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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...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Springer Netherlands
2019
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| 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 |