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Persistent high-latitude ionospheric response to solar wind forcing

Borries, Claudia und Iochem, Pelin und Tasnim, Samira und 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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Offizielle URL: https://www.swsc-journal.org/articles/swsc/full_html/2024/01/swsc230082/swsc230082.html

Kurzfassung

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.

elib-URL des Eintrags:https://elib.dlr.de/208516/
Dokumentart:Zeitschriftenbeitrag
Titel:Persistent high-latitude ionospheric response to solar wind forcing
Autoren:
AutorenInstitution oder E-Mail-AdresseAutoren-ORCID-iDORCID Put Code
Borries, Claudiaclaudia.borries (at) dlr.dehttps://orcid.org/0000-0001-9948-3353NICHT SPEZIFIZIERT
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.deNICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Datum:2024
Erschienen in:Journal of Space Weather and Space Climate
Referierte Publikation:Ja
Open Access:Ja
Gold Open Access:Ja
In SCOPUS:Ja
In ISI Web of Science:Ja
Band:14
DOI:10.1051/swsc/2024029
Verlag:EDP Sciences
ISSN:2115-7251
Status:veröffentlicht
Stichwörter:Ionosphere / Coupling / Auroral zone / Solar wind / Convection / Joule heating
HGF - Forschungsbereich:Luftfahrt, Raumfahrt und Verkehr
HGF - Programm:Raumfahrt
HGF - Programmthema:Erdbeobachtung
DLR - Schwerpunkt:Raumfahrt
DLR - Forschungsgebiet:R EO - Erdbeobachtung
DLR - Teilgebiet (Projekt, Vorhaben):R - Solar-Terrestrische Kopplungsprozesse, R - Solar-Terrestrische Physik SO
Standort: Neustrelitz
Institute & Einrichtungen:Institut für Solar-Terrestrische Physik > Solar-Terrestrische Kopplungsprozesse
Hinterlegt von: Borries, Dr. Claudia
Hinterlegt am:18 Nov 2024 09:53
Letzte Änderung:18 Nov 2024 09:53

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