ARE THE HIGH-LATITUDE TORSIONAL OSCILLATIONS OF THE SUN REAL

被引:19
作者
LABONTE, BJ
HOWARD, R
机构
[1] CARNEGIE INST WASHINGTON,MT WILSON OBSERV,WASHINGTON,DC 20005
[2] CARNEGIE INST WASHINGTON,LAS CAMPANAS OBSERV,WASHINGTON,DC 20005
关键词
D O I
10.1007/BF00147983
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:373 / 378
页数:6
相关论文
共 5 条
[1]   THE SUN IS OBSERVED TO BE A TORSIONAL OSCILLATOR WITH A PERIOD OF 11 YEARS [J].
HOWARD, R ;
LABONTE, BJ .
ASTROPHYSICAL JOURNAL, 1980, 239 (01) :L33-L36
[2]   SURFACE MAGNETIC-FIELDS DURING THE SOLAR-ACTIVITY CYCLE [J].
HOWARD, R ;
LABONTE, BJ .
SOLAR PHYSICS, 1981, 74 (01) :131-145
[3]   TORSIONAL WAVES ON THE SUN AND THE ACTIVITY CYCLE [J].
LABONTE, BJ ;
HOWARD, R .
SOLAR PHYSICS, 1982, 75 (1-2) :161-178
[4]  
SCHUSSLER M, 1981, ASTRON ASTROPHYS, V94, pL17
[5]   SOLAR-CYCLE LORENTZ FORCE WAVES AND THE TORSIONAL OSCILLATIONS OF THE SUN [J].
YOSHIMURA, H .
ASTROPHYSICAL JOURNAL, 1981, 247 (03) :1102-1112