Titlebook: Solar Prominences; Jean-Claude Vial,Oddbjørn Engvold Book 2015 Springer International Publishing Switzerland 2015 Coronagraphy.Images Sola

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MHD Equilibria and Triggers for Prominence Eruption,rate how twisted and sheared coronal magnetic structures (with free magnetic energy), capable of driving filament eruptions, can form in the corona in emerging active regions. Several basic mechanisms that can disrupt the quasi-equilibrium coronal structures and trigger the release of the stored fre

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GLOSS

Formation and Large-Scale Patterns of Filament Channels and Filaments,els and filaments are discussed, along with their hemispheric pattern. Next, observations of the formation of filament channels and filaments are described where two opposing views are considered. Finally, the wide range of models that have been constructed to consider the formation of filament chan

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The Dynamics of Eruptive Prominences,es are a part of CMEs is emphasized in terms of their physical association and kinematics. The continued propagation of prominence material into the heliosphere is illustrated using in-situ observations. The solar-cycle variation of eruptive prominence locations is discussed with a particular emphas

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Schlemms-Canal

PANT

Stellar Activity and CMEs: Important Factors of Planetary Evolution,ing an idea of a solar-stellar analogy, CME phenomena are expected on other stars as well. The main planetary impact factors of the stellar CMEs include the associated interplanetary shocks, plasma density and velocity disturbances, energetic particles accelerated in the shock regions, as well as di

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0067-0057 nts a historical description of the developments in spectros.This volume presents the latest research results on solar prominences, including new developments on e.g. chirality, fine structure, magnetism, diagnostic tools and relevant solar plasma physics..In 1875 solar prominences, as seen out of t

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