Abstract
Abstract A series of revised Serential response curves and yield functions have been deduced for the nucleonic and ionizing components of the secondary cosmic radiation at various atmospheric depths, using the most recent data on the primary spectrum and on geomagnetic cut-off rigidities.
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.
