Relative abundances of 10?Z?26 nuclei in medium energy cosmic rays
- 1 January 1980
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 69 (2) , 461-470
- https://doi.org/10.1007/bf00661930
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- On improvement of charge resolution of cosmic ray particles using a cellulose nitrate plastic detectorNuclear Instruments and Methods, 1979
- The isotopic composition of cosmic rays with Z between 5 and 26The Astrophysical Journal, 1976
- Enhanced abundances of Ca, Ti and Cr in low energy cosmic rays in Skylab experimentNature, 1975
- Composition of heavy cosmic rays from 25 to 180 MeV per atomic mass unitThe Astrophysical Journal, 1974
- Partial Cross-Sections in High-Energy Nuclear Reactions, and Astrophysical Applications. I. Targets WITh Z <= 28. II. Targets Heavier than NickelThe Astrophysical Journal Supplement Series, 1973
- Evidence for Differences in the Energy Spectra of Cosmic Ray NucleiNature Physical Science, 1973
- Steady State of Cosmic-Ray Nuclei—Their Spectral Shape and Path Length at Low EnergiesPhysical Review B, 1967
- Matter Traversed by Low-Energy Cosmic-Ray Nuclei in SpacePhysical Review B, 1966
- Low-Energy Spectrum of Cosmic Rays as an Indicator of Primary Source Characteristics and Interstellar PropagationPhysical Review B, 1965
- On the modulation of cosmic-ray nuclei with Z>2 during their propagationIl Nuovo Cimento (1869-1876), 1964