Radial Evolution of Large-scale Solar Wind Structures

Radial Evolution of Large-scale Solar Wind Structures

333 pages· 2008· ISBN 9781109143140
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Stream interaction regions (SIRs) and interplanetary coronal mass ejections (ICMEs) are two types of large-scale solar wind structures. Both can cause interplanetary shocks, generate energetic particles, and affect planetary magnetospheres and ionospheres. One key element of successful space weather forecasting is being able to predict how these two structures evolve radially from the Sun.

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