Dependence of cosmic ray component in background of atmosphere surface from solar magnetic activity
Using Geant4 toolkit the changes of the flux density and of the dose rates of the secondary cosmic radiation at the heights up to 50 m from the land surface (at a depth of atmosphere about 1030 g/cm²) and depending on solar magnetic activity were estimated. For changes of Wolf’s number (sunspots) in...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
KamGU by Vitus Bering
2021-04-01
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| Series: | Vestnik KRAUNC: Fiziko-Matematičeskie Nauki |
| Subjects: | |
| Online Access: | http://krasec.ru/zelinskiy-34/ |