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Study of the Components of the Double Star ADS 15571 by Speckle Interferometry

Astronomy letters, 2024, Vol.50 (2), p.138-147

2024

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The Method of Periodic Principal Components for the Dynamic Spectrum of Radio Pulsars and Faraday Rotation of Nine Pulse Components of PSR B0329

Astronomy letters, 2024, Vol.50 (2), p.120-137

2024

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Passage of a Gamma-Ray Burst through a Molecular Cloud: Cloud Ionization Structure

Astronomy letters, 2024, Vol.50 (2), p.99-119

Nesterenok, A. V.

2024

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Magnetic Field Structures of the Stars HD 94660, HD 75049, and HD 154708

Astronomy letters, 2024, Vol.50 (2), p.148-158

Glagolevskij, Yu. V.

2024

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Comparative analysis of the parameters of pulsars with braking indices n>0 and n<0

Astrophysics and space science, 2024-05, Vol.369 (5), p.51

2024

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Boson star superradiance

Science China. Physics, mechanics & astronomy, 2024, Vol.67 (6), p.260413

2024

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Cavity optomechanics with directionally squeezed light

Science China. Physics, mechanics & astronomy, 2024, Vol.67 (6), p.260331

Meystre, Pierre

2024

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Principal components of nuclear mass models

Science China. Physics, mechanics & astronomy, 2024, Vol.67 (7), p.272011

2024

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Shape factor and temperature-dependent viscosity analysis for the unsteady flow of magnetic Al2O3–TiO2/C2H6O2–H2O using Legendre wavelet technique

Pramāṇa, 2024-06, Vol.98 (2)

2024

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Growth, structural, thermal and THz generation properties of modified DAST, CMST and BMST crystals: A comparative study

Pramāṇa, 2024-05, Vol.98 (2)

2024

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SolarAccel: FPGA accelerated 2D cross-correlation of digital images: Application to solar adaptive optics

Journal of astrophysics and astronomy, 2024-05, Vol.45 (1)

2024

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Centering algorithm of an unresolved primary and satellite system

Astrophysics and space science, 2024-05, Vol.369 (5), p.54

2024

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Disturbances in the Rotational Dynamics of Asteroid (99942) Apophis at its Approach to the Earth in 2029

Solar system research, 2024, Vol.58 (2), p.208-219

2024

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Studying the Dynamics of Multiplets of Orbital Resonances of Asteroids with Small Perihelion Distances

Solar system research, 2024, Vol.58 (3), p.326-333

2024

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Manifestations of Anomalous Dissipation in Dusty Plasma in the Solar System: Atmosphereless Cosmic Bodies

Solar system research, 2024, Vol.58 (2), p.220-239

2024

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Numerical Investigation of Slope Stability in Valles Marineris, Mars

Solar system research, 2024, Vol.58 (2), p.176-186

2024

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One-Dimensional Model of Vertical Transport of Chemical Components in the Mars Atmosphere up to the Lower Thermosphere

Solar system research, 2024, Vol.58 (2), p.187-195

2024

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Valley Relief of the Northeastern Part of Terra Cimmeria on Mars

Solar system research, 2024, Vol.58 (3), p.269-275

Mukhamedzhanova, A. E.

2024

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Potentially Primary Xenon Components in Nanodiamond-Enriched Meteorite Fractions: New Isotopic Compositions and Carrier Phases

Solar system research, 2024, Vol.58 (2), p.240-249

2024

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On the Influence of the Rayleigh–Taylor Instability on the Formation of Dust Clouds in the Mesosphere of Mars

Solar system research, 2024, Vol.58 (3), p.263-268

2024

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Crater Formed by the Impact of the Luna-25 Spacecraft

Solar system research, 2024, Vol.58 (2), p.141-147

2024

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Analysis of Spacecraft Flight Trajectories to Venus with a Flyby of Asteroids

Solar system research, 2024, Vol.58 (3), p.334-352

2024

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Obtaining Plasma–Dust Clouds from Meteoritic Matter, its Analogs and Simulants of Lunar Regolith Using Microwave Discharge

Solar system research, 2024, Vol.58 (3), p.289-314

2024

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Impact Structures on Venus as a Result of Asteroid Destruction in the Atmosphere

Solar system research, 2024, Vol.58 (2), p.163-175

2024

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The Influence of the Exosphere of an Active Asteroid on the Polarization of Scattered Light and the Possibility of Estimating Its Properties from Ground-Based Measurements

Solar system research, 2024, Vol.58 (2), p.196-207

Petrova, E. V.

2024

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Study of the Components of the Double Star ADS 15571 by Speckle Interferometry

The Method of Periodic Principal Components for the Dynamic Spectrum of Radio Pulsars and Faraday Rotation of Nine Pulse Components of PSR B0329

Passage of a Gamma-Ray Burst through a Molecular Cloud: Cloud Ionization Structure

Magnetic Field Structures of the Stars HD 94660, HD 75049, and HD 154708

Comparative analysis of the parameters of pulsars with braking indices n>0 and n<0

Boson star superradiance

Cavity optomechanics with directionally squeezed light

Principal components of nuclear mass models

Shape factor and temperature-dependent viscosity analysis for the unsteady flow of magnetic Al2O3–TiO2/C2H6O2–H2O using Legendre wavelet technique

Growth, structural, thermal and THz generation properties of modified DAST, CMST and BMST crystals: A comparative study

SolarAccel: FPGA accelerated 2D cross-correlation of digital images: Application to solar adaptive optics

Centering algorithm of an unresolved primary and satellite system

Disturbances in the Rotational Dynamics of Asteroid (99942) Apophis at its Approach to the Earth in 2029

Studying the Dynamics of Multiplets of Orbital Resonances of Asteroids with Small Perihelion Distances

Manifestations of Anomalous Dissipation in Dusty Plasma in the Solar System: Atmosphereless Cosmic Bodies

Numerical Investigation of Slope Stability in Valles Marineris, Mars

One-Dimensional Model of Vertical Transport of Chemical Components in the Mars Atmosphere up to the Lower Thermosphere

Valley Relief of the Northeastern Part of Terra Cimmeria on Mars

Potentially Primary Xenon Components in Nanodiamond-Enriched Meteorite Fractions: New Isotopic Compositions and Carrier Phases

On the Influence of the Rayleigh–Taylor Instability on the Formation of Dust Clouds in the Mesosphere of Mars

Crater Formed by the Impact of the Luna-25 Spacecraft

Analysis of Spacecraft Flight Trajectories to Venus with a Flyby of Asteroids

Obtaining Plasma–Dust Clouds from Meteoritic Matter, its Analogs and Simulants of Lunar Regolith Using Microwave Discharge

Impact Structures on Venus as a Result of Asteroid Destruction in the Atmosphere

The Influence of the Exosphere of an Active Asteroid on the Polarization of Scattered Light and the Possibility of Estimating Its Properties from Ground-Based Measurements

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