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The Global Survey Method Applied to Ground-level Cosmic Ray Measurements

Solar physics, 2018-04, Vol.293 (4), p.1-23, Article 68

2018

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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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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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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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Large Scale Modulation: View from the Earth Points

Physics of atomic nuclei, 2021-11, Vol.84 (6), p.1159-1170

2021

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Coronal Mass Ejections and Non-recurrent Forbush Decreases

Solar physics, 2014-10, Vol.289 (10), p.3949-3960

2014

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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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Solar wind temperature–velocity relationship over the last five solar cycles and Forbush decreases associated with different types of interplanetary disturbance

Monthly notices of the Royal Astronomical Society, 2021-01, Vol.500 (3), p.2786-2797

2021

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Galactic Cosmic Ray Density Variations in Magnetic Clouds

Solar physics, 2015-05, Vol.290 (5), p.1429-1444

2015

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Global Survey Method for the World Network of Neutron Monitors

Geomagnetism and Aeronomy, 2018-05, Vol.58 (3), p.356-372

2018

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A Method for Correcting Neutron Monitor Data for the Snow Effect

Geomagnetism and Aeronomy, 2022-12, Vol.62 (6), p.737-742

2022

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

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

2024

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On recurrent Forbush Decreases

Journal of physics. Conference series, 2019-02, Vol.1181 (1), p.12009

2019

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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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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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Similarities and Differences between Forbush Decreases Associated with Streams from Coronal Holes, Filament Ejections, and Ejections from Active Regions

Geomagnetism and Aeronomy, 2022-06, Vol.62 (3), p.159-177

2022

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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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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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Main Properties of Forbush Effects Related to High-Speed Streams from Coronal Holes

Geomagnetism and Aeronomy, 2018-03, Vol.58 (2), p.154-168

2018

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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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The Global Survey Method Applied to Ground-level Cosmic Ray Measurements

Forbush decreases caused by paired interacting solar wind disturbances

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

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

Large Scale Modulation: View from the Earth Points

Coronal Mass Ejections and Non-recurrent Forbush Decreases

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

Solar wind temperature–velocity relationship over the last five solar cycles and Forbush decreases associated with different types of interplanetary disturbance

Galactic Cosmic Ray Density Variations in Magnetic Clouds

Global Survey Method for the World Network of Neutron Monitors

A Method for Correcting Neutron Monitor Data for the Snow Effect

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

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

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

On recurrent Forbush Decreases

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

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

Forbush Effects Created by Coronal Mass Ejections with Magnetic Clouds

Similarities and Differences between Forbush Decreases Associated with Streams from Coronal Holes, Filament Ejections, and Ejections from Active Regions

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

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

Main Properties of Forbush Effects Related to High-Speed Streams from Coronal Holes

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

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