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Persistent high-latitude ionospheric response to solar wind forcing

Borries, Claudia and Iochem, Pelin and Tasnim, Samira and Davis, Fredy (2024) Persistent high-latitude ionospheric response to solar wind forcing. Journal of Space Weather and Space Climate, 14 (33). EDP Sciences. doi: 10.1051/swsc/2024029. ISSN 2115-7251.

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Official URL: https://www.swsc-journal.org/articles/swsc/full_html/2024/01/swsc230082/swsc230082.html

Abstract

The solar wind continuously transfers energy into the Earth’s thermosphere-ionosphere system and variations in the solar wind properties modify the state of the system. The modifications are best visible during storm conditions when the ingestion of extreme amounts of solar wind energy into the thermosphere-ionosphere system causes global changes in thermosphere as well as large deviations in the ionospheric electron density from its quiet conditions. This study shows that there exists a persistent impact of the solar wind on the high-latitude electron density. A data set of 22 years of Total Electron Content (TEC) and 15 years of ionosonde data (critical frequency foF2 and height of maximum electron density hmF2) at Tromsø (70°N, 19°E) are used for correlation analyses with different solar wind parameters from OMNIWEB hourly “Near-Earth” solar wind magnetic field and plasma data. The results show that the ionospheric parameters systematically respond with an increase or decrease depending on local time, season, and solar cycle. TEC and foF2 increase with solar wind energy during winter night conditions and decrease with increasing solar wind energy during summer daytime. The summer negative ionospheric response is more intense during high solar activity conditions, while the winter positive ionospheric response is stronger during low solar activity. An anomaly is observed around 10 UT (noon) when TEC and foF2 respond with an increase during low solar activity conditions. Plasma convection, particle precipitation and Joule heating are the main drivers of the observed electron density changes at Tromsø. Local time, season, and solar cycle changes in the background ionosphere-thermosphere conditions lead to different effects of these driving processes. The results help to better understand the variability of the high-latitude electron density and show that solar wind forcing causes a systematic and persistent response of the ionosphere, which alternates depending on local time, season, and solar cycle.

Item URL in elib:https://elib.dlr.de/208516/
Document Type:Article
Title:Persistent high-latitude ionospheric response to solar wind forcing
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Borries, Claudiaclaudia.borries (at) dlr.dehttps://orcid.org/0000-0001-9948-3353UNSPECIFIED
Iochem, Pelinpelin.iochem (at) dlr.dehttps://orcid.org/0000-0003-4308-8439171938515
Tasnim, Samirasamira.tasnim (at) dlr.dehttps://orcid.org/0000-0002-0305-2071171938518
Davis, Fredyfredy.davis (at) dlr.deUNSPECIFIEDUNSPECIFIED
Date:2024
Journal or Publication Title:Journal of Space Weather and Space Climate
Refereed publication:Yes
Open Access:Yes
Gold Open Access:Yes
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:14
DOI:10.1051/swsc/2024029
Publisher:EDP Sciences
ISSN:2115-7251
Status:Published
Keywords:Ionosphere / Coupling / Auroral zone / Solar wind / Convection / Joule heating
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Earth Observation
DLR - Research area:Raumfahrt
DLR - Program:R EO - Earth Observation
DLR - Research theme (Project):R - Solar-Terrestrial coupling processes, R - Solar-Terrestrial Physics SO
Location: Neustrelitz
Institutes and Institutions:Institute for Solar-Terrestrial Physics > Solar-Terrestrial Coupling Processes
Deposited By: Borries, Dr. Claudia
Deposited On:18 Nov 2024 09:53
Last Modified:18 Nov 2024 09:53

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