The cosmic ray ground level enhancement (GLE) of December 7-8, 1982, occurred when the interplanetary magnetic field (IMF) direction measured near Earth indicated significant distortion from the nominal form. We have modeled the ground level response to this event to derive rigidity spectra and pitch angle distributions centered on apparent arrival directions. A deficit region associated with a near-Earth magnetic cloud-like structure has been modeled during the initial phase of the GLE. Using this modified model, we find agreement between the derived particle arrival directions and the measured IMF directions. We find a significant contribution from pitch angles greater than 90° throughout the event. This is probably due to scattering in the turbulent region behind the cloud-like structure. Copyright 1997 by the American Geophysical Union.
History
Publication title
Journal of Geophysical Research-Space Physics
Volume
102
Issue
A3
Pagination
4919-4925
ISSN
0148-0227
Department/School
School of Natural Sciences
Publisher
American Geophysical Union
Publication status
Published
Place of publication
Washington
Socio-economic Objectives
280120 Expanding knowledge in the physical sciences