| タイトル | Sources of the ultraheavy cosmic rays |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850026555 |
| 著者（英） | Margolis, S. H.; Blake, J. B. |
| 著者所属（英） | Washington Univ. |
| 発行日 | 1985-08-01 |
| 言語 | eng |
| 内容記述 | The suggestions that the source abundances of cosmic ray nuclei heavier then Fe differ significantly from Solar System abundances are not well supported by the data without assuming preferential acceleration. The Solar System abundances of Pb and Bi are split into r-, standard s-, and cyclic 8-process components; the apprarent deficiency of Pb seen in the HEAO-3 Heavy Nuclei Experiment data might indicate an absence of Pb from the recycling 8-process. |
| NASA分類 | SPACE RADIATION |
| レポートNO | 85N34868
OG-7.1-7 |
| 権利 | No Copyright |
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