Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1777494 | Journal of Atmospheric and Solar-Terrestrial Physics | 2009 | 20 Pages |
Abstract
Use of a magnetospheric model suggests that a change in the character of the particle fluxes in the afternoon sector around the time of transition between slow and fast wind was due to the field lines being pulled back into the tail at a time when the pressure exerted by the solar wind was at its greatest.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
M.J. Birch, J.K. Hargreaves, B.J.I. Bromage, D.S. Evans,