Dynamics of Solar Eruptive Filaments

Dynamics of Solar Eruptive Filaments

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These results improve our understanding of the physical processes leading to the destabilization and eruption of solar filaments, and have significant impact on the modeling of the CME initiation and evolution.... pointing is a little more complicated than is the case with a full disk imager where the solar limb provides a reference. ... photospheric line-of-sight magnetic fields: (1) overlay one TRACE 1600 A (UV continuum) image with a magnetogramanbsp;...

Title:Dynamics of Solar Eruptive Filaments
Author:Rui Liu
Publisher:ProQuest - 2008


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