We investigate a new modeling way for describing the continuous absorption of electromagnetic radiation in a dense partially ionized hydrogen plasma with electron densities 5·1018-1.5·1019 cm-3 and temperatures 16 000–25 000 K, in the wavelength range 300–500 nm. The results can be applied to the plasma of partially ionized layers of stellar atmospheres
We construct hydrogen atmosphere models for strongly magnetized neutron stars in thermodynamic equil...
Context.The hydrogen ionisation degree deviates substantially from statistical equilibrium under th...
Context. The hydrogen ionisation degree deviates substantially from statistical equilibrium under th...
International audienceIn this work, we present a study dedicated to determination of the inverse bre...
A model to predict the emissivity and absorption coefficient of atomic hydrogen plasma is presented ...
Radiation transport in dense plasmas can be an important process in plasma dynamics and diagnostics,...
We developed a model for the equation of state of fully ionized plasmas which we apply to hydrogen. ...
The ionization and radiation dynamics of dense magnetohydrodynamic plasmas has been modeled in a fas...
The problem of ionization produced by a hot star embedded in a hydrogen nebula is studied from basic...
We describe an experimental concept at the National Ignition Facility for specifically tailored sphe...
http://deepblue.lib.umich.edu/bitstream/2027.42/6901/5/bad0524.0001.001.pdfhttp://deepblue.lib.umich...
International audienceA model aimed at describing the electronic structure of hot dense plasmas is p...
We examined the applicability of the Doppler-broadened absorption spectrum of the hydrogen Balmer-al...
The ionization degree of hydrogen is crucial in the physics of the plasma in the solar chromosphere....
Calculations of the hydrogen molecular continuum (a3Σ+g → b3Σ+u, where the latter is repulsive) have...
We construct hydrogen atmosphere models for strongly magnetized neutron stars in thermodynamic equil...
Context.The hydrogen ionisation degree deviates substantially from statistical equilibrium under th...
Context. The hydrogen ionisation degree deviates substantially from statistical equilibrium under th...
International audienceIn this work, we present a study dedicated to determination of the inverse bre...
A model to predict the emissivity and absorption coefficient of atomic hydrogen plasma is presented ...
Radiation transport in dense plasmas can be an important process in plasma dynamics and diagnostics,...
We developed a model for the equation of state of fully ionized plasmas which we apply to hydrogen. ...
The ionization and radiation dynamics of dense magnetohydrodynamic plasmas has been modeled in a fas...
The problem of ionization produced by a hot star embedded in a hydrogen nebula is studied from basic...
We describe an experimental concept at the National Ignition Facility for specifically tailored sphe...
http://deepblue.lib.umich.edu/bitstream/2027.42/6901/5/bad0524.0001.001.pdfhttp://deepblue.lib.umich...
International audienceA model aimed at describing the electronic structure of hot dense plasmas is p...
We examined the applicability of the Doppler-broadened absorption spectrum of the hydrogen Balmer-al...
The ionization degree of hydrogen is crucial in the physics of the plasma in the solar chromosphere....
Calculations of the hydrogen molecular continuum (a3Σ+g → b3Σ+u, where the latter is repulsive) have...
We construct hydrogen atmosphere models for strongly magnetized neutron stars in thermodynamic equil...
Context.The hydrogen ionisation degree deviates substantially from statistical equilibrium under th...
Context. The hydrogen ionisation degree deviates substantially from statistical equilibrium under th...