RELATION BETWEEN CORONAL LAMBDA-5303 INTENSITY, RECURRENT GEOMAGNETIC STORMS, AND SOLAR SECTOR STRUCTURE

被引：13

作者：

GULBRANDSEN, A ^{[1
]}

机构：

[1] NORWEGIAN INST COSMIC PHYS, BLINDERN, OSLO 3, NORWAY

来源：

JOURNAL OF GEOPHYSICAL RESEARCH | 1973年 / 78卷 / 22期

关键词：

D O I：

10.1029/JA078i022p04787

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

引用

页码：4787 / 4791

页数：5

共 18 条

[11]

Wilcox J. M., 1968, Solar Physics, V5, P564, DOI 10.1007/BF00147021

[12]

Wilcox J.M., 1967, SOPH, V1, P437, DOI DOI 10.1007/BF00151368

[13] QUASI-STATIONARY COROTATING STRUCTURE IN INTERPLANETARY MEDIUM [J].

WILCOX, JM .

JOURNAL OF GEOPHYSICAL RESEARCH, 1965, 70 (23) :5793-+

[14] INTERPLANETARY SECTOR STRUCTURE AT SOLAR MAXIMUM [J].

WILCOX, JM ;

COLBURN, DS .

JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (04) :751-+

[15]

WILCOX JM, 1971, SOLAR MAGNETIC FIELD

[16]

WILCOX JM, 1971, 83 ASTR SOC PAC PUBL, P561

[17]

1962, 5658 HIGH ALT OBS RE

[18]

6061 HIGH ALT OBS RE