0519293 - ASÚ 2020 RIV IT eng J - Článek v odborném periodiku
Susino, R. - Bemporad, A. - Heinzel, Petr - Jejčič, Sonja - Anzer, U. - Dzifčáková, Elena
Determination of the physical properties of an erupting prominence from SOHO/LASCO and UVCS observations.
Nuovo Cimento. Roč. 42, č. 1 (2019), č. článku 37. ISSN 2037-4909. E-ISSN 1826-9885
Institucionální podpora: RVO:67985815
Klíčová slova: physical conditions * erupting prominence * ultraviolet data
Obor OECD: Astronomy (including astrophysics,space science)
Způsob publikování: Open access
DOI: https://doi.org/10.1393/ncc/i2019-19037-6

We studied the physical conditions of an erupting prominence observed in the core of a coronal mass ejection, using combination of SOHO/LASCO-C2 visible-light images and SOHO/UVCS ultraviolet data. Measured intensities and profiles of the neutral-hydrogen Lyman-alpha and Lyman-beta lines and the 977 angstrom C III line were used together with the visible-light brightness to derive the geometrical and physical parameters of the prominence, such as the line-of-sight apparent thickness. electron column density, kinetic temperature, and microturbolent velocity. These parameters were used to constrain a non-LTE (i.e., out of local thermodynamic equilibrium) radiative-transfer model of the prominence that provides the effective thickness, electron density, and flow velocity, in a sample of points selected along the prominence. The prominence can be described as a hot structure with low electron density and very low gas pressure compared to typical quiescent prominences. Intensities of the hydrogen lines were also used for a detailed determination of the plasma line-of-sight filling factor, in the two prominence points where simultaneous and cospatial LASCO-C2 and UVCS observations were available.

Trvalý link: http://hdl.handle.net/11104/0304292