Comment on the paper "CAWSES November 7-8, 2004, Superstorm: Complex Solar and Interplanetary Features in the Post-Solar Maximum Phase," B. T. Tsurutani, E. Echer, F. L. Guarnieri, and J. U. Kozyra, Geophys. Res. Lett. 35 (2008)

被引：1

作者：

Eselevich, V. G. ^{[1
]}

Bogod, V. M. ^{[2
]}

Chashey, I. V. ^{[4
]}

Eselevich, M. V. ^{[1
]}

Yermolaev, Yu. I. ^{[3
]}

机构：

[1] Russian Acad Sci, Inst Solar Terr Phys, Siberian Branch, Irkutsk 664033, Russia

[2] Russian Acad Sci, St Petersburg Branch, Special Astron Pulkovo Observ, St Petersburg, Russia

[3] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia

[4] Russian Acad Sci, PN Lebedev Phys Inst, Pushchino Radio Astron Observ, Pushchino 142292, Moscow Oblast, Russia

来源：

GEOMAGNETISM AND AERONOMY | 2009年 / 49卷 / 01期

基金：

俄罗斯基础研究基金会;

关键词：

94.30.Lr; 96.60.qe;

D O I：

10.1134/S0016793209010186

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

The solar sources of the magnetic storms of November 8 and 10, 2004, are analyzed. The preliminary results of such an analysis [Yermolaev et al., 2005] are critically compared with the results of the paper [Tsurutani et al., 2008], where solar flares were put in correspondence with these magnetic storms. The method for determining solar sources that cause powerful magnetospheric storms is analyzed. It has been indicated that an optimal approach consists in considering coronal mass ejections (CMEs) as storm sources and accompanying flares as additional information about the location of CME origination.

引用

页码：133 / 135

页数：3