Interhemispheric comparison of the ionosphere and plasmasphere total electron content using GPS, radio occultation and ionosonde observations
| Autor: | Jean-Marie Chevalier, Tshimangadzo Merline Matamba, Mpho Tshisaphungo, Zama T. Katamzi-Joseph, Gopi Seemala, Elisa Pinat, John Bosco Habarulema, Dalia Buresova, Daniel Okoh, Nicolas Bergeot |
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| Rok vydání: | 2021 |
| Předmět: |
Ionospheric storm
Atmospheric Science 010504 meteorology & atmospheric sciences Total electron content TEC Aerospace Engineering Astronomy and Astrophysics Plasmasphere Space weather Geodesy 01 natural sciences Physics::Geophysics Geophysics Space and Planetary Science Physics::Space Physics 0103 physical sciences General Earth and Planetary Sciences Radio occultation Ionosphere 010303 astronomy & astrophysics Ionosonde Physics::Atmospheric and Oceanic Physics Geology 0105 earth and related environmental sciences |
| Zdroj: | Advances in Space Research. 68:2339-2353 |
| ISSN: | 0273-1177 |
| DOI: | 10.1016/j.asr.2021.05.004 |
| Popis: | We present a comparison of the ionosphere and plasmasphere total electron content over nearly geomagnetic conjugate locations Pruhonice ( 50.0 ° N, 14.6 ° E; 45.7 ° N geomagnetic), Czech Republic and Hermanus ( 34.4 ° S, 19.2 ° E; 42.3 ° S geomagnetic), South Africa during the low solar activity period of 2009–2010. The bottomside ionosphere, topside ionosphere and plasmaspheric contributions to the total electron content (TEC) derived from the Global Positioning System (GPS) observations are separately estimated from ionosonde and Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) radio occultation data. Over the ionosonde location, COSMIC electron density (Ne) profiles are considered when the maximum height of the F2 layer (hmF2) lies within spatial resolutions of 4.5 ° × 4.5 ° in latitudes/longitudes, and the Ne profile does not exceed 10 ° . For the first time, we have statistically quantified the topside ionosphere contribution to GPS TEC based on radio occultation data and revealed that it accounts for about 50% of the TEC during low solar activity periods. Finally, we have demonstrated that the determination of electron content contribution at different altitudes is important for understanding ionospheric storm mechanisms during space weather events especially geomagnetic storms. |
| Databáze: | OpenAIRE |
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