On the depth-dependent production of radionuclides (44≤A≤59) by solar protons in extraterrestrial matter
- 1 September 1980
- journal article
- physical methods-section
- Published by Springer Nature in Journal of Radioanalytical and Nuclear Chemistry
- Vol. 59 (2) , 467-510
- https://doi.org/10.1007/bf02517298
Abstract
No abstract availableKeywords
This publication has 58 references indexed in Scilit:
- Cosmic ray intensity over long time scalesReviews of Geophysics, 1979
- Proton-induced reactions on titanium with energies between 13 and 45 MeVJournal of Inorganic and Nuclear Chemistry, 1978
- Beryllium-10 Mass Spectrometry with a CyclotronScience, 1978
- The age of the galactic cosmic rays derived from the abundance of Be-10The Astrophysical Journal, 1977
- On the flux of low-energy particles in the solar system: The record in St. Séverin meteoriteNuclear Track Detection, 1977
- Be-10 abundance and the age of cosmic rays - A balloon measurementThe Astrophysical Journal, 1977
- Reaction List for charged-particle-induced nuclear reactions: Z = 1 to Z = 98 (H to Cf), October 1974–January 1976Atomic Data and Nuclear Data Tables, 1976
- Heavy Cosmic Ray NucleiAnnual Review of Nuclear Science, 1970
- Formation cross sections of various radionuclides from Ni, Fe, Si, Mg, O and C for protons of energies between 0·5 and 2·9 GeVJournal of Inorganic and Nuclear Chemistry, 1968
- () and () Cross Sections in Medium Weight ElementsPhysical Review B, 1955