The results of measurements of cosmogenic radionuclides in the Peace River and Harleton chondrites shortly after their falls are reported. Activity ratios of short- and long-lived nuclides are compared with ratios observed in other freshly fallen meteorites. Long-term temporal constancy of the cosmic-ray flux within 50% is supported, and a spatial variation of cosmic radiation of less than a factor of 2 throughout meteoritic orbits is indicated. The 11-year solar cycle does not appear to have had any significant effect on activities with half-lives of the order of about a year, such as Mn54 and Na22, except for Co60 in Harleton, which seems to be high in our specimen as a result of solar-particle effects. The activities are compared with thick-target production cross sections.
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Shedlovsky et al. (1967) studied this question.
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