North-south cosmic ray asymmetry and high speed solar wind

被引：4

作者：

Svirzhevskaya, AK

Bazilevskaya, GA

Svirzhevsky, NS

Krainev, MB

机构：

[1] Lebedev Physical Institute, 117924 Moscow

来源：

HELIOSPHERE AT SOLAR MINIMUM AND BEYOND | 1997年 / 19卷 / 06期

基金：

俄罗斯基础研究基金会;

关键词：

D O I：

10.1016/S0273-1177(97)00305-0

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The data on the north-south asymmetry in cosmic ray intensity as obtained in the stratospheric radiosound observations at the high-latitude stations Murmansk and Mirny in 1963-1994 are presented. A significant asymmetry (7-10%) but with the opposite sign was found in 1973 (positive) and in 1992-1993 (negative). Rises in the asymmetry sometimes happen simultaneously with the appearance of the asymmetric high-speed streams of solar wind at the Earth's orbit. (C) 1997 COSPAR. Published by Elsevier Science Ltd.

引用

页码：929 / 932

页数：4

共 7 条

[1]

CHARAKHCHYAN TN, 1986, GEOMAGN AERON+, V26, P10

[2]

CHARAKHCHYAN TN, 1986, COSMIC RAY VARIATION, P110

[3]

POKREVSKY PE, 1990, P 21 INT COSM RAY C, V6, P112

[4]

SHEA MA, 1975, AFCRLTR750247 HANSC

[5] Cosmic rays in the atmosphere: North-south asymmetry [J].

Stozhkov, YI ;

Bazilevskaya, GA ;

Pokrevsky, PE ;

Svirzhevsky, NS ;

Martin, IM ;

Turtelli, A .

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1996, 101 (A2) :2523-2528

[6]

Vernov S N, 1965, P 9 ICCR, V1, P517

[7] GLOBAL EVOLUTION OF INTERPLANETARY SECTOR STRUCTURE, CORONAL HOLES, AND SOLAR-WIND STREAMS DURING 1976-1993 - STACKPLOT DISPLAYS BASED ON SOLAR MAGNETIC OBSERVATIONS [J].

WANG, YM ;

SHEELEY, NR .

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1994, 99 (A4) :6597-6608

← 1 →