Understanding Interplanetary Coronal Mass Ejection SignaturesReport of Working Group B

被引：0
作者：
R. F. Wimmer-Schweingruber
N. U. Crooker
A. Balogh
V. Bothmer
R. J. Forsyth
P. Gazis
J. T. Gosling
T. Horbury
A. Kilchenmann
I. G. Richardson
J. D. Richardson
P. Riley
L. Rodriguez
R. von Steiger
P. Wurz
T. H. Zurbuchen
机构：
[1] Christian-Albrechts-Universityät zu Kiel,Institut für Experimentelle und Angewandte Physik, Extraterrestrische Physik
[2] Boston University,Center for Space Physics
[3] Imperial College London,The Blackett Laboratory
[4] Max-Planck-Institut für Sonnensystemforschung,Physikalisches Institut
[5] San Jose State University Foundation,Dept. of Atmosph.,Oceanic, and Space Sciences
[6] NASA Ames Research Center,undefined
[7] Laboratory for Atmospheric and Space Physicsm University of Colorado,undefined
[8] International Space Science Institute,undefined
[9] NASA Goddard Space Flight Center,undefined
[10] Massachusets Institute of Technology,undefined
[11] Science Applications International Corporation,undefined
[12] Universität Bern,undefined
[13] University of Michigan,undefined
来源：
Space Science Reviews | 2006年 / 123卷
关键词：
coronal mass ejections; interplanetary physics; solar wind;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
While interplanetary coronal mass ejections (ICMEs) are understood to be the heliospheric counterparts of CMEs, with signatures undeniably linked to the CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research. These issues are discussed in the context of traditional understanding, and recent results using innovative analysis techniques are reviewed.
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页码：177 / 216
页数：39
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