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Modeling the UT effect in global distribution of ionospheric electric fields. / Lukianova, R.; Christiansen, F.

в: Journal of Atmospheric and Solar-Terrestrial Physics, Том 70, № 2-4, 01.02.2008, стр. 637-645.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Lukianova, R & Christiansen, F 2008, 'Modeling the UT effect in global distribution of ionospheric electric fields', Journal of Atmospheric and Solar-Terrestrial Physics, Том. 70, № 2-4, стр. 637-645. https://doi.org/10.1016/j.jastp.2007.08.047

APA

Lukianova, R., & Christiansen, F. (2008). Modeling the UT effect in global distribution of ionospheric electric fields. Journal of Atmospheric and Solar-Terrestrial Physics, 70(2-4), 637-645. https://doi.org/10.1016/j.jastp.2007.08.047

Vancouver

Lukianova R, Christiansen F. Modeling the UT effect in global distribution of ionospheric electric fields. Journal of Atmospheric and Solar-Terrestrial Physics. 2008 Февр. 1;70(2-4):637-645. https://doi.org/10.1016/j.jastp.2007.08.047

Author

Lukianova, R. ; Christiansen, F. / Modeling the UT effect in global distribution of ionospheric electric fields. в: Journal of Atmospheric and Solar-Terrestrial Physics. 2008 ; Том 70, № 2-4. стр. 637-645.

BibTeX

@article{2a87f1db92af450b83c8abdda6e942a7,
title = "Modeling the UT effect in global distribution of ionospheric electric fields",
abstract = "A new approach for modeling the global distribution of ionospheric electric potentials utilizing high-precision maps of field-aligned currents (FACs) derived from measurements by the {\O}rsted and Magsat satellites as input to a comprehensive numerical scheme is presented. We simulate the universal time (UT) effect in convection patterns caused by variation of solar luminosity and its effect on ionospheric conductivity. A rather complicated dependence of the convection patterns on the combination of UT and IMF clock angle is found. We consider different seasons and IMF conditions and find an increase of the daily variation in the cross-polar potential drop (UPC) at the equinoxes and a decrease at the solstices. Under equinoctial and zero IMF conditions the UPC can vary by a factor of two, while the convection cells keep their shape. The model predicts that the summer UPC can be smaller or larger than the winter UPC depending on the combination of UT and IMF clock angle. If a UT control of the FAC is introduced to the model, the UPC does not vary more than 10% over the course of the day.",
keywords = "Conductance, Convection, Field-aligned currents, Ionospheric electric field",
author = "R. Lukianova and F. Christiansen",
year = "2008",
month = feb,
day = "1",
doi = "10.1016/j.jastp.2007.08.047",
language = "English",
volume = "70",
pages = "637--645",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
issn = "1364-6826",
publisher = "Elsevier",
number = "2-4",

}

RIS

TY - JOUR

T1 - Modeling the UT effect in global distribution of ionospheric electric fields

AU - Lukianova, R.

AU - Christiansen, F.

PY - 2008/2/1

Y1 - 2008/2/1

N2 - A new approach for modeling the global distribution of ionospheric electric potentials utilizing high-precision maps of field-aligned currents (FACs) derived from measurements by the Ørsted and Magsat satellites as input to a comprehensive numerical scheme is presented. We simulate the universal time (UT) effect in convection patterns caused by variation of solar luminosity and its effect on ionospheric conductivity. A rather complicated dependence of the convection patterns on the combination of UT and IMF clock angle is found. We consider different seasons and IMF conditions and find an increase of the daily variation in the cross-polar potential drop (UPC) at the equinoxes and a decrease at the solstices. Under equinoctial and zero IMF conditions the UPC can vary by a factor of two, while the convection cells keep their shape. The model predicts that the summer UPC can be smaller or larger than the winter UPC depending on the combination of UT and IMF clock angle. If a UT control of the FAC is introduced to the model, the UPC does not vary more than 10% over the course of the day.

AB - A new approach for modeling the global distribution of ionospheric electric potentials utilizing high-precision maps of field-aligned currents (FACs) derived from measurements by the Ørsted and Magsat satellites as input to a comprehensive numerical scheme is presented. We simulate the universal time (UT) effect in convection patterns caused by variation of solar luminosity and its effect on ionospheric conductivity. A rather complicated dependence of the convection patterns on the combination of UT and IMF clock angle is found. We consider different seasons and IMF conditions and find an increase of the daily variation in the cross-polar potential drop (UPC) at the equinoxes and a decrease at the solstices. Under equinoctial and zero IMF conditions the UPC can vary by a factor of two, while the convection cells keep their shape. The model predicts that the summer UPC can be smaller or larger than the winter UPC depending on the combination of UT and IMF clock angle. If a UT control of the FAC is introduced to the model, the UPC does not vary more than 10% over the course of the day.

KW - Conductance

KW - Convection

KW - Field-aligned currents

KW - Ionospheric electric field

UR - http://www.scopus.com/inward/record.url?scp=38949136980&partnerID=8YFLogxK

U2 - 10.1016/j.jastp.2007.08.047

DO - 10.1016/j.jastp.2007.08.047

M3 - Article

AN - SCOPUS:38949136980

VL - 70

SP - 637

EP - 645

JO - Journal of Atmospheric and Solar-Terrestrial Physics

JF - Journal of Atmospheric and Solar-Terrestrial Physics

SN - 1364-6826

IS - 2-4

ER -

ID: 36801587