A Dynamical Model for the Onset of Magnetospheric Substorms.
Abstract
A model for the onset of magnetospheric substorms is developed based on the observations of Pytte et al (1976). North-south single-particle motion across the plasma sheet becomes instrumental in generating magnetic instabilities when the plasma sheet is sufficiently compressed. The number density times the square of the plasma sheet thickness is found to be the critical parameter (nl squared less than or equal to 8.1 x 10 to the 15th power protons/cm). A merging theory is developed based on these magnetic instabilities. The nightside merging rate is controlled by the value of the magnetic field in the tail lobes which, in turn, is dependent on the dayside merging rate. Merging and collisional damping of the J X B force contribute to the heating of the plasma sheet. The 10-15 min interval between onsets is interpreted in terms of a weak coupling between the tail lobes and the plasma sheet. A straightforward application of small-amplitude oscillation theory shows that the period between onsets is a direct measure of the mean collision frequency in the plasma sheet. The obtained value is in good agreement with that calculated from the resistivity relation. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Dec 13, 1978
- Accession Number
- ADA072987
Entities
People
- G. K. Yates
- P. L. Rothwell
Organizations
- Air Force Research Laboratory