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Interrelationships between Halo-Type Coronal Mass Ejections and Solar Flares Based on Observations in the 23rd and 24th Cycles

Astrophysics, 2021-02, Vol.64 (1), p.61-70

2021

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New classification parameter of solar flares based on the maximum flux in soft X-rays and on duration of flare

Journal of astrophysics and astronomy, 2020-12, Vol.41 (1), Article 3

Bruevich, E. A.

2020

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Lyman Decrements of Neutral Hydrogen Lines in the Spectrum of the Sun Based on SDO/EVE Observations. Variations During the 24-th Solar Cycle and in Individual Flares of Classes M and X

Astrophysics, 2019-09, Vol.62 (3), p.377-386

2019

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Powerful Solar Flares in September 2017. Comparison with the Largest Flares in Cycle 24

Astrophysics, 2018-06, Vol.61 (2), p.241-253

2018

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Changed Relation between Solar 10.7-cm Radio Flux and some Activity Indices which describe the Radiation at Different Altitudes of Atmosphere during Cycles 21–23

Journal of astrophysics and astronomy, 2014-03, Vol.35 (1), p.1-15

2014

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Flare Activity of the Sun and Variations in its UV Emission During Cycle 24

Astrophysics, 2017-09, Vol.60 (3), p.387-400

2017

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Flux Variations in Lines of Solar EUV Radiation beyond Flares in Cycle 24

Geomagnetism and Aeronomy, 2019-03, Vol.59 (2), p.155-161

2019

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Cyclic Variations in the Solar Radiation Fluxes at the Beginning of the 21st Century

Moscow University physics bulletin, 2018-03, Vol.73 (2), p.216-222

2018

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Variations of Solar EUV Radiation Fluxes in Hydrogen Lines from Observations by the TIMED Satellite in Cycle 23 and by SDO/EVE in Cycle 24

Geomagnetism and Aeronomy, 2019-12, Vol.59 (8), p.1048-1054

2019

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Hysteresis Effect in the Activity Indices of the Atmospheres of the Sun and Solar-Type Stars During the Rising and Falling Phases of Cycles

Astrophysics, 2016-09, Vol.59 (3), p.369-382

2016

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Comparative Analysis of the Activity Cycles of the Atmospheres of the Sun and of Stars of the Solar-Type

Astrophysics, 2016-03, Vol.59 (1), p.101-113

2016

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Methods for Monitoring Strong Space Weather Disturbances to Support International Air Navigation

Russian meteorology and hydrology, 2021-01, Vol.46 (3), p.205-211

2021

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General trends in the change in solar activity indices in the period from the late XX to early XXI century

Geomagnetism and Aeronomy, 2015-12, Vol.55 (8), p.1060-1065

2015

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Hysteresis of indices of solar and ionospheric activity during 11-year cycles

Geomagnetism and Aeronomy, 2016-12, Vol.56 (8), p.1075-1081

2016

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Solar Flares in Extreme Ultraviolet and X-Ray Bands Based on SDO and TIMED Satellite Data

Geomagnetism and aeronomy, 2021-12, Vol.61 (8), p.1122-1127

2021

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24th Cycle of Solar Activity: Geoefficiency of Flares

Geomagnetism and aeronomy, 2020-12, Vol.60 (7), p.876-880

2020

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Solar-Flux Variation in Helium Lines According to SDO/EVE Data in the 24th Cycle and the Forecast for Different Levels of Solar Activity. Lyman Decrements of Hydrogen and Helium Lines

Geomagnetism and aeronomy, 2020-12, Vol.60 (7), p.966-973

2020

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Levels of coronal and chromospheric activity in late-type stars and various types of dynamo waves

Astronomy reports, 2001-09, Vol.45 (9), p.718-728

2001

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Spotting in stars with a low level of activity, close to solar activity

Astrophysics, 2007-04, Vol.50 (2), p.187-193

2007

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Large Flares (M1–X7) in Solar Activity Cycle 24

Geomagnetism and aeronomy, 2017-12, Vol.57 (8), p.1077-1085

2017

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The cyclic activity of the sun from observations of the activity indices at different time scales

Moscow University physics bulletin, 2015-07, Vol.70 (4), p.282-290

2015

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Methods for Monitoring Strong Space Weather Disturbances to Support International Air Navigation

Meteorologiâ i gidrologiâ, 2021, Vol.3, p.102-110

2021

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The possibility of simulation of the chromospheric variations for main-sequence stars

Astronomical and astrophysical transactions, 2004-04, Vol.23 (2), p.165-172

2004

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On chromospheric variations modeling for main-sequence stars of G and K spectral classes

Natural science (Irvine, Calif.), 2011, Vol.3 (8), p.641-645

Bruevich, E. A

2011

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The activity of the solar atmosphere and solar-type stars at 11-year and quasi-biennial timescales

Moscow University physics bulletin, 2011-02, Vol.66 (1), p.72-77

2011

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Interrelationships between Halo-Type Coronal Mass Ejections and Solar Flares Based on Observations in the 23rd and 24th Cycles

New classification parameter of solar flares based on the maximum flux in soft X-rays and on duration of flare

Lyman Decrements of Neutral Hydrogen Lines in the Spectrum of the Sun Based on SDO/EVE Observations. Variations During the 24-th Solar Cycle and in Individual Flares of Classes M and X

Powerful Solar Flares in September 2017. Comparison with the Largest Flares in Cycle 24

Changed Relation between Solar 10.7-cm Radio Flux and some Activity Indices which describe the Radiation at Different Altitudes of Atmosphere during Cycles 21–23

Flare Activity of the Sun and Variations in its UV Emission During Cycle 24

Flux Variations in Lines of Solar EUV Radiation beyond Flares in Cycle 24

Cyclic Variations in the Solar Radiation Fluxes at the Beginning of the 21st Century

Variations of Solar EUV Radiation Fluxes in Hydrogen Lines from Observations by the TIMED Satellite in Cycle 23 and by SDO/EVE in Cycle 24

Hysteresis Effect in the Activity Indices of the Atmospheres of the Sun and Solar-Type Stars During the Rising and Falling Phases of Cycles

Comparative Analysis of the Activity Cycles of the Atmospheres of the Sun and of Stars of the Solar-Type

Methods for Monitoring Strong Space Weather Disturbances to Support International Air Navigation

General trends in the change in solar activity indices in the period from the late XX to early XXI century

Hysteresis of indices of solar and ionospheric activity during 11-year cycles

Solar Flares in Extreme Ultraviolet and X-Ray Bands Based on SDO and TIMED Satellite Data

24th Cycle of Solar Activity: Geoefficiency of Flares

Solar-Flux Variation in Helium Lines According to SDO/EVE Data in the 24th Cycle and the Forecast for Different Levels of Solar Activity. Lyman Decrements of Hydrogen and Helium Lines

Levels of coronal and chromospheric activity in late-type stars and various types of dynamo waves

Spotting in stars with a low level of activity, close to solar activity

Large Flares (M1–X7) in Solar Activity Cycle 24

The cyclic activity of the sun from observations of the activity indices at different time scales

Methods for Monitoring Strong Space Weather Disturbances to Support International Air Navigation

The possibility of simulation of the chromospheric variations for main-sequence stars

On chromospheric variations modeling for main-sequence stars of G and K spectral classes

The activity of the solar atmosphere and solar-type stars at 11-year and quasi-biennial timescales

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