The Behaviour of Galactic Cosmic-Ray Intensity During Solar Activity Cycle 24

We have studied long-term variations of galactic cosmic-ray (GCR) intensity in relation to the sunspot number (SSN) during the most recent solar cycles. This study analyses the time lag between the GCR intensity and SSN, and hysteresis plots of the GCR count rate against SSN for Solar Cycles 20 – 23...

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Detalles Bibliográficos
Autores principales: Ross, Eddie, Chaplin, William J.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2019
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6383758/
https://www.ncbi.nlm.nih.gov/pubmed/30872867
http://dx.doi.org/10.1007/s11207-019-1397-7

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6383758/
https://www.ncbi.nlm.nih.gov/pubmed/30872867
http://dx.doi.org/10.1007/s11207-019-1397-7

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