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Method of tethered system control for deorbiting objects using earth's atmosphere
Razoumny Y.N., Kupreev S.A., Misra A.K.
A 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 fields
Suleimanov V., Werner K.
Aims. 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 decision
Brakovich, A. I., Urbanovich, P. P.
Mathematical model of control points placing for monitoring polluting substances emissions
Carbon neutron star atmospheres
Suleimanov V., Klochkov D., Pavlov G., Werner K.
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
Jacobi C., Fröhlich K., Portnyagin Y., Merzlyakov E., Solovjova T., Makarov N., Rees D., Fahrutdinova A., Guryanov V., Fedorov D., Korotyshkin D., Forbes J., Pogoreltsev A., Kürschner D.
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
Ivanova D., Sakhibullin N., Shimanskiǐ V.
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
Suleimanov V., Poutanen J., Werner K.
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
Sakhibullin N., Shimanskii V.
for computing X-ray irradiated blanketed model atmospheres is described. The heating function
Atmospheres and spectra of X-ray illuminated stars: A gray model
Sakhibullin N., Shimanskii V.
A 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
Sakhibullin N., Shimansky V.
I model atom for the LTE model atmospheres of irradiated F-G stars obtained with allowance for a

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