DO SOLAR-TYPE STARS HAVE MAGNETIC CORES QUESTIONABLE QUESTION OF STABILITY

被引：30

作者：

DICKE, RH

机构：

来源：

关键词：

D O I：

10.1086/156916

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：898 / 902

页数：5

共 20 条

ACHESON, DJ ;

GIBBONS, MP .

PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 1978, 289 (1363) :459-500

[2]

APPENZELLER I, 1975, ASTRON ASTROPHYS, V40, P397

[3] AN ENERGY PRINCIPLE FOR HYDROMAGNETIC STABILITY PROBLEMS [J].

BERNSTEIN, IB ;

FRIEMAN, EA ;

KRUSKAL, MD ;

KULSRUD, RM .

PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1958, 244 (1236) :17-40

[4]

DEMARQUE P, 1978, COMMUNICATION

DICKE, RH .

[6]

DICKE RH, 1976, SOL PHYS, V47, P475, DOI 10.1007/BF00154759

DICKE, RH .

[8] 12.2 DAY SOLAR ROTATIONAL PERIOD [J].

DICKE, RH .

[9]

DICKE RH, 1978, JAN C P STAT FUT SOL

[10]

Ezer D, 1968, ASTROPHYS LETT, V1, P177