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- W2000903508 abstract "The crystal detectors developed from eight meteorites and two different moon samples (Luna-12 and Luna-16) have been used for the measurement of VH (Fe-group) and VVH galactic nuclei tracks. The partial annealing technique has been used to eliminate tracks formed due to charges around Z < 50. Charge spectrum for galactic nuclei has been drawn for several meteorites and moon crystal detectors after calibration and comparison with tracks developed in unexposed crystal detectors due to known cyclotron/ accelerator heavy ion beams. The Eagle Station and Marjalahti meteorites confirm the existence of 6 Superheavy nuclei also falling in the charge range 110 < Z < 120. The results also indicate an enhancement in the relative abundance of U-group nuclei in the galactic spaces as compared to the U-group nuclei in the solar system which is in agreement with the results of other workers." @default.
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- W2000903508 date "1988-01-01" @default.
- W2000903508 modified "2023-09-30" @default.
- W2000903508 title "Study of VVH galactic nuclei using meteoritic and moon crystal detectors" @default.
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- W2000903508 doi "https://doi.org/10.1016/1359-0189(88)90226-9" @default.
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