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Ionization in the earth’s atmosphere due to isotropic energetic electron precipitation : Ion production and primary electron spectra. / Mironova, Irina; Kovaltsov, Gennadiy; Mishev, Alexander; Artamonov, Anton.

в: Remote Sensing, Том 13, № 20, 4161, 18.10.2021.

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

Harvard

Mironova, I, Kovaltsov, G, Mishev, A & Artamonov, A 2021, 'Ionization in the earth’s atmosphere due to isotropic energetic electron precipitation: Ion production and primary electron spectra', Remote Sensing, Том. 13, № 20, 4161. https://doi.org/10.3390/rs13204161

APA

Mironova, I., Kovaltsov, G., Mishev, A., & Artamonov, A. (2021). Ionization in the earth’s atmosphere due to isotropic energetic electron precipitation: Ion production and primary electron spectra. Remote Sensing, 13(20), [4161]. https://doi.org/10.3390/rs13204161

Vancouver

Mironova I, Kovaltsov G, Mishev A, Artamonov A. Ionization in the earth’s atmosphere due to isotropic energetic electron precipitation: Ion production and primary electron spectra. Remote Sensing. 2021 Окт. 18;13(20). 4161. https://doi.org/10.3390/rs13204161

Author

Mironova, Irina ; Kovaltsov, Gennadiy ; Mishev, Alexander ; Artamonov, Anton. / Ionization in the earth’s atmosphere due to isotropic energetic electron precipitation : Ion production and primary electron spectra. в: Remote Sensing. 2021 ; Том 13, № 20.

BibTeX

@article{e31d5074d11f499f9c4965d8020e349d,
title = "Ionization in the earth{\textquoteright}s atmosphere due to isotropic energetic electron precipitation: Ion production and primary electron spectra",
abstract = "Energetic electron precipitation (EEP) via atmospheric ion production rates is a natural force acting on the atmosphere and climate systems. The correct estimation of EEP ion production and spectra for the computation of ionization rates is an important issue for estimating climate forces. In the present paper, we propose a favorable method for the computation of ionization rates forced by EEP using the new parameterization of ion production and a new spectrum shape, which allow one to take into account the range of precipitating particles from tens of keV to several MeV. A new function of spectral fit will also be helpful in obtaining information about EEP from satellite and balloon observations. Presented here, the parameterization of atmospheric ionization in the Earth{\textquoteright}s atmosphere includes a new yield function of isotropically precipitating monoenergetic electrons and ionization via Bremsstrahlung radiation. Look-up tables with ion production/yield function for isotropically precipitating monoenergetic electrons (30 keV–5 MeV) can be easily used for the computation of ionization rates and can further be used by atmospheric and chemistry-climate models for accurate quantification of atmospheric parameters during energetic electron precipitation.",
keywords = "Atmospheric ionization, EEP spectra, Electron ionization yield function, Energetic electron precipitation (EEP), MONTE-CARLO, energetic electron precipitation (EEP), EXCITATION, electron ionization yield function, DEPOSITION, MODEL, atmospheric ionization, AURORA",
author = "Irina Mironova and Gennadiy Kovaltsov and Alexander Mishev and Anton Artamonov",
note = "Publisher Copyright: {\textcopyright} 2021 by the authors. Licensee MDPI, Basel, Switzerland.",
year = "2021",
month = oct,
day = "18",
doi = "10.3390/rs13204161",
language = "English",
volume = "13",
journal = "Remote Sensing",
issn = "2072-4292",
publisher = "MDPI AG",
number = "20",

}

RIS

TY - JOUR

T1 - Ionization in the earth’s atmosphere due to isotropic energetic electron precipitation

T2 - Ion production and primary electron spectra

AU - Mironova, Irina

AU - Kovaltsov, Gennadiy

AU - Mishev, Alexander

AU - Artamonov, Anton

N1 - Publisher Copyright: © 2021 by the authors. Licensee MDPI, Basel, Switzerland.

PY - 2021/10/18

Y1 - 2021/10/18

N2 - Energetic electron precipitation (EEP) via atmospheric ion production rates is a natural force acting on the atmosphere and climate systems. The correct estimation of EEP ion production and spectra for the computation of ionization rates is an important issue for estimating climate forces. In the present paper, we propose a favorable method for the computation of ionization rates forced by EEP using the new parameterization of ion production and a new spectrum shape, which allow one to take into account the range of precipitating particles from tens of keV to several MeV. A new function of spectral fit will also be helpful in obtaining information about EEP from satellite and balloon observations. Presented here, the parameterization of atmospheric ionization in the Earth’s atmosphere includes a new yield function of isotropically precipitating monoenergetic electrons and ionization via Bremsstrahlung radiation. Look-up tables with ion production/yield function for isotropically precipitating monoenergetic electrons (30 keV–5 MeV) can be easily used for the computation of ionization rates and can further be used by atmospheric and chemistry-climate models for accurate quantification of atmospheric parameters during energetic electron precipitation.

AB - Energetic electron precipitation (EEP) via atmospheric ion production rates is a natural force acting on the atmosphere and climate systems. The correct estimation of EEP ion production and spectra for the computation of ionization rates is an important issue for estimating climate forces. In the present paper, we propose a favorable method for the computation of ionization rates forced by EEP using the new parameterization of ion production and a new spectrum shape, which allow one to take into account the range of precipitating particles from tens of keV to several MeV. A new function of spectral fit will also be helpful in obtaining information about EEP from satellite and balloon observations. Presented here, the parameterization of atmospheric ionization in the Earth’s atmosphere includes a new yield function of isotropically precipitating monoenergetic electrons and ionization via Bremsstrahlung radiation. Look-up tables with ion production/yield function for isotropically precipitating monoenergetic electrons (30 keV–5 MeV) can be easily used for the computation of ionization rates and can further be used by atmospheric and chemistry-climate models for accurate quantification of atmospheric parameters during energetic electron precipitation.

KW - Atmospheric ionization

KW - EEP spectra

KW - Electron ionization yield function

KW - Energetic electron precipitation (EEP)

KW - MONTE-CARLO

KW - energetic electron precipitation (EEP)

KW - EXCITATION

KW - electron ionization yield function

KW - DEPOSITION

KW - MODEL

KW - atmospheric ionization

KW - AURORA

UR - http://www.scopus.com/inward/record.url?scp=85117381793&partnerID=8YFLogxK

U2 - 10.3390/rs13204161

DO - 10.3390/rs13204161

M3 - Article

AN - SCOPUS:85117381793

VL - 13

JO - Remote Sensing

JF - Remote Sensing

SN - 2072-4292

IS - 20

M1 - 4161

ER -

ID: 87637927