition) from the ionospheric footpoint back to a perturbed minimum B location. The instantaneous change n Roederer L*, dL*/dt, can then be computed as the product (dL*/dphi)*(dphi/dt). dL*/Dphi is linearly dependent on the perturbation parameters (to first order) and is obtained by computing the drift across L*-labeled perturbed field lines, while dphi/dt is related to the bounce-averaged gradient-curvature drift velocity. The advantage of assuming a dipole background magnetic field, as in these previous studies, is that the instantaneous dL*/dt can be computed analytically (with some approximations), as can the DLL that results from integrating dL*/dt over time and computing the expected value of (dL*)^2. The approach can also be applied to complex background magnetic field models like T89 or TS04, on top of which the small perturbations are added, but an analytical solution is not possible and so a numerical solution must be implemented. In this talk, I discuss our progress in implementing a numerical solution to the calculation of DL*L* using arbitrary background field models with simple electromagnetic perturbations.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Laboratory Directed Research and Development (LDRD) Program
DOE Contract Number:
AC52-06NA25396
OSTI ID:
1182627
Report Number(s):
LA-UR-15-23879
Country of Publication:
United States
Language:
English

Similar Records

Modification of the Loss Cone for Energetic Particles in the Earth's Inner Magnetosphere
Journal Article · Thu Jul 21 00:00:00 EDT 2022 · Journal of Geophysical Research. Space Physics · OSTI ID:1182627

Magnetospheric signature of some F layer positive storms
Journal Article · Fri May 01 00:00:00 EDT 1981 · J. Geophys. Res.; (United States) · OSTI ID:1182627

The Effects of Localized Thermal Pressure on Equilibrium Magnetic Fields and Particle Drifts in The Inner Magnetosphere
Journal Article · Fri May 31 00:00:00 EDT 2019 · Journal of Geophysical Research. Space Physics · OSTI ID:1182627