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Height and time variability of planetary wave activityReference atmosphere models

A method for modeling the formation of Call lines in the spectra of irradiated stellar atmospheres to calculate model irradiated atmospheres in a semi-grey approximation has been improved. We have modified

Accretion heated atmospheres of X-ray bursting neutron stars is well described by the atmosphere model of a passively cooling neutron star when the burst luminosity

Radiative properties of magnetic neutron stars with metallic surfaces and thin atmospheresContext. Simple models fail to describe the observed spectra of X-ray-dim isolated neutron stars

Investigation of Cyg OB2 #11(O5 Ifc) by modelling its atmosphere-resolution spectra. In this paper we present results of the modelling of the stellar atmosphere of Cyg OB2 #11

Model atmospheres of x-ray bursting neutron starsWe present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron

Models of neutron star atmospheres enriched with nuclear burning ashes the metal enrichment can change these factors. Methods. We have developed a new NS atmosphere modeling code

Influence of Irregularities of Water Vapor Field in Surface Layer of the Atmosphere on the Results of Satellite Monitoring of Hydropower Structures in Region of Reservoirs for the modeling of coordinate errors in the projected GNSS system of monitoring the Zagorsk GAES-2 that are caused

35 P 09 Non linear effects of spaced distribution of aerosols in turbulent atmosphere35 P 09 Non linear effects of spaced distribution of aerosols in turbulent atmosphere

Analysis of observations and results of numerical modeling of meteorological parameters and atmospheric air pollution under weak wind conditions in the city of TomskThe results of calculation of meteorological parameters using a meteorological model, TSU-NM3

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