The behavior of hydrogen-line brightness variations, depending on the prominence-velocity changes were investigated. By solving the NON-Local thermodynamic equilibrium (LTE) problem for hydrogen researchers determine quantitatively the effect of Doppler brightening and/or Doppler dimming (DBE, DDE) in the lines of Lyman and Balmer series. It is demonstrated that in low-density prominence plasmas, DBE in H alpha and H beta lines can reach a factor of three for velocities around 160 km/sec, while the L alpha line exhibits typical DDE. L beta brightness variations follow from a combined DBE in the H alpha and DDE in L alpha and L beta itself, providing that all relevant multilevel interlocking processes are taken into account
We summarize the results on the formation of the helium spectrum in solar prominences obtained over ...
The ratio of Ca II 8542 Å to Hβ line intensities has been used for a long time to diagnose the gas...
Context. Observations of hydrogen Balmer lines in solar flares remain an important source of infor...
Departures from complete frequency redistribution (CRD) in hydrogen lines are investigated for solar...
In this study we show how hydrogen and helium lines modelling can be used to make a diagnostic of a...
Active prominences exhibit plasma motions, resulting in difficulties with the interpretation of spec...
International audienceAims: We show how the observed hydrogen Balmer and Lyman emission lines constr...
Aims. We show how the observed hydrogen Balmer and Lyman emission lines constrain the modeling of qu...
Aims. We analyze the dynamics of the prominence fine structures of a quiescent prominence observed ...
International audienceWe revisit the prominence observations in the Lyman α line of Curdt et al. (As...
During 12 to 17 September 1983 a number of prominences were observed with the McMatch solar telescop...
We use the plasma parameters derived from a new global 2.5D three fluid model of the solar wind to c...
Context. Prominence oscillations have been mostly detected using Doppler velocity, although there ar...
(*** abridged ***) Context: The wings of Balmer lines are often used as effective temperature diagno...
The complete hydrogen Lyman spectrum in several prominences has been observed with the UV spectromet...
We summarize the results on the formation of the helium spectrum in solar prominences obtained over ...
The ratio of Ca II 8542 Å to Hβ line intensities has been used for a long time to diagnose the gas...
Context. Observations of hydrogen Balmer lines in solar flares remain an important source of infor...
Departures from complete frequency redistribution (CRD) in hydrogen lines are investigated for solar...
In this study we show how hydrogen and helium lines modelling can be used to make a diagnostic of a...
Active prominences exhibit plasma motions, resulting in difficulties with the interpretation of spec...
International audienceAims: We show how the observed hydrogen Balmer and Lyman emission lines constr...
Aims. We show how the observed hydrogen Balmer and Lyman emission lines constrain the modeling of qu...
Aims. We analyze the dynamics of the prominence fine structures of a quiescent prominence observed ...
International audienceWe revisit the prominence observations in the Lyman α line of Curdt et al. (As...
During 12 to 17 September 1983 a number of prominences were observed with the McMatch solar telescop...
We use the plasma parameters derived from a new global 2.5D three fluid model of the solar wind to c...
Context. Prominence oscillations have been mostly detected using Doppler velocity, although there ar...
(*** abridged ***) Context: The wings of Balmer lines are often used as effective temperature diagno...
The complete hydrogen Lyman spectrum in several prominences has been observed with the UV spectromet...
We summarize the results on the formation of the helium spectrum in solar prominences obtained over ...
The ratio of Ca II 8542 Å to Hβ line intensities has been used for a long time to diagnose the gas...
Context. Observations of hydrogen Balmer lines in solar flares remain an important source of infor...