Effects of the interaction and evolution of interplanetary shocks on “background” solar wind speeds

Author:

Wu Chin-Chun,Feng X. S.,Wu S. T.,Dryer M.,Fry C. D.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference20 articles.

1. Real-time shock arrival predictions during the “Halloween 2003” epoch;Dryer;Space Weather,2004

2. Coronal mass ejections and other extreme characteristics of the 2003 October–November solar eruptions;Gopalswamy;J. Geophys. Res.,2005

3. A three-dimensional, time-dependent numerical modeling of supersonic, super Alfvénic MHD flow;Han;Comput. Fluids,1988

4. Properties of magnetic clouds and geomagnetic storms associated with eruption of coronal sigmoids;Leamon;J. Geophys. Res.,2002

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