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Modelling of Non-Uniform Prominence Slabs

Published online by Cambridge University Press:  12 April 2016

P. Heinzel  and
U. Anzer
P. Heinzel
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic CZ–25165 Ondřejov, Czech Republic
U. Anzer
Affiliation:
Max-Planck-Institut für Astrophysik, Postfach 15 23 D–85740 Garching, Germany

Abstract

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We present new slab models for quiescent prominences in which both the condition of magnetohydrostatic equilibrium as well as NLTE are fulfilled. Using the Kippenhahn-Schlüter model, a unique relation between the components of the magnetic field on one hand and the gas pressure and width on the other is established for a given uniform temperature. We construct a grid of such NLTE models and compare them with the set of isothermal-isobaric models of Gouttebroze et al. (1993).

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 213 - 216
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Anzer, U. 1995, Solar Phys., 161, 49 CrossRefGoogle Scholar
Gouttebroze, P., Heinzel, P. and Vial, J.-C. 1993, A&AS, 99, 513 Google Scholar
Heasley, J.N. and Mihalas, D. 1976, ApJ, 205, 273 CrossRefGoogle Scholar
Heinzel, P. 1995, A&A, 299, 563 Google Scholar
Heinzel, P., Gouttebroze, P. and Vial, J.-C. 1994, A&A, 292, 656 Google Scholar