RETURN OF THE HARD SOLAR-FLARES 154 DAY PERIODICITY IN SOLAR CYCLE-22 AND EVIDENCE FOR A PHASE RELATIONSHIP OF THIS PERIODICITY BETWEEN CYCLE-21 AND CYCLE-22

被引：10

作者：

BRUECKNER, GE

COOK, JW

机构：

[1] Code 4160, Naval Research Laboratory, Washington

[2] Code 4163, Naval Research Laboratory, Washington

来源：

ASTROPHYSICAL JOURNAL | 1990年 / 350卷 / 01期

关键词：

Sun: activity; Sun: flares;

D O I：

10.1086/185658

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Solar activity rose to high levels in 1989. In 1989 March and August, groups of very strong X-ray flares were observed. The phase difference between these two groups is 155 days. There is evidence for a phase relationship of the 155 day period between solar cycles 21 and 22.

引用

页码：L21 / L24

页数：4

共 6 条

[1] CONFIRMATION OF A 152 DAY PERIODICITY IN THE OCCURRENCE OF SOLAR-FLARES INFERRED FROM MICROWAVE DATA [J].