Abstract
We present measurements of neon isotopic abundances from the ACE-CRIS experiment. These abundances have been obtained in seven energy intervals over the energy range of ~80≤E≤280 MeV/nucleon. We find that the 22 Ne/ 20 Ne abundance ratio at the cosmic-ray source is a factor of 5.0±0.2 greater than for the solar wind. These measured abundances agree well with previous experiments. The significance of these results is discussed.
Original language | English (US) |
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Pages (from-to) | 767-772 |
Number of pages | 6 |
Journal | Advances in Space Research |
Volume | 27 |
Issue number | 4 |
DOIs | |
State | Published - 2001 |
ASJC Scopus subject areas
- Aerospace Engineering
- Astronomy and Astrophysics
- Geophysics
- Atmospheric Science
- Space and Planetary Science
- General Earth and Planetary Sciences