Reconnection in Weakly-Ionized Plasma
Part of the Astrophysics and Space Science Library book series (ASSL, volume 341)
Magnetic reconnection, while being well established in the solar corona, is successfully invoked for explanation of many phenomena in the low-temperature weakly-ionized plasma in the solar atmosphere.
KeywordsMagnetic Reconnection Solar Atmosphere Convective Zone Electric Current Density Azimuthal Velocity
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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© Springer Science+Business Media, LLC 2006