Solar Wind Gases, Cosmic Ray Spallation Products, and the Irradiation History

Details Solar Wind Gases, Cosmic Ray Spallation Products, and the Irradiation History Solar Wind Gases, Cosmic Ray Spallation Products, and the Irradiation History

Jan 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970sci...167..548m&link_type=abstract

Science, Volume 167, Issue 3918, pp. 548-550

Computer Science

6

Scientific paper

The isotopic abundances of the rare gases in the fines are found to be similar to those previously reported for gas-rich meteorites. Relative to the heavy gases, neon and helium are depleted by factors of 2.5 and 10 respectively. Accurate krypton-krypton ages for rocks 10017, 10047, 10057, and 10071 were obtained covering a range of from 47 to 509 × 106 years. Varying relative production rates of the krypton and xenon isotopes in these rocks suggest different irradiation conditions and a complex history for at least some of the rocks.

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