Abstract
Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower.
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Anzer, U. and Tandberg-Hanssen, E.: 1971, in R. Howard (ed.),IAU Symp. 43, 656.
Athay, R. G., Querfeld, C. W., Smartt, R. N., Landi Degl'Innocenti, E., and Bommier, V.: 1983,Solar Phys. 89, 3.
Bommier, V., Leroy, J. L., and Sahal-Bréchot, S.: 1981,Astron. Astrophys. 100, 231.
Bommier, V., Leroy, J. L., and Sahal-Bréchot, S.: 1986,Astron. Astrophys. 156, 79.
Bommier, V., Landi Degl'Innocenti, E., Leroy, J. L., and Sahal-Bréchot, S.: 1994,Solar Phys. 154, 231.
Harvey, J. W.: 1969, Ph.D. thesis, University of Colorado.
Hirayama, T.: 1990, in V. Ruždjak and E. Tandberg-Hanssen (eds.),IAU Colloq. 117,Lecture Notes in Physics 363, 187.
Jensen, E. and Wiik, J. E.: 1990, in V. Ruždjak and E. Tandberg-Hanssen (sds.),IAU Colloq. 117,Lecture Notes in Physics 363, 298.
Kippenhahn, R. and Schlüter, A.: 1957,Z. Astrophys. 43, 36.
Leroy, J. L.: 1989, in E.R. Priest (ed.),Dynamics and Structure of Quiescent Solar Prominences, Kluwer Academic Publishers, Dordrecht, Holland, p. 77.
Leroy, J. L., Bommier, V., and Sahal-Bréchot, S.: 1983,Solar Phys. 83, 135.
Priest, E.R.: in V. Ruždjak and E. Tandberg-Hanssen (eds.),IAU Colloq. 117,Lecture Notes in Physics 363, 150.
Rust, D. M.: 1966, Ph.D. thesis, University of Colorado, Boulder.
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Anzer, U. Parameters of quiescent prominences derived from magnetic field measurements. Sol Phys 161, 49–55 (1995). https://doi.org/10.1007/BF00732083
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DOI: https://doi.org/10.1007/BF00732083