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Forbush decreases caused by paired interacting solar wind disturbances

Monthly notices of the Royal Astronomical Society, 2022-03, Vol.511 (4), p.5897-5908

2022

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Forbush decreases associated with coronal mass ejections from active and non-active regions: statistical comparison

Monthly notices of the Royal Astronomical Society, 2022-08, Vol.515 (3), p.4430-4444

2022

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Statistical comparison of time profiles of Forbush decreases associated with coronal mass ejections and streams from coronal holes in solar cycles 23–24

Monthly notices of the Royal Astronomical Society, 2023-03, Vol.521 (3), p.4544-4560

2023

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Average characteristics of high-energy magnetospheric electron flux enhancements and the parameters of near-Earth and interplanetary medium in 1987–2021

Monthly notices of the Royal Astronomical Society, 2022-09, Vol.516 (4), p.4782-4791

2022

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Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 24

Solar physics, 2024-03, Vol.299 (3), p.40, Article 40

2024

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Ring of Stations Method in Cosmic Rays Variations Research

Solar physics, 2020-05, Vol.295 (5), Article 69

2020

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An Empirical Model for Estimating the Velocities and Delays of Interplanetary Coronal Mass Ejections

Geomagnetism and Aeronomy, 2023-09, Vol.63 (5), p.564-573

2023

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Forbush Effects and Geomagnetic Storms

Geomagnetism and Aeronomy, 2024-06, Vol.64 (3), p.289-301

2024

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Abnormal Quasi-Recurrent Variations of Cosmic Rays in September 2014–February 2015

Geomagnetism and Aeronomy, 2024-04, Vol.64 (2), p.211-223

2024

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Geoefficiency of Sporadic Phenomena in Solar Cycle 24

Geomagnetism and Aeronomy, 2023-08, Vol.63 (4), p.486-496

2023

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Solar Wind Low-Temperature Periods and Forbush Decreases: a Statistical Comparison

Geomagnetism and Aeronomy, 2024-10, Vol.64 (5), p.626-638

2024

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Solar Proton Events and Forbush Decreases with the Same Sources

Bulletin of the Russian Academy of Sciences. Physics, 2023-07, Vol.87 (7), p.938-941

2023

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Some Features of Interacting Solar Wind Disturbances

Geomagnetism and Aeronomy, 2024-08, Vol.64 (4), p.457-467

2024

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Forbush Decreases and Geomagnetic Disturbances: 1. Events Associated with Different Types of Solar and Interplanetary Sources

Geomagnetism and Aeronomy, 2023-12, Vol.63 (6), p.686-700

2023

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Forbush Decreases and Geomagnetic Disturbances: 2. Comparison of Solar Cycles 23–24 and Events with Sudden and Gradual Commencement

Geomagnetism and Aeronomy, 2024-02, Vol.64 (1), p.32-43

2024

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Using Data from a Ground-Based Network of Detectors and the PAMELA and AMS-02 Experiments to Compare Long-Term Variations in the Cosmic Ray Flux

Bulletin of the Russian Academy of Sciences. Physics, 2021-09, Vol.85 (9), p.1039-1041

2021

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Main Time Characteristics of Cosmic Ray Variations and Related Parameters in Magnetic Clouds

Geomagnetism and Aeronomy, 2024-02, Vol.64 (1), p.24-31

2024

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Forbush Effects Observed by the Helios Spacecraft

Geomagnetism and Aeronomy, 2022-08, Vol.62 (4), p.375-381

2022

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Forbush Decreases Associated with Coronal Holes, Coronal Ejections from Active Regions, and Filament Eruptions: Comparison in Solar Cycles 23 and 24

Geomagnetism and Aeronomy, 2023-09, Vol.63 (5), p.547-563

2023

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Influence of Interacting Solar Wind Disturbances on the Variations in Galactic Cosmic Rays

Geomagnetism and Aeronomy, 2021-11, Vol.61 (6), p.792-800

2021

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Selection of the Solar-Diurnal Anisotropy of Cosmic Rays by Local and Global Methods

Geomagnetism and Aeronomy, 2023-06, Vol.63 (3), p.268-282

2023

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Forbush Effects Created by Coronal Mass Ejections with Magnetic Clouds

Geomagnetism and Aeronomy, 2021-09, Vol.61 (5), p.678-687

2021

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Development of Forbush Decreases Associated with Coronal Ejections from Active Regions and non-Active Regions

Geomagnetism and Aeronomy, 2022-12, Vol.62 (Suppl 1), p.S40-S53

2022

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Features of Increases in the Fluxes of Magnetospheric Electrons with Energies >2 MeV in the Geostationary Orbit in 2009

Geomagnetism and Aeronomy, 2022-12, Vol.62 (8), p.1096-1104

2022

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Features of the Behavior of Time Parameters of Forbush Decreases Associated with Different Types of Solar and Interplanetary Sources

Geomagnetism and Aeronomy, 2022-02, Vol.62 (1-2), p.17-31

2022

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Forbush decreases caused by paired interacting solar wind disturbances

Forbush decreases associated with coronal mass ejections from active and non-active regions: statistical comparison

Statistical comparison of time profiles of Forbush decreases associated with coronal mass ejections and streams from coronal holes in solar cycles 23–24

Average characteristics of high-energy magnetospheric electron flux enhancements and the parameters of near-Earth and interplanetary medium in 1987–2021

Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 24

Ring of Stations Method in Cosmic Rays Variations Research

An Empirical Model for Estimating the Velocities and Delays of Interplanetary Coronal Mass Ejections

Forbush Effects and Geomagnetic Storms

Abnormal Quasi-Recurrent Variations of Cosmic Rays in September 2014–February 2015

Geoefficiency of Sporadic Phenomena in Solar Cycle 24

Solar Wind Low-Temperature Periods and Forbush Decreases: a Statistical Comparison

Solar Proton Events and Forbush Decreases with the Same Sources

Some Features of Interacting Solar Wind Disturbances

Forbush Decreases and Geomagnetic Disturbances: 1. Events Associated with Different Types of Solar and Interplanetary Sources

Forbush Decreases and Geomagnetic Disturbances: 2. Comparison of Solar Cycles 23–24 and Events with Sudden and Gradual Commencement

Using Data from a Ground-Based Network of Detectors and the PAMELA and AMS-02 Experiments to Compare Long-Term Variations in the Cosmic Ray Flux

Main Time Characteristics of Cosmic Ray Variations and Related Parameters in Magnetic Clouds

Forbush Effects Observed by the Helios Spacecraft

Forbush Decreases Associated with Coronal Holes, Coronal Ejections from Active Regions, and Filament Eruptions: Comparison in Solar Cycles 23 and 24

Influence of Interacting Solar Wind Disturbances on the Variations in Galactic Cosmic Rays

Selection of the Solar-Diurnal Anisotropy of Cosmic Rays by Local and Global Methods

Forbush Effects Created by Coronal Mass Ejections with Magnetic Clouds

Development of Forbush Decreases Associated with Coronal Ejections from Active Regions and non-Active Regions

Features of Increases in the Fluxes of Magnetospheric Electrons with Energies >2 MeV in the Geostationary Orbit in 2009

Features of the Behavior of Time Parameters of Forbush Decreases Associated with Different Types of Solar and Interplanetary Sources

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