Full Modeling and Practical Parameterization of Cosmogenic 10Be Transport for Cosmic-Ray Studies: SOCOL-AERv2-BE Model

115 Astronomy, Space science

This work was partly supported by the Academy of Finland (Projects ESPERAno. 321882 and GERACLIS no. 354280)). The work benefited from the discussions in the framework of the International Space Science Institute (ISSI) team 510 “SEESUP—Solar Extreme Events: Setting Up a Paradigm.” IU acknowledges the opportunity provided by the ISSI visiting fellowship. ER acknowledges the support from SPbU (research project 116234986). TS thanks the Swiss National Science Foundation for supporting this study (Grant numbers 200020E -219166, project AEON) andalso acknowledges the support from theKarbacher Fonds, Graubünden,Switzerland.

CCM SOCOL‐AERv2‐BE used for paper is preserved at link Golubenko, Rozanov, Sukhodolov, and Usos-kin (2021). Matlab code and all files for parameterization are available at Golubenko (2023).

Model runs were performed at the CSC (Finnish National Centre forScience Computing) facilities.