Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison

被引：6

作者：

Mitsakou, E. ^{[1
]}

Babasidis, G. ^{[1
]}

Moussas, X. ^{[1
]}

机构：

[1] Univ Athens, Sect Astrophys Astron & Mech, Fac Phys, GR-15783 Athens, Greece

来源：

ADVANCES IN SPACE RESEARCH | 2009年 / 43卷 / 04期

关键词：

Coronal mass ejections; Magnetic field; MAGNETIC CLOUDS; SOLAR-WIND; SOLAR-CYCLE-23; ORIGIN; MAXIMUM; PLASMA; STORMS; SHOCK; 1-AU; AU;

D O I：

10.1016/j.asr.2008.08.003

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

We have used Omniweb data in order to identify the sheath and the ejecta boundaries of 67 shock-driving interplanetary coronal mass ejections during the time period 2003-2006. We examine and compare their statistical properties (speed, magnetic field strength, proton density and temperature, proton plasma beta), with those of the typical solar wind. We also calculate their passage time and radial width. We study the correlation between the ejecta and sheath characteristics. (C) 2008 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：495 / 498

页数：4

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