Cahuasqui Llerena, Juan Andres und Hoque, Mohammed Mainul und Jakowski, Norbert und Buchert, Stephan und Kriegel, Martin und David, Paul und Vasylyev, Dmytro und Tagargouste, Youssef und Berdermann, Jens und Nielsen, Klaus (2024) Monitoring Ionospheric Gradients using Swarm onboard GPS and Langmuir-probe data. In: Swarm 10 Year Anniversary & Science Conference. European Space Agency ESA. Swarm 10 Year Anniversary & Science Conference, 2024-04-08 - 2024-04-12, Copenhagen, Denmark.
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Offizielle URL: https://www.swarm-anniversary-and-science.org/
Kurzfassung
Within the scope of MIGRAS, a project of Swarm DISC, we developed two new data products that focus on monitoring mid-scale plasma density irregularities with horizontal spatial scales in the order of about 100 km utilizing measurements from the Swarm satellites A and C in polar orbits at heights of about 460 km. Two new Swarm products are the total electron content (TEC) Gradient Ionosphere indeX (TEGIX) and the electron density (NE) Gradient Ionosphere indeX (NEGIX) derived from topside TEC and in-situ electron density measurements onboard GPS receivers and Langmuir probes. The TEGIX and NEGIX results during the St. Patrick‘s Day Storm on 17th March 2015 will be shown and discussed for both North-South and West-East components. For the same storm day, the NEGIX and TEGIX products are validated against the Gradient Ionosphere IndeX (GIX) derived from numerous ground GNSS stations data over the European region. We found that the North-South component of TEGIX and NEGIX products correlate very well with the same component of the ground-based GIX data. A prototype data product of NEGIX and TEGIX has been produced for the time period 2018-01-01 until 2018-06-30. The data set has nearly 2 million records of estimated density gradient TEGIX and NEGIX vectors. Considering six months of data, NEGIX is validated using basic statistical tests. Clear terminator related gradients at sunrise and sunset, i.e. ~6 and ~18 LT are observed. The NEGIX product shows consistent results with gradients at equatorial crests ~+/- 20 deg and also signatures of the mid-latitude ionospheric trough (MIT) at ~+/- 60 deg latitude. A use case of NEGIX for ionospheric scintillation modelling is discussed. An innovative scintillation modelling technique shows that the large gradients of electron density visible in the NEGIX are associated with high phase scintillation occurrence.
elib-URL des Eintrags: | https://elib.dlr.de/209502/ | ||||||||||||||||||||||||||||||||||||||||||||
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Dokumentart: | Konferenzbeitrag (Vortrag) | ||||||||||||||||||||||||||||||||||||||||||||
Zusätzliche Informationen: | Acknowledgement: The work is funded by the MIGRAS (Monitoring of Ionospheric Gradients At SWARM) project under the Swarm DISC Subcontract Doc. no: SW‐CO‐DTU‐GS‐133, Rev: 1, 13 September 2022. | ||||||||||||||||||||||||||||||||||||||||||||
Titel: | Monitoring Ionospheric Gradients using Swarm onboard GPS and Langmuir-probe data | ||||||||||||||||||||||||||||||||||||||||||||
Autoren: |
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Datum: | April 2024 | ||||||||||||||||||||||||||||||||||||||||||||
Erschienen in: | Swarm 10 Year Anniversary & Science Conference | ||||||||||||||||||||||||||||||||||||||||||||
Referierte Publikation: | Nein | ||||||||||||||||||||||||||||||||||||||||||||
Open Access: | Ja | ||||||||||||||||||||||||||||||||||||||||||||
Gold Open Access: | Nein | ||||||||||||||||||||||||||||||||||||||||||||
In SCOPUS: | Nein | ||||||||||||||||||||||||||||||||||||||||||||
In ISI Web of Science: | Nein | ||||||||||||||||||||||||||||||||||||||||||||
Verlag: | European Space Agency ESA | ||||||||||||||||||||||||||||||||||||||||||||
Status: | veröffentlicht | ||||||||||||||||||||||||||||||||||||||||||||
Stichwörter: | ESA, Swarm, ionosphere, GNSS, ionospheric indices, space weather | ||||||||||||||||||||||||||||||||||||||||||||
Veranstaltungstitel: | Swarm 10 Year Anniversary & Science Conference | ||||||||||||||||||||||||||||||||||||||||||||
Veranstaltungsort: | Copenhagen, Denmark | ||||||||||||||||||||||||||||||||||||||||||||
Veranstaltungsart: | internationale Konferenz | ||||||||||||||||||||||||||||||||||||||||||||
Veranstaltungsbeginn: | 8 April 2024 | ||||||||||||||||||||||||||||||||||||||||||||
Veranstaltungsende: | 12 April 2024 | ||||||||||||||||||||||||||||||||||||||||||||
Veranstalter : | European Space Agency ESA | ||||||||||||||||||||||||||||||||||||||||||||
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 - Weltraumwetterbeobachtung, R - Ionosphäre, R - GNSS Technologien und Dienste, R - Schwarmnavigation, R - Solar-Terrestrische Physik SO | ||||||||||||||||||||||||||||||||||||||||||||
Standort: | Neustrelitz | ||||||||||||||||||||||||||||||||||||||||||||
Institute & Einrichtungen: | Institut für Solar-Terrestrische Physik Institut für Solar-Terrestrische Physik > Weltraumwetterbeobachtung Institut für Solar-Terrestrische Physik > Weltraumwettereinfluß | ||||||||||||||||||||||||||||||||||||||||||||
Hinterlegt von: | Cahuasqui Llerena, Dr. Juan Andres | ||||||||||||||||||||||||||||||||||||||||||||
Hinterlegt am: | 04 Dez 2024 12:12 | ||||||||||||||||||||||||||||||||||||||||||||
Letzte Änderung: | 04 Dez 2024 12:12 |
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