Ionospheric disturbances under low solar activity conditions

• Published in: Advances in space research Vol. 54; no. 2; pp. 185 - 196
• Main Authors: Buresova, D., Lastovicka, J., Hejda, P., Bochnicek, J.
• Format: Journal Article
• Language: English
• Published: Elsevier Ltd 01.07.2014
• Subjects: F 2 region; Ionosphere; Ionospheric variability; Latitude; Magnetic disturbances; Magnetic storms; Phases; Solar activity; Solar minimum; Storms; Ionospheric variability; Solar minimum; Ionosphere; Magnetic storms
• ISSN: 0273-1177; 1879-1948
• DOI: 10.1016/j.asr.2014.04.007

The paper is focused on ionospheric response to occasional magnetic disturbances above selected ionospheric stations located at middle latitudes of the Northern and Southern Hemisphere under extremely low solar activity conditions of 2007–2009. We analyzed changes in the F2 layer critical frequency foF2 and the F2 layer peak height hmF2 against 27-days running mean obtained for different longitudinal sectors of both hemispheres for the initial, main and recovery phases of selected magnetic disturbances. Our analysis showed that the effects on the middle latitude ionosphere of weak-to-moderate CIR-related magnetic storms, which mostly occur around solar minimum period, could be comparable with the effects of strong magnetic storms. In general, both positive and negative deviations of foF2 and hmF2 have been observed independent on season and location. However positive effects on foF2 prevailed and were more significant. Observations of stormy ionosphere also showed large departures from the climatology within storm recovery phase, which are comparable with those usually observed during the storm main phase. The IRI STORM model gave no reliable corrections of foF2 for analyzed events.