Publication Date:
2019-07-13
Description:
In an attempt to match the observed charge spectrum of VVH particles, several source spectra have been constructed from combinations of r- and s-process nuclei. Their propagation has then been followed, allowing for interactions and decay, and comparisons have been made between the calculated near-earth spectra and those observed during high-altitude balloon flights. None of the models yet used leads to good agreement with observation, suggesting either that more complicated models need to be examined, or that different components (for instance the r- and s-process nuclei) have different histories.
Keywords:
SPACE RADIATION
Type:
International Cosmic Ray Conference; Aug 17, 1973 - Aug 30, 1973; Denver, CO
Format:
text
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