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Method of tethered system control for deorbiting objects using earth's atmosphereA space tethered system used as an atmospheric braking device for deorbiting small satellites from

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

Mathematical model of control points placing for monitoring polluting substances emissions in the atmosphere on the basis of the NP-full coloring graph task decisionMathematical model of control points placing for monitoring polluting substances emissions

Carbon neutron star atmospheres this composition for other similar sources, a publicly available detailed grid of the carbon model atmosphere

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

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

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

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

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

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

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