THE 22-YEAR CYCLE OF THE SUN

被引:3
作者
KUNDT, W
机构
关键词
D O I
10.1007/BF00642688
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The 22-yr solar cycle is being explained as due to a spin-aligned magnetic quadrupole frozen into the (radiative) core. Differential rotation of the poorly conducting convection zone gives rise to flux winding and to an alternating dominance, near the surface, of one of the two constituent dipoles. Equatorial superrotation and polar subrotation are stabilized by the same magnetic flux that transfers angular momentum from the (radiative) core to the (escaping) solar wind. The time- and radius-dependent magnetic torque is also responsible for the rigid and twisting oscillations of a thin surface layer, and for the relative velocities of different tracers.
引用
收藏
页码:75 / 85
页数:11
相关论文
共 57 条
[1]   HIGH-RESOLUTION MAPPING OF MAGNETIC-FIELD OF SOLAR CORONA [J].
ALTSCHULER, MD ;
LEVINE, RH ;
STIX, M ;
HARVEY, J .
SOLAR PHYSICS, 1977, 51 (02) :345-375
[2]  
[Anonymous], INTERNAL SOLAR ANGUL
[3]   ANGULAR VELOCITY DISTRIBUTION IN CONVECTIVE REGIONS AND THE ORIGIN OF SOLAR DIFFERENTIAL ROTATION [J].
BISNOVATYIKOGAN, GS .
SOLAR PHYSICS, 1990, 128 (01) :299-304
[4]  
BLOME HJ, 1988, ASTROPHYS SPACE SCI, V148, P343, DOI 10.1007/BF00645969
[5]   RECURRENCE OF SOLAR-ACTIVITY - EVIDENCE FOR ACTIVE LONGITUDES [J].
BOGART, RS .
SOLAR PHYSICS, 1982, 76 (01) :155-165
[6]   THE SOLAR-CYCLE - A CENTRAL-SOURCE WAVE THEORY [J].
BRACEWELL, RN .
PROCEEDINGS ASTRONOMICAL SOCIETY OF AUSTRALIA, 1989, 8 (02) :145-147
[7]  
BRANDENBURG A, 1990, THESIS HELSINKI
[8]   TURBULENT POWER AND DISSIPATION IN THE SOLAR TRANSITION ZONE [J].
DERE, KP .
ASTROPHYSICAL JOURNAL, 1989, 340 (01) :599-606
[9]   IS THE SOLAR OBLATENESS VARIABLE - MEASUREMENTS OF 1985 [J].
DICKE, RH ;
KUHN, JR ;
LIBBRECHT, KG .
ASTROPHYSICAL JOURNAL, 1987, 318 (01) :451-458
[10]   THE TOROIDAL MAGNETIC-FIELD INSIDE THE SUN [J].
DZIEMBOWSKI, WA ;
GOODE, PR .
ASTROPHYSICAL JOURNAL, 1989, 347 (01) :540-550