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Changes in the Chemical Composition of the Polar Atmosphere According to Satellite Observations in January 2005. / Doronin, Grigoriy; Mironova, Irina; Mironov, Andrey; Bobrov, Nikita.

In: Bulletin of the Russian Academy of Sciences: Physics, Vol. 89, No. 6, 01.06.2025, p. 963-968.

Research output: Contribution to journal › Article › peer-review

Harvard

Doronin, G, Mironova, I, Mironov, A & Bobrov, N 2025, 'Changes in the Chemical Composition of the Polar Atmosphere According to Satellite Observations in January 2005', Bulletin of the Russian Academy of Sciences: Physics, vol. 89, no. 6, pp. 963-968. https://doi.org/10.1134/S106287382571147X

APA

Doronin, G., Mironova, I., Mironov, A., & Bobrov, N. (2025). Changes in the Chemical Composition of the Polar Atmosphere According to Satellite Observations in January 2005. Bulletin of the Russian Academy of Sciences: Physics, 89(6), 963-968. https://doi.org/10.1134/S106287382571147X

Vancouver

Doronin G, Mironova I, Mironov A, Bobrov N. Changes in the Chemical Composition of the Polar Atmosphere According to Satellite Observations in January 2005. Bulletin of the Russian Academy of Sciences: Physics. 2025 Jun 1;89(6):963-968. https://doi.org/10.1134/S106287382571147X

Author

Doronin, Grigoriy ; Mironova, Irina ; Mironov, Andrey ; Bobrov, Nikita. / Changes in the Chemical Composition of the Polar Atmosphere According to Satellite Observations in January 2005. In: Bulletin of the Russian Academy of Sciences: Physics. 2025 ; Vol. 89, No. 6. pp. 963-968.

BibTeX

@article{dc5e327d6f284e5dbe0b2f5046c887d6,
title = "Changes in the Chemical Composition of the Polar Atmosphere According to Satellite Observations in January 2005",
abstract = "On January 16–22, 2005 huge fluxes of high-energy charged particles came from the Sun through magnetosphere to our Earth. Charged particles mostly solar protons and magnetospheric electrons affect the atmosphere by inducing additional ionization sources in ionosphere and atmosphere. Ionization plays main role in the formation of ozone-depleting odd oxides of nitrogen (NOx) and hydrogen (HOx). Here we study the energetic particle impact on the chemical properties of the stratosphere and mesosphere in the Northern Hemisphere using MLS Aura data obtained during January 16–22, 2005. We show how strong can be depleted the polar ozone layer in mesosphere and change the chemistry from the mesosphere to the stratosphere during geoeffective coronal mass ejections and magnetic storms.",
keywords = "and MLS observations, chemical compositions, energetic particle precipitation, mesosphere, ozone",
author = "Grigoriy Doronin and Irina Mironova and Andrey Mironov and Nikita Bobrov",
year = "2025",
month = jun,
day = "1",
doi = "10.1134/S106287382571147X",
language = "English",
volume = "89",
pages = "963--968",
journal = "Bulletin of the Russian Academy of Sciences: Physics",
issn = "1062-8738",
publisher = "Allerton Press, Inc.",
number = "6",

}

RIS

TY - JOUR

T1 - Changes in the Chemical Composition of the Polar Atmosphere According to Satellite Observations in January 2005

AU - Doronin, Grigoriy

AU - Mironova, Irina

AU - Mironov, Andrey

AU - Bobrov, Nikita

PY - 2025/6/1

Y1 - 2025/6/1

N2 - On January 16–22, 2005 huge fluxes of high-energy charged particles came from the Sun through magnetosphere to our Earth. Charged particles mostly solar protons and magnetospheric electrons affect the atmosphere by inducing additional ionization sources in ionosphere and atmosphere. Ionization plays main role in the formation of ozone-depleting odd oxides of nitrogen (NOx) and hydrogen (HOx). Here we study the energetic particle impact on the chemical properties of the stratosphere and mesosphere in the Northern Hemisphere using MLS Aura data obtained during January 16–22, 2005. We show how strong can be depleted the polar ozone layer in mesosphere and change the chemistry from the mesosphere to the stratosphere during geoeffective coronal mass ejections and magnetic storms.

AB - On January 16–22, 2005 huge fluxes of high-energy charged particles came from the Sun through magnetosphere to our Earth. Charged particles mostly solar protons and magnetospheric electrons affect the atmosphere by inducing additional ionization sources in ionosphere and atmosphere. Ionization plays main role in the formation of ozone-depleting odd oxides of nitrogen (NOx) and hydrogen (HOx). Here we study the energetic particle impact on the chemical properties of the stratosphere and mesosphere in the Northern Hemisphere using MLS Aura data obtained during January 16–22, 2005. We show how strong can be depleted the polar ozone layer in mesosphere and change the chemistry from the mesosphere to the stratosphere during geoeffective coronal mass ejections and magnetic storms.

KW - and MLS observations

KW - chemical compositions

KW - energetic particle precipitation

KW - mesosphere

KW - ozone

UR - https://www.mendeley.com/catalogue/32d2ed0d-8cc4-3fa0-a9be-38eddc1657ad/

U2 - 10.1134/S106287382571147X

DO - 10.1134/S106287382571147X

M3 - Article

VL - 89

SP - 963

EP - 968

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

SN - 1062-8738

IS - 6

ER -

ID: 135959430