NON-LINEAR ASTROPHYSICAL DYNAMOS - SOLAR-CYCLE AS A NON-LINEAR OSCILLATION OF GENERAL MAGNETIC-FIELD DRIVEN BY NON-LINEAR DYNAMO AND ASSOCIATED MODULATION OF DIFFERENTIAL-ROTATION-GLOBAL-CONVECTION SYSTEM

被引：62

作者：

YOSHIMURA, H ^{[1
]}

机构：

[1] UNIV TOKYO,DEPT ASTRON,TOKYO 113,JAPAN

来源：

关键词：

D O I：

10.1086/155953

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：692 / 711

页数：20

共 49 条

[1]

[Anonymous], 1969, ASTRON NACHR

[2] THE TOPOLOGY OF THE SUNS MAGNETIC FIELD AND THE 22-YEAR CYCLE [J].

BABCOCK, HW .

[3]

BRAGINSKII S. I., 1964, SOV PHYS JETP, V20, P1462

[4]

Braginsky S.I., 1964, GEOMAGN AERON, V4, P732

[5]

BRAGINSKY SI, 1965, SOV PHYS JETP-USSR, V20, P726

[6] DIFFERENTIAL ROTATION IN STELLAR CONVECTION ZONES [J].

BUSSE, FH .

[7]

Chandrasekhar S., 1961, HYDRODYNAMIC HYDROMA

[8]

DOUGLASS AE, 1919, CLIMATIC CYCLES TREE, P102

[9] NONAXISYMMETRIC CONVECTION IN A ROTATING SPHERICAL SHELL [J].

DURNEY, B .

[10]

DURNEY BR, 1976, BASIC MECHANISMS SOL