Results of a calibration of olivines from meteorites by means of 238U nuclei at the Bevalac accelerator.

Details Results of a calibration of olivines from meteorites by means of 238U nuclei at the Bevalac accelerator. Results of a calibration of olivines from meteorites by means of 238U nuclei at the Bevalac accelerator.

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jetpl..49..292p&link_type=abstract

JETP Lett., Vol. 49, No. 5, p. 292 - 296

Physics

Meteorites: Cosmic Rays

Scientific paper

The results of a calibration of the sensitivity of olivine crystals from meteorites by means by 238U nuclei at the Bevalac accelerator are reported. It is shown that the group of ancient tracks ≡210 μm long found in 1980 was caused by galactic cosmic rays of the Th-U group. The possibility of an unambiguous identification of a group of anomalously long cosmic-ray tracks, 340 - 360 μm long, is discussed.

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