Hemispheric sunspot numbers Rn and Rs from 1945-2004:: catalogue and N-S asymmetry analysis for solar cycles 18-23

被引:163
作者
Temmer, M
Rybák, J
Bendík, P
Veronig, A
Vogler, F
Otruba, W
Pötzi, W
Hanslmeier, A
机构
[1] Graz Univ, IGAM Inst Phys, A-8010 Graz, Austria
[2] Astron Inst SAS, Tatranska Lomnica 05960, Slovakia
[3] Graz Univ, Kanzelhohe Solar Observ, IGAM Inst Phys, A-9521 Treffen, Austria
关键词
catalogs; Sun : activity; Sun : sunspots; Sun : photosphere;
D O I
10.1051/0004-6361:20054060
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
From Sunspot drawings provided by the Kanzelhohe Solar Observatory, Austria, and the Skalnate Pleso Observatory, Slovak Republic, we extracted a data catalogue of hemispheric Sunspot Numbers covering the time span 1945-2004. The validated catalogue includes daily, monthly-mean, and smoothed-monthly relative Sunspot numbers for the northern and Southern hemispheres separately and is available for scientific use. These data we then investigated with respect to north-south asymmetries for almost 6 entire solar cycles (Nos. 18-23). For all the cycles studied, we found that the asymmetry based on the absolute asymmetry index is enhanced near the cycle maximum, which contradicts to Previous results that are based on the normalized asymmetry index. Moreover, the weak magnetic interdependence between the two solar hemispheres is confirmed by their self-contained evolution during a cycle. For the time span 1945-2004, We found that the cycle maxima and also the declining and increasing phases are clearly shifted, whereas the minima seem to be in phase for both hemispheres. The asymmetric behavior reveals no obvious connection to either the Sunspot cycle period of similar to 11 - or the magnetic cycle of similar to 22-years. The most striking excess of activity is observed for the northern hemisphere in cycles 19 and 20.
引用
收藏
页码:735 / 743
页数:9
相关论文
共 55 条
[1]   ROTATION OF THE PHOTOSPHERIC MAGNETIC-FIELDS - A NORTH-SOUTH ASYMMETRY [J].
ANTONUCCI, E ;
HOEKSEMA, JT ;
SCHERRER, PH .
ASTROPHYSICAL JOURNAL, 1990, 360 (01) :296-304
[2]  
Atac T, 1996, SOL PHYS, V166, P201, DOI 10.1007/BF00179363
[3]   Flare index during the rising phase of solar cycle 23 [J].
Ataç, T ;
Özgüç, A .
SOLAR PHYSICS, 2001, 198 (02) :399-407
[5]   The periodic behaviour of the North-South asymmetry of sunspot areas revisited [J].
Ballester, JL ;
Oliver, R ;
Carbonell, M .
ASTRONOMY & ASTROPHYSICS, 2005, 431 (02) :L5-L8
[6]   Structure of the maximum phase of solar cycles 21 and 22 [J].
Bazilevskaya, GA ;
Krainev, MB ;
Makhmutov, VS ;
Flückiger, EO ;
Sladkova, AI ;
Storini, M .
SOLAR PHYSICS, 2000, 197 (01) :157-174
[7]   Active longitudes in sunspot activity: Century scale persistence [J].
Berdyugina, SV ;
Usoskin, IG .
ASTRONOMY & ASTROPHYSICS, 2003, 405 (03) :1121-1128
[8]   The Sun's preferred longitudes and the coupling of magnetic dynamo modes [J].
Bigazzi, A ;
Ruzmaikin, A .
ASTROPHYSICAL JOURNAL, 2004, 604 (02) :944-959
[9]   Differential rotation of stable recurrent sunspot groups [J].
Brajsa, R ;
Wöhl, H ;
Vrsnak, B ;
Rudjak, D ;
Sudar, D ;
Rosa, D ;
Hrina, D .
SOLAR PHYSICS, 2002, 206 (02) :229-241
[10]   LARGE-SCALE DISTRIBUTION OF SOLAR MAGNETIC FIELDS [J].
BUMBA, V ;
HOWARD, R .
ASTROPHYSICAL JOURNAL, 1965, 141 (04) :1502-&