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.


Magnetic Reconnection Solar Atmosphere Convective Zone Electric Current Density Azimuthal Velocity 
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Copyright information

© Springer Science+Business Media, LLC 2006

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