The elemental and isotopic composition of cosmic rays - Silicon to nickel
Citations Over TimeTop 10% of 1981 papers
Abstract
The reported observations were made with the aid of the Cosmic Ray Isotope Instrument System (CRISIS) which had been designed to detect and resolve the isotopes of cosmic ray nuclei with atomic numbers equal to or greater than 10. The CRISIS detector was flown on a balloon launched from Aberdeen, South Dakota on 1977 May 20. The period 1977 May 19-22 has been classified by Mason et al. (1979) as one of 'superquiet' solar activity, characterized by the lowest fluxes of low-energy solar particles ever observed. The obtained results are presented in a number of graphs and tables. It was found that the elemental and isotopic abundances of Si are solar-like. Elemental S is underabundant in the cosmic rays by a factor of approximately 3 relative to the solar system, but its isotopic composition resembles the solar composition with S-32 being the dominant isotope. Elemental Ar is virtually absent in the source, and the observed isotopic composition is consistent with a secondary origin. Elemental Ni has a solar-like abundance.
Related Papers
- → Short-Lived Radioactivities and the Birth of the sun(2000)138 cited
- Short-lived nuclei in the early solar system(1985)
- → 2. Evidence for 26Al in the Solar System(1977)5 cited
- → Evidence in meteorites for the presence of 41Ca in the early solar system(1995)
- Organics and Ices in the Outer Solar System: Connections to the Interstellar Medium(2017)