2010/08/01 by Bidya Binay Karak, Arnab Rai Choudhuri
Biochemistry, Genetics and Molecular Biology · Chemistry · Earth and Planetary Sciences · Physics and Astronomy · #Amplitude #Chemistry #Climatology #Dynamo #Flux (metallurgy) #Geology #Geomagnetism and Paleomagnetism Studies #Geophysics and Gravity Measurements #Magnetic field #Physics #Solar and Space Plasma Dynamics #astro-ph.EP #astro-ph.HE #astro-ph.SR
paper · pdf · doi:10.1017/s1743921311015705
published as The Physics of Sun and Star Spots, Proceedings of the International Astronomical Union, IAU Symposium, 273, 430 (2011) · 4 pages, 2 figures, Proceedings of IAU symposium 273, Physics of Sun and star spots, Ventura, California 22-26 August 2010
openalex publication_date 2010/08/01 · arxiv created 2011/01/23 · arxiv updated 2015/06/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Abstract We propose that at the beginning of the Maunder minimum the poloidal field or amplitude of meridional circulation or both fell abruptly to low values. With this proposition, a flux transport dynamo model is able to reproduce various important aspects of the historical records of the Maunder minimum remarkably well.