首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Solar Variability Induced in a Dynamo Code by Realistic Meridional Circulation Variations
Authors:I Lopes  D Passos
Institution:(1) CENTRA, Departamento de Física, Instituto Superior Técnico, Av. Rovisco Pais, 1049-001 Lisboa, Portugal;(2) Departamento de Física, Universidade de évora, Colégio António Luis Verney, 7002-554 évora, Portugal
Abstract:In this work we use an already-published method to infer a variation profile for the solar meridional circulation over the last 250 years. We feed this variation profile into a numerical dynamo code, and we reconstruct a sunspot time series that acts as a proxy for solar cycle activity. We perform three simulations with slightly different parameters, and the results are compared with the observational data. The medium and large correlation coefficients between reconstructed and observational time series seem to indicate that variations in meridional circulation play an important role in the modulation of solar activity.
Keywords:Solar cycle: models  Sunspots: magnetic fields  Sunspots: statistics
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号