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Physics of solar prominences: I—spectral diagnostics and non-LTE modelling
This review paper outlines background information and covers recent advances made via
the analysis of spectra and images of prominence plasma and the increased sophistication …
the analysis of spectra and images of prominence plasma and the increased sophistication …
Partial ionization of plasma in solar prominences
P Heinzel, S Gunár, S Jejčič - … Transactions of the …, 2024 - royalsocietypublishing.org
The plasma in cool cores of solar prominences is partially ionized and its ionization degree,
in general, depends on the actual kinetic temperature and density of the plasma and the …
in general, depends on the actual kinetic temperature and density of the plasma and the …
On the nature of dark extreme ultraviolet structures seen by SOHO/EIT and TRACE
U Anzer, P Heinzel - The Astrophysical Journal, 2005 - iopscience.iop.org
Spectral lines in the extreme ultraviolet (EUV) observed on the Sun can originate either from
the hot corona or the cooler chromosphere to corona transition region. In the present paper …
the hot corona or the cooler chromosphere to corona transition region. In the present paper …
Soho contribution to prominence science
We present the main current issues concerning prominence studies. We recall the large
range of plasma parameters found in prominences which makes the work of the MHD …
range of plasma parameters found in prominences which makes the work of the MHD …
Mg II h&k fine structure prominence modelling and the consequences for observations
Aims. Using 2D Mg II h&k solar prominence modelling, our aim is to understand the
formation of complex line profiles and how these are seen by the Interface Region Imaging …
formation of complex line profiles and how these are seen by the Interface Region Imaging …
Detailed comparison of downflows seen both in EIT 30.4 nm and Big Bear Hα movies
An EIT shutterless campaign was conducted on 11 July 2001 and provided 120 high-
cadence (68 s) 30.4 nm images of the north-eastern quarter of the Sun. Systematic intensity …
cadence (68 s) 30.4 nm images of the north-eastern quarter of the Sun. Systematic intensity …
What is a macrospicule?
Macrospicules are typically described as solar jets that are larger and more long-lived than
spicules, and visible mostly in transition-region spectral lines. They show a broad variation …
spicules, and visible mostly in transition-region spectral lines. They show a broad variation …
Structure of prominence legs: plasma and magnetic field
We investigate the properties of a" solar tornado" observed on 2014 July 15, and aim to link
the behavior of the plasma to the internal magnetic field structure of the associated …
the behavior of the plasma to the internal magnetic field structure of the associated …
[HTML][HTML] On the application of stark broadening data determined with a semiclassical perturbation approach
On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation
Approach Next Article in Journal / Special Issue Special Issue on Spectral Line Shapes in …
Approach Next Article in Journal / Special Issue Special Issue on Spectral Line Shapes in …
Non-LTE radiative transfer in model prominences. I. Integrated intensities of He I triplet lines
In this work we use new results of radiative transfer calculations out of local
thermodynamical equilibrium to study the triplet lines emitted by neutral helium in solar …
thermodynamical equilibrium to study the triplet lines emitted by neutral helium in solar …