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Phase Shift between Changes in Global Temperature and Atmospheric CO2 Content under External Emissions of Greenhouse Gases into the Atmosphere

Muryshev K., Eliseev A., Denisov S., Mokhov I., Arzhanov M., Timazhev A.

into the atmosphere on the basis of numerical experiments with the IAP RAS climatic model and a conceptual climate

Analyzing Effects of Directionality and Random Heights in Drone-based mmWave Communication

Kovalchukov R., Moltchanov D., Samuylov A., Ometov A., Andreev S., Koucheryavy Y., Samouylov K.

-dimensional model for drone-based mmWave communication that captures the high directionality of transmissions

Models of neutron star atmospheres enriched with nuclear burning ashes

Nättilä J., Suleimanov V., Kajava J., Poutanen J.

the metal enrichment can change these factors. Methods. We have developed a new NS atmosphere modeling code

Radiative properties of magnetic neutron stars with metallic surfaces and thin atmospheres

Potekhin A., Suleimanov V., Van Adelsberg M., Werner K.

Context. Simple models fail to describe the observed spectra of X-ray-dim isolated neutron stars

Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra

Nättilä J., Miller M., Steiner A., Kajava J., Suleimanov V., Poutanen J.

other. For the first time, we here fit atmosphere models of X-ray bursting NSs directly to the observed

Midlatitude model of the electron density gradient in the lower ionosphere

Teptin G., Khoutorova O., Zhuravlev A.

of the standard atmosphere and the theory of radiowave propagation in an inhomogeneous medium. The obtained model

Analysis of Joint Channel Coexistence Time at Space-Diversity Radio Reception of Meteor Reflections

Atmospheric modeling

Global meteorological forecast data and instrumental measurement application for simulation of mesoscale atmospheric boundary layer processes

Starchenko, Alexander V., Bart, Andrey A.

The accuracy of the results of numerical modeling of local atmospheric processes, in particular

A non-pulsating neutron star in the supernova remnant HESS J1731-347/G353.6-0.7 with a carbon atmosphere

Klochkov D., Pühlhofer G., Suleimanov V., Simon S., Werner K., Santangelo A.

scale and used a carbon atmosphere model to describe the X-ray spectrum of the CCO and to estimate

The neutron star in HESS? J1731 - 347: Central compact objects as laboratories to study the equation of state of superdense matter

Klochkov D., Suleimanov V., Pühlhofer G., Yakovlev D., Santangelo A., Werner K.

of a long-term flux and spectral variability. Results. The analysis shows that atmosphere models

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