The Rotation Rate of the Active Longitude and Sunspot Groups on It and Other Characteristics of Sunspot Groups at the End of the Descending Branch of Solar Cycle 24

被引：0
作者：
I. G. Kostyuchenko
E. S. Vernova
机构：
[1] Karpov Institute of Physical Chemistry,
[2] St. Petersburg Branch,undefined
[3] Pushkov Institute of Terrestrial Magnetism,undefined
[4] the Ionosphere,undefined
[5] and Radio Wave Propagation,undefined
[6] Russian Academy of Sciences,undefined
来源：
Geomagnetism and Aeronomy | 2023年 / 63卷
关键词：
solar activity; sunspots; active longitudes; solar magnetic fields; Sun: rotation;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
引用
收藏
页码：1210 / 1217
页数：7
相关论文
共 53 条
[1]  
Bassom A.P.(2005)Non-axisymmetric α Geophys. Astrophys. Fluid Dyn. 99 309-336
[2]  
Kuzanyan K.M.(2006)Ω-dynamo waves in thin stellar shells Ser. Fiz. 70 1413-1416
[3]  
Sokoloff D.(2012)Variations in the structure and rotation of the convection zone with the cycle phase and their connection with the dynamics of magnetic fields, Adv. Space Res. 50 656-L166
[4]  
Soward A.M.(1999)Synoptic magnetic field in cycle 23 and in the beginning of the cycle 24 Astrophys. J. 517 L163-1128
[5]  
Benevolenskaya E.E.(2003)The interaction of new and old magnetic fluxes at the beginning of solar cycle 23 Astron. Astrophys. 405 1121-714
[6]  
Kosovichev A.G.(2006)Active longitudes in sunspot activity: Century scale persistence Astron. Astrophys. 445 703-L196
[7]  
Benevolenskaya E.E.(2004)Active longitudes, nonaxisymmetric dynamos and phase mixing Astrophys. J. 604 944-1422
[8]  
Ponyavin D.I.(2005)The Sun’s preferred longitudes and the coupling of magnetic dynamo modes Astrophys. J. 635 L193-5166
[9]  
Benevolenskaya E.E.(2022)A shallow-water theory for the Sun’s active longitudes Astrophys. J. 937 41-224
[10]  
Hoeksema J.T.(2006)Spatial scales and time variation of solar subsurface convection Ser. Fiz. 70 1417-5323
123456