- 1Institute of Ionosphere, National Technical University “Kharkiv Polytechnic Institute”, Kharkiv, Ukraine (mrezn.cbk@gmail.com)
- 2Space Research Centre of Polish Academy of Sciences, Warsaw, Poland (mreznychenko@cbk.waw.pl)
- 3University of Alabama in Huntsville, Huntsville, United States
- 4State Institution National Antarctic Scientific Center, Ministry of Education and Science of Ukraine, Kyiv, Ukraine
- 5MIT Haystack Observatory, Westford, MA, United States
- 6Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
- 7JUPC-IonSAT, IEEC-UPC, Universitat Politècnica de Catalunya, Barcelona, Spain
- 8Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Kharkiv, Ukraine
A typical long-duration positive ionospheric storm (LDPS) developed in the midlatitude ionosphere in the European sector in response to a strong geomagnetic storm of February 26-27, 2023 (Kp = 7-, minimum SYM-H = -161 nT). To advance the current understanding of storm-time midlatitude ionosphere, we investigated the drivers of this LDPS using combination of multi-instrument observations and modeling, with focus on magnetically conjugate locations. Simulations with the field line interhemispheric plasma (FLIP) model constrained by the observed F2-layer peak height (hmF2) and density (NmF2) data at Kharkiv (50oN, 36oE) and Grahamstown (33.3oS, 26.5oE) were validated with the O/N2 ratio data from the Global Ultraviolet Imager (GUVI). Our results indicate that neither the F2-layer peak uplift nor the O/N2 ratio increase can be considered exclusive drivers of an LDPS. Each driver can be dominant depending on conditions. An LDPS can develop even when the hmF2 decreases and sometimes, a small hmF2 increase of ~10-20 km can cause a strong LDPS. Similarly, an O/N2 increase is not a primary or necessary condition for an LDPS to develop but a small O/N2 increase of ~20-30% can cause a prominent LDPS. Finally, the formation of a positive or negative storm can be inhibited if the raising/lowering of hmF2 is counterbalanced by a decrease/increase in the O/N2 ratio.
How to cite: Reznychenko, M., Kotov, D., Richards, P. G., Bogomaz, O., Goncharenko, L., Paxton, L. J., Hernandez-Pajares, M., Reznychenko, A., Shkonda, D., Barabash, V., and Domnin, I.: Investigation of the Drivers of Long-Duration Positive Ionospheric Storms During the Geomagnetic Storm on February 26-27, 2023, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5836, https://doi.org/10.5194/egusphere-egu25-5836, 2025.