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Published in Solar Physics, 229, 373-385, 2005. PREDICTIONS OF GALACTIC COSMIC RAY INTENSITY DEDUCED FROM THAT OF SUNSPOT NUMBER P. Lantos, Observatoire de Meudon
| Content Provider | Semantic Scholar |
|---|---|
| Abstract | A new method is proposed to predict cosmic ray intensity and solar modulation parameters. The method is coupled with McNish and Lincoln method, which predicts first smoothed sunspot numbers. The error done is estimated and compared with the same chain of predictions using two other methods developed for US and Russian space applications. The three methods give satisfactory results when applied, for example, to prediction of dose received on-board commercial aeroplane flights. |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | https://previ.obspm.fr/articles/SolPhy-229-373.pdf |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |