Abstract
A set of experiment data on the energy spectra of peak (maximum) flux and fluence values in solar cosmic ray (SCR) events is analysed. It is shown that the proton energy spectra, averaged over events with identical fluences can be described by power law functions of the particle rigidity. The phenomenon of monotonic increase in the averaged spectral index with increase of SCR fluence is described. A classification of SCR events by fluence magnitude is suggested.
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.
