Published 1985
| Version v1
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Search for the tracks of heavy and superheavy cosmic ray nuclei in olivines from meteorites
Description
The results of investigating the tracks of cosmic nuclei with Z >= 50 in olivine crystals from meteorites are presented. The obtained spectrum of track lengths for the Z >= 50 nuclei exhibits two pronounced groups of tracks: 190-230 μm tracks, attributed to nuclei ranging from Th to U, and abnormally long 310-360 μm tracks. The hypothesis that the nuclei of superheavy elements with Z >= 110 may be present in cosmic rays is discussed
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17000912.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 7 p.
- Report number
- JINR-E--7-85-245
INIS
- Country of Publication
- USSR
- Country of Input or Organization
- USSR
- INIS RN
- 17000912
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC NUCLEI; ELEMENT ABUNDANCE; METEORITES; OLIVINE; TRANS 104 ELEMENTS; TRANSURANIUM ELEMENTS
- Descriptors DEC
- COSMIC RADIATION; ELEMENTS; IONIZING RADIATIONS; MINERALS; NUCLEI; PRIMARY COSMIC RADIATION; QUANTITY RATIO; RADIATIONS; SILICATE MINERALS; TRANSPLUTONIUM ELEMENTS
Optional Information
- Notes
- 21 refs.; 2 figs.