Computer Science
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982p%26ss...30..293h&link_type=abstract
Planetary and Space Science, vol. 30, Mar. 1982, p. 293-305. Research supported by the U.K. Atomic Energy Authority.
Computer Science
6
Current Sheets, Geomagnetic Tail, Magnetic Effects, Magnetic Storms, Magnetospheric Instability, Tearing Modes (Plasmas), Computerized Simulation, Current Density, Fast Fourier Transformations, Magnetohydrodynamic Stability, Magnetospheric Ion Density, Particle Production, Particle Trajectories, Phase-Space Integral, Temporal Distribution
Scientific paper
A geomagnetic tail current-sheet region, two-and-one-half-dimensional particle-mesh computer model is described which features: (1) the efficient solution of Ampere's equation by Fast Fourier techniques, (2) the incorporation of particle sources and sinks, (3) facilities for the simulation of finite width effects, and (4) the optional inclusion of a normal magnetic field component, linking through the sheet. Simulations based on the model show that current sheets with a non-zero normal field component and an infinite width are stable, with the particles tracing out Speiser-like orbits. Although finite-width sheets are unstable with respect to the ion tearing-mode instability, the presence of a normal magnetic field stabilizes the system. The results suggest that a geomagnetic substorm occurs when the normal magnetic field drops below the critical value needed for stability.
Eastwood James W.
Hamilton E. M. J.
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