After-effects of geomagnetic storms: statistical analysis and theoretical explanation
Автор: Ratovsky K.G., Klimenko M.V., Klimenko V.V., Chirik N.V., Korenkova N.A., Kotova D.S.
Журнал: Солнечно-земная физика @solnechno-zemnaya-fizika
Статья в выпуске: 4 т.4, 2018 года.
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Our previous studies have shown the presence of daytime positive electron density disturbances during several days after the start of the recovery phase. The aim of this paper is to study after-effects of geomagnetic storms (after-storm effects), i.e. ionospheric effects observed on the 3-5th day after the beginning of the storm recovery phase. From numerical calculations with the GSM TIP model, we have found the main mechanisms for the formation of the after-storm effects. Using Irkutsk (52° N, 104° E) and Kaliningrad (54° N, 20° E) ionosonde data, we have carried out a statistical analysis of daytime ionospheric responses to geomagnetic storms. As a result of the analysis, we obtained averaged ionospheric responses at the beginning of the storm recovery phase and for five consecutive days. The statistical analysis results received near the beginning of the recovery phase are in good agreement with the well-known ionospheric effects of geomagnetic storms obtained in previous studies. For the first time, the obtained statistics of ionospheric responses observed on the 3-5th day after the beginning of the recovery phase allowed us to reveal the dependence of after-storm ionospheric effects on season, storm intensity, and ionosonde geomagnetic latitude. In addition, we for the first time present the interpretation of after-storm ionospheric effects from numerical simulation results.
Geomagnetic storm, after-storm ionospheric effects, statistics, gsm tip model
Короткий адрес: https://sciup.org/142220307
IDR: 142220307 | DOI: 10.12737/szf-44201804