<b>Context</b>: Extreme ultraviolet resonance lines of neutral and ionised helium observed in prominences are difficult to interpret as the prominence plasma is optically thick at these wavelengths. If mass motions are taking place, as is the case in active and eruptive prominences, the diagnostic is even more complex. <b>Aims</b>: We aim at studying the effect of radial motions on the spectrum emitted by moving prominences in the helium resonance lines and at facilitating the interpretation of observations, in order to improve our understanding of these dynamic structures. <b>Methods</b>: We develop our non-local thermodynamic equilibrium radiative transfer code formerly used for the study of quiescent...
The resonance lines of helium in the Sun are several times stronger than expected, relative to lines...
We present the first comparison of profiles of H et He resonance lines observed by SUMER with theore...
Context: Spectral lines of helium are commonly observed on the Sun. These observations contain impor...
We aim at facilitating the interpretation of observations in the helium resonance lines in moving pr...
We summarize the results on the formation of the helium spectrum in solar prominences obtained over ...
Active prominences exhibit plasma motions, resulting in difficulties with the interpretation of spec...
In this study we show how hydrogen and helium lines modelling can be used to make a diagnostic of a...
Even quiescent solar prominences may become active and sometimes erupt. These events are occasionall...
Context. While classical models successfully reproduce intensities of many transition region lines, ...
Context. While classical models successfully reproduce intensities of many transition region lines, ...
To investigate the cause of anomalously bright resonance lines of helium in the Sun, we have studied...
We present new non-LTE modelling of the helium spectrum emitted by quiescent solar prominences. The ...
Context. Theoretical calculations have shown that when solar prominences move away from the surface ...
<b>Context</b>. During a multi-wavelength observation campaign with Hinode and ground-ba...
This contribution aims to present non-local thermodynamic Equilibrium (NLTE) modeling of hydrogen an...
The resonance lines of helium in the Sun are several times stronger than expected, relative to lines...
We present the first comparison of profiles of H et He resonance lines observed by SUMER with theore...
Context: Spectral lines of helium are commonly observed on the Sun. These observations contain impor...
We aim at facilitating the interpretation of observations in the helium resonance lines in moving pr...
We summarize the results on the formation of the helium spectrum in solar prominences obtained over ...
Active prominences exhibit plasma motions, resulting in difficulties with the interpretation of spec...
In this study we show how hydrogen and helium lines modelling can be used to make a diagnostic of a...
Even quiescent solar prominences may become active and sometimes erupt. These events are occasionall...
Context. While classical models successfully reproduce intensities of many transition region lines, ...
Context. While classical models successfully reproduce intensities of many transition region lines, ...
To investigate the cause of anomalously bright resonance lines of helium in the Sun, we have studied...
We present new non-LTE modelling of the helium spectrum emitted by quiescent solar prominences. The ...
Context. Theoretical calculations have shown that when solar prominences move away from the surface ...
<b>Context</b>. During a multi-wavelength observation campaign with Hinode and ground-ba...
This contribution aims to present non-local thermodynamic Equilibrium (NLTE) modeling of hydrogen an...
The resonance lines of helium in the Sun are several times stronger than expected, relative to lines...
We present the first comparison of profiles of H et He resonance lines observed by SUMER with theore...
Context: Spectral lines of helium are commonly observed on the Sun. These observations contain impor...