Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters: Modeling and Observations for Case Studies

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Standard

Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters : Modeling and Observations for Case Studies. / Klimenko, M. V.; Ratovsky, K. G.; Themens, D.; Yasukevich, A. S.; Klimenko, V. V.

2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 - Proceedings. Institute of Electrical and Electronics Engineers (IEEE), 2019. p. 3469-3473 9017784 (Progress in Electromagnetics Research Symposium; Vol. 2019-June).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Harvard

Klimenko, MV, Ratovsky, KG, Themens, D, Yasukevich, AS & Klimenko, VV 2019, Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters: Modeling and Observations for Case Studies. in 2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 - Proceedings., 9017784, Progress in Electromagnetics Research Symposium, vol. 2019-June, Institute of Electrical and Electronics Engineers (IEEE), pp. 3469-3473, 2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019, Rome, Italy, 17/06/19. https://doi.org/10.1109/PIERS-Spring46901.2019.9017784

APA

Klimenko, M. V., Ratovsky, K. G., Themens, D., Yasukevich, A. S., & Klimenko, V. V. (2019). Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters: Modeling and Observations for Case Studies. In 2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 - Proceedings (pp. 3469-3473). [9017784] (Progress in Electromagnetics Research Symposium; Vol. 2019-June). Institute of Electrical and Electronics Engineers (IEEE). https://doi.org/10.1109/PIERS-Spring46901.2019.9017784

Vancouver

Klimenko MV, Ratovsky KG, Themens D, Yasukevich AS, Klimenko VV. Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters: Modeling and Observations for Case Studies. In 2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 - Proceedings. Institute of Electrical and Electronics Engineers (IEEE). 2019. p. 3469-3473. 9017784. (Progress in Electromagnetics Research Symposium). https://doi.org/10.1109/PIERS-Spring46901.2019.9017784

Author

Klimenko, M. V. ; Ratovsky, K. G. ; Themens, D. ; Yasukevich, A. S. ; Klimenko, V. V. / Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters : Modeling and Observations for Case Studies. 2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 - Proceedings. Institute of Electrical and Electronics Engineers (IEEE), 2019. pp. 3469-3473 (Progress in Electromagnetics Research Symposium).

Bibtex

@inproceedings{ea3683ba606d406eaf4152ef8eda6caf,
title = "Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters: Modeling and Observations for Case Studies",
abstract = "We investigated the effect of 27 day solar rotation on the thermosphere-ionosphere system at different latitudes using both model results and multi-instrumental observation data. Considered ionospheric stations (ionosondes, GPS receivers, ISR radars) were located from the middle to high latitudes in Northern hemisphere. We analyzed also TIMED/GUVI variations of the O/N2 ratio in the thermosphere. Three different temporal periods were considered: December 2012-January 2013; January 2014; June - July 2014. The Global Self-consistent Model of the Thermosphere, Ionosphere, and Protonosphere (GSM TIP) were used for interpretation of coupled processes in the thermosphere-ionosphere system during one solar rotation cycle. There is a distinct response of daytime ionospheric electron density to the 27-day variation in solar flux (F10.7). Using comparative and correlative analysis we revealed a delay in variation of modeled daytime critical frequency (foF2) and total electron content (TEC) with respect to F10.7 variation. According to model results variations in O/N2 ratio seems to be the main possible mechanism for this delay. Some model/data disagreement was discussed in context of importance of atmosphere-ionosphere coupling and geomagnetic control of ionospheric variability. Seasonal changes and difference between 27-day variation in foF2 and TEC were discussed.",
author = "Klimenko, {M. V.} and Ratovsky, {K. G.} and D. Themens and Yasukevich, {A. S.} and Klimenko, {V. V.}",
year = "2019",
month = jun,
doi = "10.1109/PIERS-Spring46901.2019.9017784",
language = "English",
series = "Progress in Electromagnetics Research Symposium",
publisher = "Institute of Electrical and Electronics Engineers (IEEE)",
pages = "3469--3473",
booktitle = "2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 - Proceedings",
note = "2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 ; Conference date: 17-06-2019 Through 20-06-2019",

}

RIS

TY - GEN

T1 - Influence of Solar Rotation Influence on Ionospheric/Thermospheric Parameters

T2 - 2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019

AU - Klimenko, M. V.

AU - Ratovsky, K. G.

AU - Themens, D.

AU - Yasukevich, A. S.

AU - Klimenko, V. V.

PY - 2019/6

Y1 - 2019/6

N2 - We investigated the effect of 27 day solar rotation on the thermosphere-ionosphere system at different latitudes using both model results and multi-instrumental observation data. Considered ionospheric stations (ionosondes, GPS receivers, ISR radars) were located from the middle to high latitudes in Northern hemisphere. We analyzed also TIMED/GUVI variations of the O/N2 ratio in the thermosphere. Three different temporal periods were considered: December 2012-January 2013; January 2014; June - July 2014. The Global Self-consistent Model of the Thermosphere, Ionosphere, and Protonosphere (GSM TIP) were used for interpretation of coupled processes in the thermosphere-ionosphere system during one solar rotation cycle. There is a distinct response of daytime ionospheric electron density to the 27-day variation in solar flux (F10.7). Using comparative and correlative analysis we revealed a delay in variation of modeled daytime critical frequency (foF2) and total electron content (TEC) with respect to F10.7 variation. According to model results variations in O/N2 ratio seems to be the main possible mechanism for this delay. Some model/data disagreement was discussed in context of importance of atmosphere-ionosphere coupling and geomagnetic control of ionospheric variability. Seasonal changes and difference between 27-day variation in foF2 and TEC were discussed.

AB - We investigated the effect of 27 day solar rotation on the thermosphere-ionosphere system at different latitudes using both model results and multi-instrumental observation data. Considered ionospheric stations (ionosondes, GPS receivers, ISR radars) were located from the middle to high latitudes in Northern hemisphere. We analyzed also TIMED/GUVI variations of the O/N2 ratio in the thermosphere. Three different temporal periods were considered: December 2012-January 2013; January 2014; June - July 2014. The Global Self-consistent Model of the Thermosphere, Ionosphere, and Protonosphere (GSM TIP) were used for interpretation of coupled processes in the thermosphere-ionosphere system during one solar rotation cycle. There is a distinct response of daytime ionospheric electron density to the 27-day variation in solar flux (F10.7). Using comparative and correlative analysis we revealed a delay in variation of modeled daytime critical frequency (foF2) and total electron content (TEC) with respect to F10.7 variation. According to model results variations in O/N2 ratio seems to be the main possible mechanism for this delay. Some model/data disagreement was discussed in context of importance of atmosphere-ionosphere coupling and geomagnetic control of ionospheric variability. Seasonal changes and difference between 27-day variation in foF2 and TEC were discussed.

UR - http://www.scopus.com/inward/record.url?scp=85082025561&partnerID=8YFLogxK

U2 - 10.1109/PIERS-Spring46901.2019.9017784

DO - 10.1109/PIERS-Spring46901.2019.9017784

M3 - Conference contribution

AN - SCOPUS:85082025561

T3 - Progress in Electromagnetics Research Symposium

SP - 3469

EP - 3473

BT - 2019 PhotonIcs and Electromagnetics Research Symposium - Spring, PIERS-Spring 2019 - Proceedings

PB - Institute of Electrical and Electronics Engineers (IEEE)

Y2 - 17 June 2019 through 20 June 2019

ER -