000005204 001__ 5204
000005204 005__ 20210127153202.0
000005204 037__ $$aCTALK-2021-0018
000005204 100__ $$aHabarulema, J. B. 
000005204 245__ $$aInterhemispheric comparison of the ionospheric electron density response during geomagnetic storm conditions
000005204 260__ $$c2020
000005204 269__ $$c2020-05-07
000005204 520__ $$aThe ionospheric electron density response to the occurrence of geomagnetic storms remains one of the challenges that is less understood partially on both short and long-term scales. This is even more complicated given that different locations within the same latitude region (for example in mid-latitudes) at times show different electron density responses as a result of complex dynamic and electrodynamics processes that may be present during one storm duration.  Mid-latitude regions are influenced by storm induced processes originating from both low and high latitudes. Using a combination of ionosonde and Global Navigational Satellite Systems (GNSS) observations, we show differences and or similarities in the electron density response during selected storm periods in both northern and southern hemisphere over the Europe-African sector. Physical mechanisms at play within different storm phases are explored using both observations and empirical modeling efforts.  
000005204 536__ $$aBEZA/$$cBEZA/$$fBEZA
000005204 594__ $$aSTCE
000005204 700__ $$aBergeot, N. 
000005204 700__ $$aChevalier, J.-M. 
000005204 700__ $$aPinat, E. 
000005204 700__ $$aBuresova, D. 
000005204 700__ $$aMatamba, T. 
000005204 700__ $$aKatamzi-Joseph, Z. 
000005204 773__ $$tEGU online
000005204 8560_ $$fjean-marie.chevalier@observatoire.be
000005204 85642 $$ahttps://meetingorganizer.copernicus.org/EGU2020/EGU2020-8268.html
000005204 906__ $$aContributed
000005204 980__ $$aCTALKCONT