The Butterfly diagram leopard skin pattern

被引:0
作者
Ternullo, Maurizio [1 ]
机构
[1] INAF Osservatorio Astrofis Catania, I-95123 Catania, Italy
来源
PHYSICS OF SUN AND STAR SPOTS | 2011年 / 273期
关键词
Sun: activity; sun: magnetic fields; sun: sunspots;
D O I
10.1017/S1743921311015237
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A time-latitude diagram where spotgroups are given proportional relevance to their area is presented. The diagram reveals that the spotted area distribution is higly dishomogeneous, most of it being concentrated in few, small portions ("knots") of the Butterfly Diagram; because of this structure, the BD may be properly described as a cluster of knots. The description, assuming that spots scatter around the "spot mean latitude" steadily drifting equatorward, is challenged. Indeed, spots cluster around at as many latitudes as knots; a knot may appear at either lower or higher latitudes than previous ones, in a seemingly random way; accordingly, the spot mean latitude abruptly drifts eguatorward or even poleward at any knot; activation, in spite of any smoothing procedure. Preliminary analyses suggest that the activity splits, in any hemisphere, into two or more distinct "activity waves", drifting equatorward at a rate higher than the spot zone as a. whole.
引用
收藏
页码:195 / 199
页数:5
相关论文
共 16 条
[11]  
Ternullo M., 2001, Memorie della Societa Astronomica Italiana, V72, P681
[12]  
Ternullo M, 2010, MSAIS, V14, P202
[13]  
Ternullo M., 2007, MEM SOC ASTRON ITAL, V78, P596
[14]  
Ternullo M., 2010, IAU S, V274, P195
[15]  
Ternullo M., 2008, EL P 12 EUR SOL PHYS
[16]   The butterfly diagram fine structure [J].
Ternullo, Maurizio .
SOLAR PHYSICS, 2007, 240 (01) :153-164