Year-end Sale % OFF 
Abstract
One of the prerequisites for the study of cosmic-ray isotopic composition was the development of detector technology capable of providing measurements of the required precision. This was accomplished during the 1970s, and these technological advances are described in the next section. This description is between different experiments and extrapolation of the data to the cosmic-ray source, unfolding the effects of galactic propagation and solar modulation. The comparison between cosmic-ray source matter and solar-system material is given and several models for the nucleosynthesis and the evolution of cosmic-ray source matter are also presented. (AIP)
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
