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Models of magnetized neutron star atmospheres: Thin atmospheres and partially ionized hydrogen atmospheres with vacuum polarization for modeling magnetized neutron star atmospheres in a wide range of magnetic fields (10 12-1015 G

Models of magnetized neutron star atmospheres: Thin atmospheres and partially ionized hydrogen atmospheres with vacuum polarization for modeling magnetized neutron star atmospheres in a wide range of magnetic fields (10 12-1015 G

Models of magnetized neutron star atmospheresWe present a new computer code for modeling magnetized neutron star atmospheres in a wide range

Measuring the basic parameters of neutron stars using model atmospheres© 2016, SIF, Springer-Verlag Berlin Heidelberg. Model spectra of neutron star atmospheres

Atmospheres and spectra of X-ray illuminated stars: A nongray model for computing X-ray irradiated blanketed model atmospheres is described. The heating function

Modeling the dielectric barrier micro-discharge in argon at atmospheric pressureDielectric barrier micro-discharge in argon at atmospheric pressure is simulated. Spatial

Atmospheres and spectra of X-ray illuminated stars: A gray modelA gray model is used to explore the effect of heating of stellar atmospheres by an external X

Semi-empirical model of middle atmosphere wind from the ground to the lower thermosphere empirical middle atmosphere wind models, such as CIRA-86 and HWM-93 to the new data. This has led

X-ray bursting neutron star atmosphere models using an exact relativistic kinetic equation for Compton scatteringContext. Theoretical spectra of X-ray bursting neutron star (NS) model atmospheres are widely used

Measuring the basic parameters of neutron stars using model atmospheres© 2016, SIF, Springer-Verlag Berlin Heidelberg. Model spectra of neutron star atmospheres

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