PROMPT PENETRATION ELECTRIC FIELDS AND PARTICLE PRECIPITATION AS DRIVERS OF STORM-TIME IONOSPHERIC RESPONSE

This study investigated the interplanetary and magnetospheric phenomena responsible for the intense geomagnetic storm of 9 March 2012 (minimum Dst ≈ −145 nT; interplanetary Bz ≈ −16 nT, obtained from OMNIWeb), using the superposed epoch method. Hourly foF2 values from six ionosonde stations spanning five longitudinal sectors: Moscow and Port Stanley (high latitude), Brisbane and Grahamstown (middle latitude), and Darwin and Puerto Rico (low latitude) were obtained from the SPIDR network and superposed about the Dst-minimum epoch over a ±72 h window. High-latitude foF2 increased near storm onset and was suppressed during recovery, consistent with intensified auroral particle precipitation. Middle-latitude stations showed a brief onset enhancement followed by pronounced depletion around Dst minimum that persisted into recovery, while low-latitude stations exhibited a positive response after commencement, depletion near Dst minimum, and recovery-phase enhancement. The close correspondence between the Dst/Bz variation and the foF2 response across all latitudes indicates a common interplanetary driver for both the geomagnetic and ionospheric disturbances. Prompt penetration electric fields are inferred to govern the middle-latitude depletion-then-enhancement pattern, while particle precipitation is implicated in the high-latitude enhancement. These findings align with recent superposed-epoch and case studies of the 2023–2025 superstorm sequence, reaffirming the value of the superposed epoch method for isolating storm-time ionospheric morphology across the global ionosonde network