Charge composition of the VVH cosmic ray nuclei in the energy range of 1–2GeV/nucleon: The results of the track investigation in olivine from the Marjalahti pallasite-Reference-Cited by-同舟云学术

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Charge composition of the VVH cosmic ray nuclei in the energy range of 1–2GeV/nucleon: The results of the track investigation in olivine from the Marjalahti pallasite

Published:2009-10 Issue:9-10 Volume:44 Page:898-900
ISSN:1350-4487
Container-title:Radiation Measurements
language:en
Short-container-title:Radiation Measurements

Author:

Bagulya A.V.,Goncharova L.A.,Ivliev A.I.,Kalinina G.V.,Kashkarov L.L.,Konovalova N.S.,Okat'eva N.M.,Polukhina N.G.,Roussetski A.S.,Starkov N.I.,Tsarev V.A.,Vladymyrov M.S.

Publisher

Elsevier BV

Subject

Instrumentation,Radiation

Reference12 articles.

1. Method of determination of charge of cosmic ray nuclei from tracks in olivine crystals from meteorites;Aleksandrov;Kratkie Soobsh. Po Fizike,2008

2. Studies of the charge and energy spectra of the ancient VVH cosmic rays;Bull;Proc. Lunar Sci. Conf.,1978

3. Completely automated measuring complex (PAVICOM) for track-detector data processing;Feinberg;Physics of Particles and Nuclei,2004

4. Physics and Astrophysics. A Section of Key Problems;Ginzburg,1985

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Use of Pattern Recognition Methods in Track Analysis of Solid Detectors;Journal of Physics: Conference Series;2017-01

2. The software peculiarities of pattern recognition in track detectors;AIP Conference Proceedings;2015

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