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Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms

Journal of Geophysical Research: Space Physics, 2012-09, Vol.117 (A9), p.n/a

2012

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Specific interplanetary conditions for CIR-, Sheath-, and ICME-induced geomagnetic storms obtained by double superposed epoch analysis

Annales geophysicae (1988), 2010-12, Vol.28 (12), p.2177-2186

2010

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Occurrence rate of extreme magnetic storms

Journal of geophysical research. Space physics, 2013-08, Vol.118 (8), p.4760-4765

2013

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Dynamics of large-scale solar wind streams obtained by the double superposed epoch analysis

Journal of geophysical research. Space physics, 2015-09, Vol.120 (9), p.7094-7106

2015

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Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 2. Comparisons of CIRs vs. Sheaths and MCs vs. Ejecta

Solar physics, 2017-12, Vol.292 (12), p.1-14, Article 193

2017

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Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 3. Deflection of the Velocity Vector

Solar physics, 2018-06, Vol.293 (6), p.1-12, Article 91

2018

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Dynamics of Large‐Scale Solar‐Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance

Journal of geophysical research. Space physics, 2020-07, Vol.125 (7), p.n/a

2020

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Comment on “A Statistical Study of the Plasma and Composition Distribution inside Magnetic Clouds: 1998–2011” by J. Huang et al

Geomagnetism and Aeronomy, 2021-05, Vol.61 (3), p.416-417

2021

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Influence of the interplanetary driver type on the durations of the main and recovery phases of magnetic storms

Journal of geophysical research. Space physics, 2014-10, Vol.119 (10), p.8126-8136

2014

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Medium-Scale Variations of Helium Abundance inside Coronal Mass Ejections

Cosmic research, 2022-12, Vol.60 (6), p.452-460

2022

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Dynamics of Interplanetary Parameters and Geomagnetic Indices during Magnetic Storms Induced by Different Types of Solar Wind

Geomagnetism and Aeronomy, 2019-11, Vol.59 (6), p.639-650

2019

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Statistical study of interplanetary condition effect on geomagnetic storms

Cosmic research, 2010-12, Vol.48 (6), p.485-500

2010

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Statistical Study of the Effect of Different Solar Wind Types on Magnetic Storm Generation During 1995–2016

Geomagnetism and Aeronomy, 2018-12, Vol.58 (6), p.737-743

2018

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Helium Abundance Variations in Interplanetary Coronal Mass Ejections

Cosmic research, 2022, Vol.60 (2), p.67-72

2022

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Recovery phase of magnetic storms induced by different interplanetary drivers

Journal of Geophysical Research: Space Physics, 2012-08, Vol.117 (A8), p.n/a

2012

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Modern view of the solar wind from micro to macro scales

Physics Uspekhi, 2020-11, Vol.63 (8), p.801-811

2020

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Variations of Protons and Doubly Ionized Helium Ions in the Solar Wind

Cosmic research, 2021-11, Vol.59 (6), p.415-426

2021

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Characteristics of Turbulent Solar Wind Flow in Plasma Compression Regions

Cosmic research, 2020-11, Vol.58 (6), p.468-477

2020

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Dependence of the Properties of a Turbulent Cascade behind the Bow Shock on the Dynamics of the Solar Wind Parameters

Cosmic research, 2020-11, Vol.58 (6), p.478-486

2020

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Turbulent Cascade in the Magnetosheath Affected by the Solar Wind’s Plasma Turbulence

Cosmic research, 2019-11, Vol.57 (6), p.443-450

2019

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Catalog of large-scale solar wind phenomena during 1976–2000

Cosmic research, 2009-04, Vol.47 (2), p.81-94

2009

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Relationship between the Parameters of Various Solar Wind Types and Geomagnetic Activity Indices

Cosmic research, 2018-11, Vol.56 (6), p.426-433

2018

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Some Problems of Identifying Types of Large-Scale Solar Wind and Their Role in Magnetosphere Physics: 3. Use of Published Incorrect Data

Cosmic research, 2020-09, Vol.58 (5), p.338-356

2020

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Some Problems of Identifying Types of Large-Scale Solar Wind and Their Role in the Physics of the Magnetosphere: 4. The “Lost Driver”

Cosmic research, 2020-11, Vol.58 (6), p.492-500

2020

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Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams

Cosmic research, 2019-11, Vol.57 (6), p.434-442

2019

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Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms

Specific interplanetary conditions for CIR-, Sheath-, and ICME-induced geomagnetic storms obtained by double superposed epoch analysis

Occurrence rate of extreme magnetic storms

Dynamics of large-scale solar wind streams obtained by the double superposed epoch analysis

Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 2. Comparisons of CIRs vs. Sheaths and MCs vs. Ejecta

Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 3. Deflection of the Velocity Vector

Dynamics of Large‐Scale Solar‐Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance

Comment on “A Statistical Study of the Plasma and Composition Distribution inside Magnetic Clouds: 1998–2011” by J. Huang et al

Influence of the interplanetary driver type on the durations of the main and recovery phases of magnetic storms

Medium-Scale Variations of Helium Abundance inside Coronal Mass Ejections

Dynamics of Interplanetary Parameters and Geomagnetic Indices during Magnetic Storms Induced by Different Types of Solar Wind

Statistical study of interplanetary condition effect on geomagnetic storms

Statistical Study of the Effect of Different Solar Wind Types on Magnetic Storm Generation During 1995–2016

Helium Abundance Variations in Interplanetary Coronal Mass Ejections

Recovery phase of magnetic storms induced by different interplanetary drivers

Modern view of the solar wind from micro to macro scales

Variations of Protons and Doubly Ionized Helium Ions in the Solar Wind

Characteristics of Turbulent Solar Wind Flow in Plasma Compression Regions

Dependence of the Properties of a Turbulent Cascade behind the Bow Shock on the Dynamics of the Solar Wind Parameters

Turbulent Cascade in the Magnetosheath Affected by the Solar Wind’s Plasma Turbulence

Catalog of large-scale solar wind phenomena during 1976–2000

Relationship between the Parameters of Various Solar Wind Types and Geomagnetic Activity Indices

Some Problems of Identifying Types of Large-Scale Solar Wind and Their Role in Magnetosphere Physics: 3. Use of Published Incorrect Data

Some Problems of Identifying Types of Large-Scale Solar Wind and Their Role in the Physics of the Magnetosphere: 4. The “Lost Driver”

Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams

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