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- W2004106784 abstract "Under the assumption that the solar-flare bombardment of the irradiated grains of gas-rich meteorites occurred about 4.5 b.y. ago on the parent body regoliths at 3 A.U., an estimate of the solar cosmic ray-produced Ne-21 is made by studying etched pyroxene minera separates from both light and dark portions of the gas-rich meteorites Fayetteville and Kapoeta. Excesses of solar cosmic ray Ne-21 were observed in dark portions of these meteorites, after accounting for their galactic cosmic ray Ne-21 production and solar flare Ne-21. In order to produce the estimated solar cosmic ray Ne-21 in the present samples, highly enhanced solar cosmic ray proton fluxes from the ancient sun are required." @default.
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- W2004106784 date "1989-06-01" @default.
- W2004106784 modified "2023-09-26" @default.
- W2004106784 title "Neon isotope studies of Fayetteville and Kapoeta meteorites and clues to ancient solar activity" @default.
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- W2004106784 doi "https://doi.org/10.1016/0016-7037(89)90078-1" @default.
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