Abstract:
We investigated the ionosphere response to the two severe geomagnetic storms in the ascending phase of solar cycle 25 which
occurred during the 23-24 March 2023 (SYM-Hmin = −169 nT) and 23-24 April 2023 (SYM-Hmin = −233 nT) using a
latitudinally aligned dense network of Global Navigation Satellite System (GNSS) receivers, magnetometers, and digisonde
along the Indian longitude sector. The significant variations in TEC during the storm’s main and recovery phases are mainly
linked to the influence of westward Disturbance Dynamo Electric Fields (DDEFs). During the initial phase of the March
23-24 geomagnetic storm, no changes in daytime TEC were observed, despite the storm occurring at noon time with a southward
IMF Bz due to the influence of electron density in the top side ionosphere. Furthermore, both pre-reversal enhancement
(PRE) and ionosphere irregularities are suppressed within two hours of their onset during the main phase of the March 23-
24 storm, owing to the westward transition of zonal electric fields from an eastward direction. During the recovery phase of
both storms, a daytime positive storm effect is observed over the dip equatorial region, while the beyond equatorial ionization
anomaly (EIA) and mid-latitude regions perceived a negative ionospheric storm effect. This phenomenon is attributed to the
influence of the dominant westward DDEFs during the period. Moreover, these DDEFs effectively inhibited the equinoctial
manifestation of PRE effects and post-sunset ionospheric irregularities during the recovery phase of both storms. These findings
are further confirmed with supporting information from TEC recorded by Swarm satellites, model-derived ionospheric
electric fields, and thermospheric O/N2. The results from this study may advance the understanding of ionospheric response
to severe geomagnetic storms under the prevailing westward DDEFs during the dayside recovery phase, complementing the
global efforts for more reliable space weather modeling and prediction services
