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Modeling intermittent fluctuations of transionospheric signals. / Makarenkova, E. V.; Gherm, V. E.

в: Journal of Atmospheric and Solar-Terrestrial Physics, Том 221, 105703, 01.09.2021.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

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Makarenkova EV, Gherm VE. Modeling intermittent fluctuations of transionospheric signals. Journal of Atmospheric and Solar-Terrestrial Physics. 2021 Сент. 1;221. 105703. https://doi.org/10.1016/j.jastp.2021.105703

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Makarenkova, E. V. ; Gherm, V. E. / Modeling intermittent fluctuations of transionospheric signals. в: Journal of Atmospheric and Solar-Terrestrial Physics. 2021 ; Том 221.

BibTeX

@article{022291114192413c9acd2653dc83f90c,
title = "Modeling intermittent fluctuations of transionospheric signals",
abstract = "The paper proposes a methodology and presents the results of modeling fluctuations of transionospheric radio signals propagating under conditions of intermittent ionospheric turbulence. To account for the intermittency of turbulence, the earlier developed model of a non-Gaussian multifractal phase screen is further extended to the case of the log-Poisson cascade model and additionally validated. Employing this technique, the intermittent fluctuations of the field on the ground are studied. An effect of the non-Gaussianity of phase fluctuations on the statistical characteristics of the field on Earth is demonstrated. In particular, an increase in the field coherence radius and a decrease in the scintillation index were found with an increase in the degree of intermittency of phase fluctuations on the screen, other parameters being equal. The results for the lognormal and log-Poisson models are slightly different in detail, but generally appear quite similar. The fluctuations of phase on the ground and screen possess the same multifractal scaling for the scales larger than the Fresnel zone size. This allows for solving the inverse problem of estimating the parameters of the model of the ionospheric turbulence employing the ground measurements data. The small-scale fluctuations (less than the Fresnel scale) of the field on the ground do not inherit the multifractal scaling of the field emerging from the screen due to the diffraction in free space.",
keywords = "Fluctuations, Ionosphere, Multifractal, Non-Gaussianity, Turbulence, FLUID, LOW-LATITUDE, SCINTILLATIONS",
author = "Makarenkova, {E. V.} and Gherm, {V. E.}",
note = "Publisher Copyright: {\textcopyright} 2021 Elsevier Ltd Copyright: Copyright 2021 Elsevier B.V., All rights reserved.",
year = "2021",
month = sep,
day = "1",
doi = "10.1016/j.jastp.2021.105703",
language = "English",
volume = "221",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
issn = "1364-6826",
publisher = "Elsevier",

}

RIS

TY - JOUR

T1 - Modeling intermittent fluctuations of transionospheric signals

AU - Makarenkova, E. V.

AU - Gherm, V. E.

N1 - Publisher Copyright: © 2021 Elsevier Ltd Copyright: Copyright 2021 Elsevier B.V., All rights reserved.

PY - 2021/9/1

Y1 - 2021/9/1

N2 - The paper proposes a methodology and presents the results of modeling fluctuations of transionospheric radio signals propagating under conditions of intermittent ionospheric turbulence. To account for the intermittency of turbulence, the earlier developed model of a non-Gaussian multifractal phase screen is further extended to the case of the log-Poisson cascade model and additionally validated. Employing this technique, the intermittent fluctuations of the field on the ground are studied. An effect of the non-Gaussianity of phase fluctuations on the statistical characteristics of the field on Earth is demonstrated. In particular, an increase in the field coherence radius and a decrease in the scintillation index were found with an increase in the degree of intermittency of phase fluctuations on the screen, other parameters being equal. The results for the lognormal and log-Poisson models are slightly different in detail, but generally appear quite similar. The fluctuations of phase on the ground and screen possess the same multifractal scaling for the scales larger than the Fresnel zone size. This allows for solving the inverse problem of estimating the parameters of the model of the ionospheric turbulence employing the ground measurements data. The small-scale fluctuations (less than the Fresnel scale) of the field on the ground do not inherit the multifractal scaling of the field emerging from the screen due to the diffraction in free space.

AB - The paper proposes a methodology and presents the results of modeling fluctuations of transionospheric radio signals propagating under conditions of intermittent ionospheric turbulence. To account for the intermittency of turbulence, the earlier developed model of a non-Gaussian multifractal phase screen is further extended to the case of the log-Poisson cascade model and additionally validated. Employing this technique, the intermittent fluctuations of the field on the ground are studied. An effect of the non-Gaussianity of phase fluctuations on the statistical characteristics of the field on Earth is demonstrated. In particular, an increase in the field coherence radius and a decrease in the scintillation index were found with an increase in the degree of intermittency of phase fluctuations on the screen, other parameters being equal. The results for the lognormal and log-Poisson models are slightly different in detail, but generally appear quite similar. The fluctuations of phase on the ground and screen possess the same multifractal scaling for the scales larger than the Fresnel zone size. This allows for solving the inverse problem of estimating the parameters of the model of the ionospheric turbulence employing the ground measurements data. The small-scale fluctuations (less than the Fresnel scale) of the field on the ground do not inherit the multifractal scaling of the field emerging from the screen due to the diffraction in free space.

KW - Fluctuations

KW - Ionosphere

KW - Multifractal

KW - Non-Gaussianity

KW - Turbulence

KW - FLUID

KW - LOW-LATITUDE

KW - SCINTILLATIONS

UR - http://www.scopus.com/inward/record.url?scp=85108538809&partnerID=8YFLogxK

U2 - 10.1016/j.jastp.2021.105703

DO - 10.1016/j.jastp.2021.105703

M3 - Article

AN - SCOPUS:85108538809

VL - 221

JO - Journal of Atmospheric and Solar-Terrestrial Physics

JF - Journal of Atmospheric and Solar-Terrestrial Physics

SN - 1364-6826

M1 - 105703

ER -

ID: 78301307