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Absorption Phenomena and a Probable Blast Wave in the 13 July 2004 Eruptive Event

Solar physics, 2008-12, Vol.253 (1-2), p.263-290

2008

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Prediction of Geomagnetic Storms Associated with Interplanetary Coronal Mass Ejections

Astronomy reports, 2024-02, Vol.68 (2), p.192-199

2024

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CORONAS-F/SPIRIT EUV observations of October–November 2003 solar eruptive events in combination with SOHO/EIT data

Journal of Geophysical Research - Space Physics, 2005-09, Vol.110 (A9), p.A09S07-n/a

2005

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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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Search for Solar Sources of Interplanetary Coronal Mass Ejections Using the Reverse Model of Magnetodynamic Interaction of the Solar Wind in the Heliosphere

Astronomy reports, 2023-03, Vol.67 (3), p.280-287

2023

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Development of a Fast CME and Properties of a Related Interplanetary Transient

Solar physics, 2019-10, Vol.294 (10), p.1-34, Article 139

2019

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Fe Ion Composition in Solar-Wind Streams in the Solar Corona and Heliosphere

Cosmic research, 2023-02, Vol.61 (1), p.8-17

2023

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A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. I. Unusual History of an Eruptive Filament

Solar physics, 2014, Vol.289 (1), p.289-318

2014

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Formation of Coronal Mass Ejections in the Solar Corona and Propagation of the Resulting Plasma Streams in the Heliosphere

Plasma physics reports, 2019-10, Vol.45 (10), p.889-920

2019

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A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. IV. Unusual Magnetic Cloud and Overall Scenario

Solar physics, 2014-12, Vol.289 (12), p.4653-4673

2014

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A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. II. CMEs, Shock Waves, and Drifting Radio Bursts

Solar physics, 2014-04, Vol.289 (4), p.1279-1312

2014

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Geomagnetic Storms and Forbush-Decreases Related to Single and Complex Transient Structures of Solar Wind

Bulletin of the Lebedev Physics Institute, 2020-03, Vol.47 (3), p.92-96

2020

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A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. III. Catastrophe of the Eruptive Filament at a Magnetic Null Point and Formation of an Opposite-Handedness CME

Solar physics, 2014-10, Vol.289 (10), p.3747-3772

2014

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Dynamic 10 MK plasma structures observed in monochromatic full-Sun images by the SPIRIT spectroheliograph on the CORONAS-F mission

Monthly notices of the Royal Astronomical Society, 2003-01, Vol.338 (1), p.67-71

2003

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Features of solar wind streams on June 21–28, 2015 as a result of interactions between coronal mass ejections and recurrent streams from coronal holes

Cosmic research, 2017-11, Vol.55 (6), p.389-395

2017

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Large-Scale and Small-Scale Solar Wind Structures Formed during Interaction of Streams in the Heliosphere

Cosmic research, 2019, Vol.57 (1), p.18-28

2019

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Possible causes of the discrepancy between the predicted and observed parameters of high-speed solar wind streams

Cosmic research, 2017, Vol.55 (1), p.20-29

2017

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Prediction of geoeffective solar wind streams near earth according to solar observational data

Bulletin of the Lebedev Physics Institute, 2017-10, Vol.44 (10), p.303-307

2017

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Identification of coronal sources of the solar wind from solar images in the EUV spectral range

Cosmic research, 2015, Vol.53 (1), p.47-58

2015

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Interaction of high-speed and transient fluxes of solar wind at the maximum of solar cycle 24

Bulletin of the Lebedev Physics Institute, 2016-09, Vol.43 (9), p.287-290

2016

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The effect of solar activity on the evolution of solar wind parameters during the rise of the 24th cycle

Solar system research, 2016, Vol.50 (1), p.44-55

2016

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The TESIS experiment on the CORONAS-PHOTON spacecraft

Solar system research, 2011-04, Vol.45 (2), p.162-173

2011

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Main Results of the SPIRIT Experiment Onboard the CORONAS-F Satellite

Solar system research, 2005-11, Vol.39 (6), p.442-452

2005

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Search for Solar Sources of Interplanetary Coronal Mass Ejections Using the Reverse Model of Magnetodynamic Interaction of the Solar Wind in the Heliosphere

Астрономический журнал, 2023-03, Vol.100 (3), p.289-296

2023

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Observations of Solar EUV Radiation with the CORONAS-F/SPIRIT and SOHO/EIT Instruments

Solar system research, 2005-11, Vol.39 (6), p.489-500

2005

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Absorption Phenomena and a Probable Blast Wave in the 13 July 2004 Eruptive Event

Prediction of Geomagnetic Storms Associated with Interplanetary Coronal Mass Ejections

CORONAS-F/SPIRIT EUV observations of October–November 2003 solar eruptive events in combination with SOHO/EIT data

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

Search for Solar Sources of Interplanetary Coronal Mass Ejections Using the Reverse Model of Magnetodynamic Interaction of the Solar Wind in the Heliosphere

Development of a Fast CME and Properties of a Related Interplanetary Transient

Fe Ion Composition in Solar-Wind Streams in the Solar Corona and Heliosphere

A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. I. Unusual History of an Eruptive Filament

Formation of Coronal Mass Ejections in the Solar Corona and Propagation of the Resulting Plasma Streams in the Heliosphere

A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. IV. Unusual Magnetic Cloud and Overall Scenario

A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. II. CMEs, Shock Waves, and Drifting Radio Bursts

Geomagnetic Storms and Forbush-Decreases Related to Single and Complex Transient Structures of Solar Wind

A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. III. Catastrophe of the Eruptive Filament at a Magnetic Null Point and Formation of an Opposite-Handedness CME

Dynamic 10 MK plasma structures observed in monochromatic full-Sun images by the SPIRIT spectroheliograph on the CORONAS-F mission

Features of solar wind streams on June 21–28, 2015 as a result of interactions between coronal mass ejections and recurrent streams from coronal holes

Large-Scale and Small-Scale Solar Wind Structures Formed during Interaction of Streams in the Heliosphere

Possible causes of the discrepancy between the predicted and observed parameters of high-speed solar wind streams

Prediction of geoeffective solar wind streams near earth according to solar observational data

Identification of coronal sources of the solar wind from solar images in the EUV spectral range

Interaction of high-speed and transient fluxes of solar wind at the maximum of solar cycle 24

The effect of solar activity on the evolution of solar wind parameters during the rise of the 24th cycle

The TESIS experiment on the CORONAS-PHOTON spacecraft

Main Results of the SPIRIT Experiment Onboard the CORONAS-F Satellite

Search for Solar Sources of Interplanetary Coronal Mass Ejections Using the Reverse Model of Magnetodynamic Interaction of the Solar Wind in the Heliosphere

Observations of Solar EUV Radiation with the CORONAS-F/SPIRIT and SOHO/EIT Instruments

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