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Importance of Compton scattering for radiation spectra of isolated neutron stars with weak magnetic fieldsAims. Emergent model spectra of neutron-star atmospheres are widely used to fit the observed soft X

Non-LTE effects for Na I lines in X-ray illuminated stellar atmospheres I model atom for the LTE model atmospheres of irradiated F-G stars obtained with allowance for a

Radiative properties of highly magnetized isolated neutron star surfaces and approximate treatment of absorption features in their spectra surfaces and partially ionized hydrogen model atmospheres, with semi-infinite and thin atmospheres above a

Modeling of atmospheric air quality in the Tomsk using WRF/CAMx complex the level of atmospheric air quality in the city based on numerical modeling. For these periods, the values

X-ray bursting neutron star atmosphere models: Spectra and color corrections of corresponding model atmospheres is necessary for these investigations. Methods. We computed such a set of model

GPS-Derived zenith tropospheric delay assimilation into numeric atmosphere model 10%. Hardware-software complex includes the numerical model of the atmosphere on a computational

Importance of Compton scattering for radiation spectra of isolated neutron starsModel atmospheres of isolated neutron stars with low magnetic field are calculated with Compton

Importance of Compton scattering for radiation spectra of isolated neutron starsModel atmospheres of isolated neutron stars with low magnetic field are calculated with Compton

The atmospheric lithium abundances of solar analogues based on high-resolution echelle spectra using model atmospheres in a non-LTE approach. In terms

Description of radiation conditions and evaluation of the date of 137Cs release to the atmosphere using the radionuclide transfer model coupled with the forecasts by the mesoscale hydrodynamic model and wet deposition on the surface are computed using the Lagrangian stochastic model of the NOSTRADAMUS

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