| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1766847 | Advances in Space Research | 2008 | 6 Pages |
Abstract
PAMELA will be able to measure the high energy tail of the Jovian electrons in the energy range from 50 up to 130Â MeV. Moreover, it will be possible to extract the Jovian component reaccelerated at the solar wind termination shock (above 130Â MeV up to 2Â GeV) from the galactic flux.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
V. Di Felice, M. Casolino, N. De Simone, P. Picozza,