| タイトル | Implications of source abundances of ultraheavy cosmic rays |
| 著者（英） | Margolis, S. H.; Waddington, C. J.; Binns, W. R.; Klarmann, J.; Israel, M. H.; Garrard, T. L.; Stone, E. C. |
| 著者所属（英） | Minnesota Univ.|Washington Univ.|California Inst. of Tech. |
| 発行日 | 1985-01-01 |
| 言語 | eng |
| 内容記述 | The ratio of cosmic-ray source abundance to solar-system abundance for individual elements is examined. In particular correlations of these ratios with first-ionization potential (FIP) and also with the expected mass-to-charge ratio (A/Q) of the elements in a million-degree plasma are examined. The FIP correlation were previously examined and shown that the correlation is affected by the choice of C2 or C1 chondritic meteorites as the solar-system standard for comparison. An A/Q correlation was suggested by Eichler and Hainebach as a consequence of their model of shock acceleration in the hot interstellar medium, and has been examined by Israel. These correlations are presented. |
| NASA分類 | SPACE RADIATION |
| レポートNO | 85N32049 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/394888 |
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