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A non-pulsating neutron star in the supernova remnant HESS J1731-347/G353.6-0.7 with a carbon atmosphere scale and used a carbon atmosphere model to describe the X-ray spectrum of the CCO and to estimate

Direct variational assimilation algorithm for atmospheric chemistry data with transport and transformation modelAtmospheric chemistry dynamics is studied with convection-diffusion-reaction model. The numerical

The phenomenon of atmospheric mirror reflection of spatially oriented atmospheric particles of non-spherical shape can distort model representations

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

Simulation of Vortical Structures' Dynamics. II. Simulation of Interaction of Vortical Structures of modeling results for real vortex systems in atmosphere and plasma are given.

Using weather prediction data for simulation of mesoscale atmospheric processes of global model SLAV for mesoscale modelling of atmospheric processes in areas not covered by meteorological

Non-LTE models for neutron star atmospheres and supernova-fallback disks-LTE model atmospheres for NSs. It is compared to X-ray burst spectra of EXO 0748-676. It is possible

Using WRF mesoscale model to restore temperature profile in atmosphere boundary layer in TomskIn the paper, the possible use of a WRF mesoscale model for the detailed restoring of a temperature

Simulation of interaction of vortex structures of modeling results for real vortex systems in atmosphere and plasma are given.

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

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