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Structure and Topology of Magnetic Fields in Solar Prominences

Published online by Cambridge University Press:  06 January 2014

Adriaan A. van Ballegooijen  and
Yingna Su
Adriaan A. van Ballegooijen
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS-15, Cambridge, MA 02138, USA email: vanballe@cfa.harvard.edu
Yingna Su
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS-15, Cambridge, MA 02138, USA email: vanballe@cfa.harvard.edu
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Abstract

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Recent observations and models of solar prominences are reviewed. The observations suggest that prominences are located in or below magnetic flux ropes that lie horizontally above the PIL. However, the details of the magnetic structure are not yet fully understood. Gravity likely plays an important role in shaping the vertical structures observed in quiescent prominences. Preliminary results from a time-dependent model describing the interaction of a magnetic flux rope with photospheric magnetic elements are presented.

Keywords

Sun: prominencesSun: filamentsSun: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 127 - 134
Copyright
Copyright © International Astronomical Union 2013 

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