Predicting solar cycle 24 with a solar dynamo model
| dc.creator | Choudhuri, Arnab Rai | |
| dc.creator | Chatterjee, Piyali | |
| dc.creator | Jiang, Jie | |
| dc.date | 2007-01-18 | |
| dc.date.accessioned | 2026-07-07T10:21:32Z | |
| dc.date.available | 2026-07-07T10:21:32Z | |
| dc.description | Whether the upcoming cycle 24 of solar activity will be strong or not is being hotly debated. The solar cycle is produced by a complex dynamo mechanism. We model the last few solar cycles by `feeding' observational data of the Sun's polar magnetic field into our solar dynamo model. Our results fit the observed sunspot numbers of cycles 21-23 extremely well and predict that cycle~24 will be about 35% weaker than cycle~23. | |
| dc.description | 10 pages 1 table 3 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701527 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701527 | |
| dc.identifier | Phys.Rev.Lett.98:131103,2007 | |
| dc.identifier | doi:10.1103/PhysRevLett.98.131103 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/175206 | |
| dc.subject | Astrophysics | |
| dc.title | Predicting solar cycle 24 with a solar dynamo model | |
| dc.type | text |