| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1771318 | Astroparticle Physics | 2008 | 4 Pages |
Abstract
We discuss the reported detection by the MILAGRO experiment of localised hot spots in the cosmic ray arrival distribution and the difficulty of interpreting these observations. A model based on secondary neutron production in the heliotail is shown to fail. An alternative model based on loss-cone leakage through a magnetic trap from a local source region is proposed.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
L.O’C. Drury, F.A. Aharonian,