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Modelling of quiescent prominence fine structures

Published online by Cambridge University Press:  06 January 2014

S. Gunár
S. Gunár*
Affiliation:
Astronomical Institute of the Academy of Sciences of Czech Republic, 251 65 Ondřejov, Czech Republic email: stanislav.gunar@asu.cas.cz
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Abstract

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We review here the current status and the latest results of the modelling of quiescent prominence fine structures. We begin with the simulations of the prominence magnetic field configurations, through an overview of the modelling of the fine structure formation and dynamics, and with the emphasis on the radiative transfer modelling of the realistic prominence fine structures. We also illuminate the future directions of the field that lie in the combining of the existing approaches into more complex multi-disciplinary models.

Keywords

Sun: prominencesSun: filamentsmagnetic fieldsradiative transfer

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