SOLAR VARIABILITY AS A MANIFESTATION OF THE SUNS MOTION

被引:19
作者
CHARVATOVA, I
STRESTIK, J
机构
[1] Geophysical Institute Czechoslovak Academy of Sciences Bočńi II 1401
来源
JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS | 1991年 / 53卷 / 11-12期
关键词
D O I
10.1016/0021-9169(91)90047-B
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
Based on records of solar activity available for the last two millenia, the relationship between the motion of the Sun around the barycentre, or centre of mass, of the solar system and the variability of solar activity was studied. The results indicate that the motion of the Sun could be the source of solar variability.
引用
收藏
页码:1019 / 1025
页数:7
相关论文
共 18 条
[1]  
ANDERSON AP, 1980, ANAL TIME SERIES
[2]  
BERGER A, 1984, JUN P WORKSH MEUD
[3]  
BRIER GW, 1961, SOLAR VARIATIONS CLI, P173
[5]  
Charvatova I., 1988, Advances in Space Research, V8, P147, DOI 10.1016/0273-1177(88)90184-6
[6]  
CHARVATOVA I, 1990, B ASTRON I CZECH, V41, P56
[7]  
CHARVATOVA I, 1990, B ASTRON I CZECH, V41, P200
[8]  
CHARVATOVA I, 1991, B ASTRON I CZECH, V42, P90
[9]   LONG-TERM PERIODICITIES IN SUNSPOT CYCLE [J].
COHEN, TJ ;
LINTZ, PR .
NATURE, 1974, 250 (5465) :398-400
[10]   NUMERICAL CALCULATION OF FREQUENCY-TIME DISPLAYS USING AMPLITUDE-TIME RECORDS [J].
DOBES, K ;
STRESTIK, J ;
PRIKNER, K .
STUDIA GEOPHYSICA ET GEODAETICA, 1971, 15 (3-4) :331-&