Properties of prominence fine-structure threads derived from SOHO/SUMER hydrogen Lyman lines - Université Pierre et Marie Curie Accéder directement au contenu
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2007

Properties of prominence fine-structure threads derived from SOHO/SUMER hydrogen Lyman lines

Résumé

Context: The SOHO/SUMER observations provide us for the first time with the prominence spectra in the Lyman-alpha line outside the attenuator together with the higher members of the hydrogen Lyman series.
Aims: We derive the prominence fine-structure thread properties by comparing the SOHO/SUMER hydrogen Lyman series observations with the synthetic Lyman lines.
Methods: To obtain the synthetic profiles of the Lyman lines, we used 2D prominence fine-structure thread models with a PCTR and consistently solved the 2D non-LTE multilevel radiative transfer. The trial-and-error method was applied to find the model with the best agreement between the synthetic Lyman line profiles and the observed ones.
Results: The properties of the resulting model with the best match of the synthetic and observed line profiles are central (minimum) temperature T0 = 7000 K, maximum column mass in the centre of the thread M0 = 1.1×10-4 g cm-2, horizontal field strength in the middle of the thread Bx(0) = 6 Gauss and the boundary pressure p0 = 0.015 dyn cm-2.
Conclusions: The Lyman line profiles observed by SOHO/SUMER can be better reproduced by using multi-thread models consisting of a set of the 2D prominence fine-structure threads placed perpendicularly to the line-of-sight, rather than with the single-thread model.
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Dates et versions

hal-03732570 , version 1 (24-10-2022)

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Stanislav Gunár, Petr Heinzel, Brigitte Schmieder, P. Schwartz, U. Anzer. Properties of prominence fine-structure threads derived from SOHO/SUMER hydrogen Lyman lines. Astronomy and Astrophysics - A&A, 2007, 472, pp.929-936. ⟨10.1051/0004-6361:20077785⟩. ⟨hal-03732570⟩
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