Non-LTE modelling of prominence fine structures using hydrogen Lyman-line profiles

0450660 - ASÚ 2016 RIV FR eng J - Článek v odborném periodiku
Schwartz, Pavol - Gunár, S. - Curdt, W.
Non-LTE modelling of prominence fine structures using hydrogen Lyman-line profiles.
Astronomy & Astrophysics. Roč. 577, May (2015), A92/1-A92/10. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA ČR GAP209/12/0906
Grant ostatní: SAV(SK) VEGA 2/0108/12
Institucionální podpora: RVO:67985815
Klíčová slova: Sun * filaments * prominences
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.185, rok: 2015

We perform a detailed statistical analysis of the spectral Lyman-line observations of the quiescent prominence observed on May 18, 2005. We investigated the plasma properties of the prominence observed with the SoHO/SUMER spectrograph on May 18, 2005 by comparing the histograms of three statistical parameters characterizing the properties of the synthetic and observed line profiles. In this way, the integrated intensity, Lyman decrement ratio, and the ratio of intensity at the central reversal to the average intensity of peaks provided insight into the column mass and the central temperature of the prominence fine structures.
Trvalý link: http://hdl.handle.net/11104/0252000