Abstract
By using a selective etching technique in olivines from the Marjalahti meteorite, more than 2000 tracks longer than 150 μm have been found to be due to galactic cosmic-ray nuclei of Z > 50. The olivines examined were taken from locations ∼ 5 cm and 8-9 cm below the preatmospheric surfaces of the meteorites, respectively. The data on the track distribution are compared with the known values of the relative abundances of the 50
Cite
CITATION STYLE
Perelygin, V. P., Stetsenko, S. G., Pellas, P., Lhagvasuren, D., Otgonsuren, O., & Jakupi, B. (1977). Long-term averaged abundances of VVH cosmic ray nuclei from studies of olivines from Marjalahti meteorite. Nuclear Track Detection, 1(3–4), 199–205. https://doi.org/10.1016/0145-224X(77)90014-X
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
