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Simulation Studies of Solar Prominence Formation
Published online by Cambridge University Press: 12 April 2016
Abstract
A series of numerical simulations are presented for formation of solar prominences. We have investigated the dynamic and thermodynamic evolution of coronal plasma in response to photospheric horizontal motions. In three different setups of field configurations and footpoint motions, different types of prominences are found to be formed by thermal instability.
- Type
- Birth and Death of Filaments
- Information
- International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 278 - 281
- Copyright
- Copyright © Astronomical Society of the Pacific 1998