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Energetic Particle Influence on the Earth’s Atmosphere

Space Science Reviews, 2015-11, Vol.194 (1-4), p.1-96

2015

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Solar signals in CMIP‐5 simulations: the stratospheric pathway

Quarterly journal of the Royal Meteorological Society, 2015-07, Vol.141 (691), p.2390-2403

2015

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Solar signals in CMIP‐5 simulations: effects of atmosphere–ocean coupling

Quarterly journal of the Royal Meteorological Society, 2016-01, Vol.142 (695), p.928-941

2016

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Russian Middle Atmosphere Research 2019–2022

Izvestiya. Atmospheric and oceanic physics, 2023-12, Vol.59 (Suppl 3), p.S340-S362

2023

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Solar signals in CMIP‐5 simulations: the ozone response

Quarterly journal of the Royal Meteorological Society, 2015-10, Vol.141 (692), p.2670-2689

2015

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Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study

Atmospheric chemistry and physics, 2011-09, Vol.11 (17), p.9089-9139

2011

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The solar cycle variation in ultraviolet irradiance

Advances in Space Research, 2001-01, Vol.27 (12), p.1927-1932

2001

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Solar cycle influence on troposphere and middle atmosphere via ozone layer in the presence of planetary waves: Simulation with ARM

Journal of geophysical research. Space physics, 2015-10, Vol.120 (10), p.8298-8306

2015

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Changes in surface UV solar irradiance and ozone over the balkans during the eclipse of August 11, 1999

Advances in Space Research, 2001-01, Vol.27 (12), p.1955-1963

2001

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Calculation of the Ionization Rate in the Atmosphere in the Polar Region during Solar Proton Events

Geomagnetism and Aeronomy, 2020-09, Vol.60 (5), p.570-576

2020

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Experimental Global Forecasts of Atmospheric Parameters Based on Experimental Technology that Takes into Account Ozone Photochemistry (FOROZ Model)

Geomagnetism and Aeronomy, 2020-03, Vol.60 (2), p.243-253

2020

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Monitoring of solar proton events at altitudes up to 1000 km: Data from the Russian space experiments. Solar proton effects in the Earth’s ozonosphere

Geomagnetism and Aeronomy, 2017-11, Vol.57 (6), p.672-683

2017

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Impact of space energetic particles on the Earth’s atmosphere (a review)

Geomagnetism and Aeronomy, 2012-11, Vol.52 (6), p.685-716

2012

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Results of Russian Studies of the Middle Atmosphere in 2015–2018

Izvestiya. Atmospheric and oceanic physics, 2019-11, Vol.55 (6), p.537-551

2019

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Results of Russian investigations into the middle atmosphere (2011–2014)

Izvestiya. Atmospheric and oceanic physics, 2016-09, Vol.52 (5), p.497-511

2016

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Nonzonal structure of the response of the global field of the Earth’s atmospheric temperature to solar activity

Geomagnetism and Aeronomy, 2017, Vol.57 (1), p.107-112

2017

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Model simulations of the impact of the 27-day solar rotation period on stratospheric ozone and temperature

Advances in Space Research, 2001-01, Vol.27 (12), p.1933-1942

2001

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Cosmic ray influence on chemical composition of the atmosphere of the earth

Advances in Space Research, 2001-01, Vol.27 (12), p.1993-2002

2001

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Changes in the chemical composition of the atmosphere in the polar regions of the Earth after solar proton flares (3d modeling)

Geomagnetism and Aeronomy, 2017-03, Vol.57 (2), p.156-176

2017

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Photochemical response of neutral and ionized middle atmosphere composition to the strong solar proton event of October 1989

Advances in Space Research, 2001-01, Vol.27 (12), p.1975-1981

2001

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Long term solar induced variations in total ozone, stratospheric temperatures and the tropopause

Advances in Space Research, 2001-01, Vol.27 (12), p.1943-1948

2001

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The three-dimensional global numerical model CHARM-I: The incorporation of processes in the ionospheric D-region

Geomagnetism and Aeronomy, 2015-07, Vol.55 (4), p.467-486

2015

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Global circulation of the Earth’s atmosphere at altitudes from 0 to 135 Km simulated with the ARM model. Consideration of the solar activity contribution

Geomagnetism and Aeronomy, 2015-11, Vol.55 (6), p.780-800

2015

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Effect of Forbush decreases of cosmic ray flux on ozone at higher middle latitudes

Advances in Space Research, 2001-01, Vol.27 (12), p.2003-2006

2001

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Variations in solar radiation in the solar activity cycle: Response of Earth’s atmospheric parameters (numerical modeling and analysis of observational data)

Geomagnetism and Aeronomy, 2016-12, Vol.56 (7), p.920-929

2016

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Energetic Particle Influence on the Earth’s Atmosphere

Solar signals in CMIP‐5 simulations: the stratospheric pathway

Solar signals in CMIP‐5 simulations: effects of atmosphere–ocean coupling

Russian Middle Atmosphere Research 2019–2022

Solar signals in CMIP‐5 simulations: the ozone response

Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study

The solar cycle variation in ultraviolet irradiance

Solar cycle influence on troposphere and middle atmosphere via ozone layer in the presence of planetary waves: Simulation with ARM

Changes in surface UV solar irradiance and ozone over the balkans during the eclipse of August 11, 1999

Calculation of the Ionization Rate in the Atmosphere in the Polar Region during Solar Proton Events

Experimental Global Forecasts of Atmospheric Parameters Based on Experimental Technology that Takes into Account Ozone Photochemistry (FOROZ Model)

Monitoring of solar proton events at altitudes up to 1000 km: Data from the Russian space experiments. Solar proton effects in the Earth’s ozonosphere

Impact of space energetic particles on the Earth’s atmosphere (a review)

Results of Russian Studies of the Middle Atmosphere in 2015–2018

Results of Russian investigations into the middle atmosphere (2011–2014)

Nonzonal structure of the response of the global field of the Earth’s atmospheric temperature to solar activity

Model simulations of the impact of the 27-day solar rotation period on stratospheric ozone and temperature

Cosmic ray influence on chemical composition of the atmosphere of the earth

Changes in the chemical composition of the atmosphere in the polar regions of the Earth after solar proton flares (3d modeling)

Photochemical response of neutral and ionized middle atmosphere composition to the strong solar proton event of October 1989

Long term solar induced variations in total ozone, stratospheric temperatures and the tropopause

The three-dimensional global numerical model CHARM-I: The incorporation of processes in the ionospheric D-region

Global circulation of the Earth’s atmosphere at altitudes from 0 to 135 Km simulated with the ARM model. Consideration of the solar activity contribution

Effect of Forbush decreases of cosmic ray flux on ozone at higher middle latitudes

Variations in solar radiation in the solar activity cycle: Response of Earth’s atmospheric parameters (numerical modeling and analysis of observational data)

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