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Causes and Effects of Filament Eruptions
Published online by Cambridge University Press: 12 April 2016
Abstract
Observational and theoretical aspects of filament destabilization are reviewed in light of the concept of filament eruption as catastrophic loss of equilibrium in a magnetic configuration of inverse polarity. Interrelations between eruptive prominences and other phenomena of solar activity such as flares, CMEs, and loop arcade are considered.
- Type
- Birth and Death of Filaments
- Information
- International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 342 - 349
- Copyright
- Copyright © Astronomical Society of the Pacific 1998
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