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Possible difference in the formation of coronal mass ejections of two types

Solar-terrestrial physics, 2022-06, Vol.8 (2), p.10-19

2022

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Fine Structure of Interplanetary Shock Front—Results from BMSW Experiment with High Time Resolution

Journal of geophysical research. Space physics, 2019-11, Vol.124 (11), p.8191-8207

2019

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Features of the Dynamics of a Shock Excited by Fast Coronal Mass Ejections

Cosmic research, 2019-05, Vol.57 (3), p.143-155

2019

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Correspondence of a global isolated substorm to the McPherron statistical model

Solar-terrestrial physics, 2022-01, Vol.8 (2), p.37-46

2022

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Evidence for shock generation in the solar corona in the absence of coronal mass ejections

Astronomy reports, 2017-09, Vol.61 (9), p.805-819

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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Initial formation of an “impulsive” coronal mass ejection

Astronomy reports, 2016-11, Vol.60 (11), p.1016-1027

2016

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Possible reasons for the frequency splitting of the harmonics of type II solar radio bursts

Astronomy reports, 2016, Vol.60 (1), p.163-173

2016

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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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Physical differences between the initial phase of the formation of two types of coronal mass ejections

Astronomy reports, 2014-04, Vol.58 (4), p.260-271

2014

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Differences in the development of the initial phase of the formation of two types of coronal mass ejections

Cosmic research, 2015, Vol.53 (1), p.21-30

2015

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The role of rising magnetic tubes in the formation of impulsive coronal mass ejections

Astronomy reports, 2013-11, Vol.57 (11), p.860-871

2013

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Fine structure of the interplanetary shock front according to measurements of the ion flux of the solar wind with high time resolution

Cosmic research, 2017, Vol.55 (1), p.30-45

2017

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Relations estimated at shock discontinuities excited by coronal mass ejections

Astronomy reports, 2011-04, Vol.55 (4), p.359-373

2011

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Blast-wave and piston shocks connected with the formation and propagation of a coronal mass ejection

Astronomy reports, 2013-02, Vol.57 (2), p.142-151

2013

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Structure of the Front of a Collisionless Oblique Interplanetary Shock Wave from High Time Resolution Measurements of Solar-Wind Plasma Parameters

Geomagnetism and Aeronomy, 2018-12, Vol.58 (6), p.728-736

2018

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Fine structure of interplanetary shock fronts from the data of the BMSW instrument of the PLASMA-F experiment

Cosmic research, 2017-11, Vol.55 (6), p.396-402

2017

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Some properties of the development of the perturbed zone and shock preceding a coronal mass ejection

Astronomy reports, 2011-11, Vol.55 (11), p.1038-1050

2011

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Effect of reflected ions on the formation of the structure of interplanetary quasi-perpendicular shocks for Mach numbers lower than the first critical mach number

Cosmic research, 2017-11, Vol.55 (6), p.403-416

2017

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On the formation mechanism of the sporadic solar wind

Geomagnetism and Aeronomy, 2011-12, Vol.51 (8), p.1083-1094

2011

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Prediction of Magnetospheric Disturbances Caused by a Quasi-Stationary Solar Wind

Kōngjiān kēxué xuébào, 2005, Vol.25 (5), p.374

2005

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The structure of the coronal-streamer belt

Astronomy reports, 2005-01, Vol.49 (1), p.71-78

2005

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On the structure of coronal streamer belts

Journal of Geophysical Research, 1998-02, Vol.103 (A2), p.2021-2027

Eselevich, V. G.

1998

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The Physical Foundation of Forecasting Disturbances in the Geospace From Solar Disk Characteristics

Kōngjiān kēxué xuébào, 2005, Vol.25 (5), p.356

2005

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Additional plasma streams with steep fronts in structures of enhanced brightness in the coronal streamer belt

Astronomy reports, 2004-08, Vol.48 (8), p.688-698

2004

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Possible difference in the formation of coronal mass ejections of two types

Fine Structure of Interplanetary Shock Front—Results from BMSW Experiment with High Time Resolution

Features of the Dynamics of a Shock Excited by Fast Coronal Mass Ejections

Correspondence of a global isolated substorm to the McPherron statistical model

Evidence for shock generation in the solar corona in the absence of coronal mass ejections

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

Initial formation of an “impulsive” coronal mass ejection

Possible reasons for the frequency splitting of the harmonics of type II solar radio bursts

Comparison of Magnetic and Plasma Overshoots of Interplanetary Shocks

Physical differences between the initial phase of the formation of two types of coronal mass ejections

Differences in the development of the initial phase of the formation of two types of coronal mass ejections

The role of rising magnetic tubes in the formation of impulsive coronal mass ejections

Fine structure of the interplanetary shock front according to measurements of the ion flux of the solar wind with high time resolution

Relations estimated at shock discontinuities excited by coronal mass ejections

Blast-wave and piston shocks connected with the formation and propagation of a coronal mass ejection

Structure of the Front of a Collisionless Oblique Interplanetary Shock Wave from High Time Resolution Measurements of Solar-Wind Plasma Parameters

Fine structure of interplanetary shock fronts from the data of the BMSW instrument of the PLASMA-F experiment

Some properties of the development of the perturbed zone and shock preceding a coronal mass ejection

Effect of reflected ions on the formation of the structure of interplanetary quasi-perpendicular shocks for Mach numbers lower than the first critical mach number

On the formation mechanism of the sporadic solar wind

Prediction of Magnetospheric Disturbances Caused by a Quasi-Stationary Solar Wind

The structure of the coronal-streamer belt

On the structure of coronal streamer belts

The Physical Foundation of Forecasting Disturbances in the Geospace From Solar Disk Characteristics

Additional plasma streams with steep fronts in structures of enhanced brightness in the coronal streamer belt

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