The Gnevyshev gap:: A review for space weather

被引：62

作者：

Storini, M ^{[1
]}

Bazilevskaya, GA ^{[1
]}

Flückiger, EO ^{[1
]}

Krainev, MB ^{[1
]}

Makhmutov, VS ^{[1
]}

Sladkova, AI ^{[1
]}

机构：

[1] CNR, IFSI, Area Ric Roma Tor Vergata, I-00133 Rome, Italy

来源：

SPACE WEATHER 2000 | 2003年 / 31卷 / 04期

基金：

俄罗斯基础研究基金会;

关键词：

D O I：

10.1016/S0273-1177(02)00789-5

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The ability to forecast long-term Space Weather effects needs a good knowledge of solar activity behaviour along the 11-year sunspot cycle. In this paper we concentrate our attention on the so-called maximum activity phase and we discuss the role of the Gnevyshev gap (a time interval in which a decrease in solar atmospheric activity is observed) in the time history of Space Weather parameters. (C) 2003 COSPAR. Published by Elsevier Science Ltd. All rights reserved.

引用

页码：895 / 900

页数：6

共 58 条

[1]

AHLUWALIA HS, 1999, P 26 ICRC SALT LAK C, V6, P260

[2]

ALANIA MV, 1999, P 26 ICRC, V7, P131

[3]

[Anonymous], P 25 ICRC

[4] Long-term changes of cosmic ray intensity: Spectral behaviour and 27-day variations [J].

Astafyeva, NM ;

Bazilevskaya, GA .

PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE, 2000, 25 (1-2) :129-132

[5]

ASTALEVA NM, 1997, P 24 INT COSM RAY C, V7, P337

[6] Flare index of solar cycle 22 [J].

Atac, T ;

Ozguc, A .

SOLAR PHYSICS, 1998, 180 (1-2) :397-407

[7]

BAO SD, 1998, JOSO AR 97, P132

[8] Structure of the maximum phase of solar cycles 21 and 22 [J].

Bazilevskaya, GA ;

Krainev, MB ;

Makhmutov, VS ;

Flückiger, EO ;

Sladkova, AI ;

Storini, M .

SOLAR PHYSICS, 2000, 197 (01) :157-174

[9]

BAZILEVSKAYA GA, 1999, P 26 INT COSM RAY C, V6, P240

[10]

BAZILEVSKAYA GA, 1995, 24 INT COSM RAY C RO, V4, P572

← 1 2 3 4 5 6 →