A possible mechanism for the formation of the source composition of ultra-heavy nuclei in cosmic rays is considered by taking into account the observed results of this composition. This composition indicates that ultra-heavy elements, together with siderophile ones, must have been relatively more ef
โฆ LIBER โฆ
Elemental abundance enhancement in cosmic rays and their relation to interstellar depletion
โ Scribed by S. P. Tarafdar; Krishna M. V. Apparao
- Publisher
- Springer Netherlands
- Year
- 1981
- Tongue
- English
- Weight
- 345 KB
- Volume
- 77
- Category
- Article
- ISSN
- 0004-640X
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Measurements of the flux of helium nuclei in the 24 January, 1971, event and of helium and (C, N, O) nuclei in the 1 September, 1971, event are combined with previous measurements to obtain the relative abundances of helium, (C, N, O), and Fe-group nuclei in these events. These data are then summari