Classification and mean behavior of magnetic storms

被引:402
作者
Loewe, CA
Prolss, GW
机构
[1] Institut für Astrophysik und Extraterrestrische Forschung, Universität Bonn, Bonn
来源
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1997年 / 102卷 / A7期
关键词
D O I
10.1029/96JA04020
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Dst index is used to identify more than 1000 storms which occurred in the time interval 1957 to 1993. Using the minimum Dst value as an indicator, we classify the storms as weak (482), moderate (346), strong (206), severe (45), and great (6). For each of these classes the mean time variation is determined. In contrast to the well-known study of Sugiura and Chapman [1960], the Dst minimum is used as a common reference epoch. This leads to much better agreement between the average and the typical storm behavior. We also find that the maximum ap and AE activity precedes the Dst minimum by 1 to 2 hours. Finally, we demonstrate that both sudden commencement and gradual commencement storms are associated with a distinct decrease in the B-z component of the interplanetary magnetic field.
引用
收藏
页码:14209 / 14213
页数:5
相关论文
共 24 条
[1]  
AKASOFU SI, 1970, ANN GEOPHYS, V26, P443
[2]  
ALLEN J, 1989, EOS T AGU, V70, P1486
[3]  
ALLEN J, 1989, EOS T AGU, V70, P1479, DOI DOI 10.1029/89EO00409
[4]  
[Anonymous], 1972, SOLAR TERRESTRIAL PH
[5]  
[Anonymous], 1992, SOLAR TERRESTRIAL EN
[6]  
BOTELER DH, 1991, EOS T AM GEOPHYS UN, V72, P159, DOI [DOI 10.1029/EO072I014P00159, 10.1029/EO072i014p00159]
[7]  
CHAPMAN S, 1962, GEOMAGNETISM
[8]  
COLE KD, 1966, SPACE SCI REV, V5, P699
[9]   MAGNETIC-FIELD OF THE MAGNETOSPHERIC RING CURRENT AND ITS DYNAMICS DURING MAGNETIC STORMS [J].
FELDSTEIN, YI ;
GRAFE, A ;
PISARSKY, VY ;
PRIGANSOVA, A ;
SUMARUK, PV .
JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1990, 52 (12) :1185-1191
[10]   WHAT IS A GEOMAGNETIC STORM [J].
GONZALEZ, WD ;
JOSELYN, JA ;
KAMIDE, Y ;
KROEHL, HW ;
ROSTOKER, G ;
TSURUTANI, BT ;
VASYLIUNAS, VM .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1994, 99 (A4) :5771-5792