Differences in regular and storm time ionospheric variability at magnetically conjugated locations of the Northern and Southern Hemisphere
- 1Institute of Atmospheric Physics, CAS, Ionosphere and Aeronomy, Prague 4, Czechia (buresd@ufa.cas.cz)
- 2SANSA Space Science, Hermanus, South Africa
- 3Mathematics and Science Department, Miami Dade College, Miami, Florida, USA
- 4JFCONSULT, Tourrettes, France
The paper is focused on differences/similarities in regular daily ionospheric variability and in the ionospheric response to CME- and CIR/CHSS-related magnetic disturbances above magnetically conjugated ionospheric stations located at Northern and Southern Hemisphere. We analysed variability of critical frequency foF2 and the F2 layer peak height hmF2 obtained for European-African sector for initial, main and recovery phases of magnetic storms of different intensity, which occurred within the last two solar cycles. We also used exclusively GPS-based detection methods, specifically information on TEC, TEC deviations in space and time from a background reference (dTEC), and the Rate of TEC change in time (ROT), all inferred from GPS receiver networks in Europe and Africa to compare behavior of Large Scale Traveling Ionospheric Disturbances (LSTIDs) at both hemispheres. We conclude that hemispheric conjugacy of LSTID is highly probable during both CME- and CIR/CHSS-related storms while interhemispheric circulation rather unlikely but still occurring during some periods.
How to cite: Buresova, D., Habarulema, J. B., Araujo-Pradere, E., Tshisaphungo, M., Watermann, J., and Lastovicka, J.: Differences in regular and storm time ionospheric variability at magnetically conjugated locations of the Northern and Southern Hemisphere , EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-4611, https://doi.org/10.5194/egusphere-egu21-4611, 2021.