DETAILED COMPARISON BETWEEN SUNSPOT ACTIVITY IN HOT-SPOTS AND GALACTIC COSMIC-RAY INTENSITY

被引：4

作者：

AKIOKA, M

KUBOTA, J

SUZUKI, M

TOHMURA, I

机构：

[1] KYOTO UNIV,FAC SCI,KWASAN OBSERV,SAKYO KU,KYOTO 606,JAPAN

[2] KYOTO UNIV,FAC SCI,HIDA OBSERV,SAKYO KU,KYOTO 606,JAPAN

[3] KAWAGOE HIGH SCH,KAWAGOE,MIE 512,JAPAN

[4] OSAKA PREFECTURAL COLL TECHNOL,NEYAGAWA,OSAKA 572,JAPAN

来源：

SOLAR PHYSICS | 1992年 / 139卷 / 01期

关键词：

D O I：

10.1007/BF00147888

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The influence of sunspot activity on the condition of the solar-terrestrial environment during cycle 21 was examined using the data of sunspots and the modulation of the galactic cosmic-ray intensity. The 'hot spots' discussed by Ichimoto et al. (1985) and Bai (1987a, 1988) were also found by analyzing the longitudinal distribution of sunspot groups. A detailed comparison between the time change of the sunspot activity in hot spots and that of the galactic cosmic rays observed by the neutron monitor reveals that several transient diminutions of the GCR intensity (with much longer duration than a Forbush decrease) occur at nearly the same time as the sporadic enhancement of sunspot area in the hot spots.

引用

页码：177 / 187

页数：11

共 17 条

[1] THE 17-MONTH PERIODICITY OF SUNSPOT ACTIVITY [J].