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- W3081034748 abstract "Transmission electron microscope study of the track density gradients and irradiation geometries of track-rich grains and chondrules in sections of Fayetteville and Kapoeta, and in sections of lunar breccias and grains from lunar soil. A substantial fraction (50 to 90%) of the meteoritic track-rich grains and chondrules show evidence of having been irradiated anisotropically in their different faces, as would be expected for irradiation on the surface of a parent body. The observations thus support the hypothesis that the irradiation of these grains and chondrules took place on the regoliths of asteroidal-sized bodies. Measurements of steepest track density gradients indicate that, while there are finite differences between spectra exhibited by individual gas-rich meteorites, the average solar flare spectral shapes have been similar over the last 4 b.y. or so." @default.
- W3081034748 created "2020-09-01" @default.
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- W3081034748 date "1974-05-01" @default.
- W3081034748 modified "2023-09-28" @default.
- W3081034748 title "On the Irradiation History and Origin of Gas-Rich Meteorites." @default.
- W3081034748 hasPublicationYear "1974" @default.
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