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Cited article:
S. Gunár , P. Heinzel , U. Anzer
A&A, 528 (2011) A47
Published online: 2011-02-28
This article has been cited by the following article(s):
7 articles
Properties of the prominence magnetic field and plasma distributions as obtained from 3D whole-prominence fine structure modeling
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Non-LTE modelling of prominence fine structures using hydrogen Lyman-line profiles
P. Schwartz, S. Gunár and W. Curdt Astronomy & Astrophysics 577 A92 (2015) https://doi.org/10.1051/0004-6361/201425138
Magnetic field and radiative transfer modelling of a quiescent prominence
S. Gunár, P. Schwartz, J. Dudík, et al. Astronomy & Astrophysics 567 A123 (2014) https://doi.org/10.1051/0004-6361/201322777
Modelling of quiescent prominence fine structures
S. Gunár Proceedings of the International Astronomical Union 8 (S300) 59 (2013) https://doi.org/10.1017/S1743921313010752
Modeling of Hα Eruptive Events Observed at the Solar Limb
P. Kotrč, M. Bárta, P. Schwartz, et al. Solar Physics 284 (2) 447 (2013) https://doi.org/10.1007/s11207-012-0167-6
Dynamics of quiescent prominence fine structures analyzed by 2D non-LTE modelling of the Hα line
S. Gunár, P. Mein, B. Schmieder, P. Heinzel and N. Mein Astronomy & Astrophysics 543 A93 (2012) https://doi.org/10.1051/0004-6361/201218940
Synthetic differential emission measure curves of prominence fine structures
S. Gunár, S. Parenti, U. Anzer, P. Heinzel and J.-C. Vial Astronomy & Astrophysics 535 A122 (2011) https://doi.org/10.1051/0004-6361/201117429