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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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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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Estimation of the Size of an Electric Current with High Helium Abundance inside a Magnetic Cloud

Cosmic research, 2019-11, Vol.57 (6), p.471-472

Yermolaev, Yu. I.

2019

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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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Spectra of Fluctuations of Solar Wind Plasma Parameters near a Shock Wave

Cosmic research, 2024-02, Vol.62 (1), p.1-9

2024

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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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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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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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Development of a Turbulent Cascade behind the Bow Shock under Quiet Conditions in the Solar Wind

Geomagnetism and Aeronomy, 2021-09, Vol.61 (5), p.696-702

2021

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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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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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Does magnetic storm generation depend on the solar wind type?

Geomagnetism and Aeronomy, 2017-09, Vol.57 (5), p.512-518

2017

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Analysis of the Behavior of the Solar Wind Ion Flux in the Region of the Interplanetary Shock Overshoot

Geomagnetism and Aeronomy, 2021-09, Vol.61 (5), p.666-677

2021

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Some Problems of Identifying Types of Large-Scale Solar Wind and Their Role in the Physics of the Magnetosphere: 2

Cosmic research, 2018-09, Vol.56 (5), p.331-342

2018

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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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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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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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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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High-frequency plasma fluctuations in the middle magnetosheath and near its boundaries: Spektr-R observations

Journal of plasma physics, 2017-04, Vol.83 (2), Article 705830204

2017

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Comparison of Magnetic and Plasma Overshoots of Interplanetary Shocks

Cosmic research, 2020-11, Vol.58 (6), p.450-459

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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Features of the Spectral Characteristics of Plasma Fluctuations in Different Large-Scale Streams of the Solar Wind

Geomagnetism and Aeronomy, 2019-03, Vol.59 (2), p.127-135

2019

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Solar and interplanetary sources of geomagnetic storms: Space weather aspects

Izvestiya. Atmospheric and oceanic physics, 2010-12, Vol.46 (7), p.799-819

2010

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Does the duration of the magnetic storm recovery phase depend on the development rate in its main phase? 2. A new method

Geomagnetism and Aeronomy, 2016-05, Vol.56 (3), p.276-280

2016

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

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

Estimation of the Size of an Electric Current with High Helium Abundance inside a Magnetic Cloud

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

Spectra of Fluctuations of Solar Wind Plasma Parameters near a Shock Wave

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

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

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

Development of a Turbulent Cascade behind the Bow Shock under Quiet Conditions in the Solar Wind

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

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”

Does magnetic storm generation depend on the solar wind type?

Analysis of the Behavior of the Solar Wind Ion Flux in the Region of the Interplanetary Shock Overshoot

Some Problems of Identifying Types of Large-Scale Solar Wind and Their Role in the Physics of the Magnetosphere: 2

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

Characteristics of Turbulent Solar Wind Flow in Plasma Compression Regions

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

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

High-frequency plasma fluctuations in the middle magnetosheath and near its boundaries: Spektr-R observations

Comparison of Magnetic and Plasma Overshoots of Interplanetary Shocks

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

Features of the Spectral Characteristics of Plasma Fluctuations in Different Large-Scale Streams of the Solar Wind

Solar and interplanetary sources of geomagnetic storms: Space weather aspects

Does the duration of the magnetic storm recovery phase depend on the development rate in its main phase? 2. A new method

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