THE RELATIONSHIP BETWEEN THE GALACTIC COSMIC-RAY INTENSITY AND THE SUNSPOT DISTRIBUTION

被引：2

作者：

BAZILEVSKAYA, GA

KRAINEV, MB

MAKHMUTOV, VS

STOZHKOV, YI

SVIRZHEVSKAYA, AK

SVIRZHEVSKY, NS

机构：

[1] P. N. Lebedev Physical Institute, Russian Academy of Sciences, 117924 Moscow

来源：

HELIOSPHERE DURING THE DECLINING SOLAR CYCLE | 1995年 / 16卷 / 09期

关键词：

D O I：

10.1016/0273-1177(95)00339-G

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A satisfactory relationship is found between the solar activity index that includes both the number of sunspot groups, eta, and their mean heliolatitude, phi, and the galactic cosmic ray (GCR) intensity over more than three 11-year cycles. The solar activity index, eta/phi, is compared with the tilt of the heliospheric current sheet (HCS).

引用

页码：221 / 225

页数：5