Standard

September 2017 Solar Flares Effect on the Middle Atmosphere. / Pikulina, Polina; Mironova, Irina; Rozanov, Eugene; Karagodin, Arseniy.

в: Remote Sensing, Том 14, № 11, 2560, 27.05.2022.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Pikulina, P, Mironova, I, Rozanov, E & Karagodin, A 2022, 'September 2017 Solar Flares Effect on the Middle Atmosphere', Remote Sensing, Том. 14, № 11, 2560. https://doi.org/10.3390/rs14112560

APA

Pikulina, P., Mironova, I., Rozanov, E., & Karagodin, A. (2022). September 2017 Solar Flares Effect on the Middle Atmosphere. Remote Sensing, 14(11), [2560]. https://doi.org/10.3390/rs14112560

Vancouver

Pikulina P, Mironova I, Rozanov E, Karagodin A. September 2017 Solar Flares Effect on the Middle Atmosphere. Remote Sensing. 2022 Май 27;14(11). 2560. https://doi.org/10.3390/rs14112560

Author

Pikulina, Polina ; Mironova, Irina ; Rozanov, Eugene ; Karagodin, Arseniy. / September 2017 Solar Flares Effect on the Middle Atmosphere. в: Remote Sensing. 2022 ; Том 14, № 11.

BibTeX

@article{ed793bbfa7ef4f69883e80b3921bf286,
title = "September 2017 Solar Flares Effect on the Middle Atmosphere",
abstract = "This paper examines the response of the upper atmosphere to increased radiation following exceptional solar activity in September 2017. The active region of the Sun AR2673 has caused intense solar-terrestrial disturbance. This active region has generated several powerful X-class solar flares. The strongest outburst of the 24th solar activity cycle X9.3 occurred on 6 September 2017. The second powerful solar flare X8.2 occurred on 10 September 2017. Both flares caused an increase of the solar irradiance in extreme ultraviolet and soft X-ray spectral regions, and Ly-α line. The empirical FISM2 model was used to obtain data on the radiation fluxes from solar flares. The HAMMONIA chemistry–climate model was used to analyze the effect of radiation on the neutral atmosphere. This work presents the results of the effect of solar flares on the chemical composition and ozone of the upper and middle atmosphere.",
keywords = "atmospheric response, ozone, solar flares",
author = "Polina Pikulina and Irina Mironova and Eugene Rozanov and Arseniy Karagodin",
note = "Publisher Copyright: {\textcopyright} 2022 by the authors. Licensee MDPI, Basel, Switzerland.",
year = "2022",
month = may,
day = "27",
doi = "10.3390/rs14112560",
language = "English",
volume = "14",
journal = "Remote Sensing",
issn = "2072-4292",
publisher = "MDPI AG",
number = "11",

}

RIS

TY - JOUR

T1 - September 2017 Solar Flares Effect on the Middle Atmosphere

AU - Pikulina, Polina

AU - Mironova, Irina

AU - Rozanov, Eugene

AU - Karagodin, Arseniy

N1 - Publisher Copyright: © 2022 by the authors. Licensee MDPI, Basel, Switzerland.

PY - 2022/5/27

Y1 - 2022/5/27

N2 - This paper examines the response of the upper atmosphere to increased radiation following exceptional solar activity in September 2017. The active region of the Sun AR2673 has caused intense solar-terrestrial disturbance. This active region has generated several powerful X-class solar flares. The strongest outburst of the 24th solar activity cycle X9.3 occurred on 6 September 2017. The second powerful solar flare X8.2 occurred on 10 September 2017. Both flares caused an increase of the solar irradiance in extreme ultraviolet and soft X-ray spectral regions, and Ly-α line. The empirical FISM2 model was used to obtain data on the radiation fluxes from solar flares. The HAMMONIA chemistry–climate model was used to analyze the effect of radiation on the neutral atmosphere. This work presents the results of the effect of solar flares on the chemical composition and ozone of the upper and middle atmosphere.

AB - This paper examines the response of the upper atmosphere to increased radiation following exceptional solar activity in September 2017. The active region of the Sun AR2673 has caused intense solar-terrestrial disturbance. This active region has generated several powerful X-class solar flares. The strongest outburst of the 24th solar activity cycle X9.3 occurred on 6 September 2017. The second powerful solar flare X8.2 occurred on 10 September 2017. Both flares caused an increase of the solar irradiance in extreme ultraviolet and soft X-ray spectral regions, and Ly-α line. The empirical FISM2 model was used to obtain data on the radiation fluxes from solar flares. The HAMMONIA chemistry–climate model was used to analyze the effect of radiation on the neutral atmosphere. This work presents the results of the effect of solar flares on the chemical composition and ozone of the upper and middle atmosphere.

KW - atmospheric response

KW - ozone

KW - solar flares

UR - http://www.scopus.com/inward/record.url?scp=85131451625&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/4894b962-6a6b-313f-90cf-093a4d0c8c41/

U2 - 10.3390/rs14112560

DO - 10.3390/rs14112560

M3 - Article

AN - SCOPUS:85131451625

VL - 14

JO - Remote Sensing

JF - Remote Sensing

SN - 2072-4292

IS - 11

M1 - 2560

ER -

ID: 96949082