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Kinematics of Flare Ribbons during Eruption of Solar Prominences

Geomagnetism and Aeronomy, 2024-08, Vol.64 (4), p.449-456

Filippov, B. P.

2024

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Influence of the Geometrical Shape of a Prominence and Structure of the Coronal Magnetic Field on the Probability of Eruption, Flare Development, and Coronal Mass Ejection

Geomagnetism and Aeronomy, 2024-02, Vol.64 (1), p.11-18

Filippov, B. P.

2024

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Failed Eruptions of Solar Filaments

Astronomy reports, 2020-03, Vol.64 (3), p.272-279

Filippov, B. P.

2020

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Mass ejections from the solar atmosphere

Physics Uspekhi, 2019-09, Vol.62 (9), p.847-864

Filippov, B P

2019

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Manifestation of Magnetic Flux Ropes in the Structure of Solar Prominences

Geomagnetism and Aeronomy, 2023-04, Vol.63 (2), p.146-152

Filippov, B. P.

2023

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Dependence of the Occurrence of Coronal Mass Ejections on the Initial Length of the Eruptive Prominence

Geomagnetism and Aeronomy, 2022-06, Vol.62 (3), p.151-158

Filippov, B. P.

2022

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Low Values of the Critical Decay Index of the Magnetic Field in Prominence Eruptions

Geomagnetism and Aeronomy, 2021-12, Vol.61 (Suppl 1), p.S16-S23

Filippov, B. P.

2021

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“False” Sigmoids in the Solar Corona

Astronomy reports, 2019-09, Vol.63 (9), p.778-785

Filippov, B. P.

2019

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Eruptive Instability of the Magnetic-Flux Rope: Gravitational Force and Mass-Unloading

Solar physics, 2019-03, Vol.294 (3), p.1-10, Article 35

2019

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Morphological indictors of the chirality of solar filaments

Astronomy reports, 2017-10, Vol.61 (10), p.891-900

Filippov, B. P.

2017

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A critical height of quiescent prominences before eruption

Journal of Geophysical Research: Space Physics, 2001-11, Vol.106 (A11), p.25177-25184

2001

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Method for the determination of the height of a solar filament

Geomagnetism and Aeronomy, 2016, Vol.56 (1), p.1-7

Filippov, B. P.

2016

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Neutral surfaces of coronal magnetic field and solar filaments

Cosmic research, 2017, Vol.55 (1), p.12-19

Filippov, B. P.

2017

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The initial trajectories of eruptive solar prominences

Astronomy reports, 2016-03, Vol.60 (3), p.356-365

Filippov, B. P.

2016

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Two Scenarios for the Eruption of Magnetic Flux Ropes in the Solar Atmosphere

Astronomy reports, 2018-05, Vol.62 (5), p.359-365

2018

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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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Height of a solar filament before eruption

Astronomy reports, 2013-10, Vol.57 (10), p.778-785

Filippov, B. P.

2013

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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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Non-radial motion of eruptive filaments

Solar physics, 2001-10, Vol.203 (1), p.119-130

2001

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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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Some properties of the joining of solar filaments

Astronomy reports, 2011-06, Vol.55 (6), p.541-550

Filippov, B. P.

2011

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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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Influence of the geometrical shape of a prominence and the structure of the coronal magnetic field on the probability of eruption, flare and coronal mass ejection development

Geomagnetizm i aėronomija, 2024-02, Vol.64 (1), p.13-22

Filippov, B. P.

2024

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Manifestation of Magnetic Flux Ropes in the Structure of Solar Prominences

Geomagnetizm i aėronomija, 2023-03, Vol.63 (2), p.174-180

Filippov, B. P.

2023

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Geometry of solar coronal rays

AIP Conference Proceedings, 2016, Vol.1714 (1)

2016

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Kinematics of Flare Ribbons during Eruption of Solar Prominences

Influence of the Geometrical Shape of a Prominence and Structure of the Coronal Magnetic Field on the Probability of Eruption, Flare Development, and Coronal Mass Ejection

Failed Eruptions of Solar Filaments

Mass ejections from the solar atmosphere

Manifestation of Magnetic Flux Ropes in the Structure of Solar Prominences

Dependence of the Occurrence of Coronal Mass Ejections on the Initial Length of the Eruptive Prominence

Low Values of the Critical Decay Index of the Magnetic Field in Prominence Eruptions

“False” Sigmoids in the Solar Corona

Eruptive Instability of the Magnetic-Flux Rope: Gravitational Force and Mass-Unloading

Morphological indictors of the chirality of solar filaments

A critical height of quiescent prominences before eruption

Method for the determination of the height of a solar filament

Neutral surfaces of coronal magnetic field and solar filaments

The initial trajectories of eruptive solar prominences

Two Scenarios for the Eruption of Magnetic Flux Ropes in the Solar Atmosphere

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

Height of a solar filament before eruption

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

Non-radial motion of eruptive filaments

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

Some properties of the joining of solar filaments

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

Influence of the geometrical shape of a prominence and the structure of the coronal magnetic field on the probability of eruption, flare and coronal mass ejection development

Manifestation of Magnetic Flux Ropes in the Structure of Solar Prominences

Geometry of solar coronal rays

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