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On formation of a shock wave in front of a coronal mass ejection with velocity exceeding the critical one

Geophysical research letters, 2008-11, Vol.35 (22), p.L22105-n/a

2008

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Observations of a Flare-Generated Blast Wave in a Pseudo Coronal Mass Ejection Event

Solar physics, 2019-06, Vol.294 (6), p.1-20, Article 73

2019

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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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Evidence of a blast shock wave formation in a “CME–streamer” interaction

Advances in space research, 2015-12, Vol.56 (12), p.2793-2803

2015

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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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Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. III. Shock-Associated CME/EUV Wave in an Event with a Two-Component EUV Transient

Solar physics, 2011-11, Vol.273 (2), p.461-477

2011

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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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On the possible reason for the formation of impulsive coronal mass ejections

Advances in space research, 2015-02, Vol.55 (3), p.949-957

2015

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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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Study of the nonradial directional property of the rays of the streamer belt and chains in the solar corona

Solar physics, 2002-07, Vol.208 (1), p.5-16

2002

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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 formation of a shock wave in front of a coronal mass ejection with velocity exceeding the critical one

Observations of a Flare-Generated Blast Wave in a Pseudo Coronal Mass Ejection Event

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

Evidence of a blast shock wave formation in a “CME–streamer” interaction

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

Correspondence of a global isolated substorm to the McPherron statistical model

Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. III. Shock-Associated CME/EUV Wave in an Event with a Two-Component EUV Transient

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

On the possible reason for the formation of impulsive 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

Study of the nonradial directional property of the rays of the streamer belt and chains in the solar corona

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

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