| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1764649 | Advances in Space Research | 2012 | 14 Pages |
Abstract
It seems that a essential part of the radiation belt temporal dynamics during magnetic storms may be explained by the change of the magnetic field configuration and the adiabatic effects. Together with the nonadiabatic radial diffusion it results in the radial displacement of the outer radiation belt rather than the large losses or total disappearance of the outer radiation belt.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
L.L. Lazutin,