This study reports comprehensive observations for the G5-level geomagnetic storm
that occurred from May 10 to 12, 2024, the most intense event since the 2003
Halloween storm. The storm was triggered by a series of coronal mass ejections
(CMEs) originating from the merging of two active regions 13664/13668, which
formed a large and complex photospheric magnetic configuration and produced
X-class flares in early May 2024. Among the events, the most significant CME,
driven by an X2.2 flare on May 9, caught up with and merged with a preceding
slower CME associated with an X-class flare on May 8. These combined CMEs
reached 1 AU simultaneously, resulting in an extreme geomagnetic storm.
Geostationary satellite observations revealed changes in Earth’s
magnetosphere due to solar wind impacts, increased fluxes of high-energy
particles, and periodic magnetic field fluctuations accompanied by particle
injections. Extreme geomagnetic storms resulting from the interaction of the
solar wind with the Earth’s magnetosphere caused significant energy
influx into Earth’s upper atmosphere over the polar regions, leading to
thermospheric heating and changes in the global atmospheric composition and
ionosphere. As part of this global disturbance, significant disruptions were
also observed in the East Asian sector, including the Korean Peninsula.
Ground-based observations show strong negative storm effects in the ionosphere,
which are associated with thermospheric heating and resulting in decreases in
the oxygen-to-nitrogen ratio (O/N2) in high-latitude regions. Global
responses of storm-time prompt penetration electric fields were also observed
from magnetometers over the East-Asian longitudinal sector. We also briefly
report storm-time responses of aurora and cosmic rays using all-sky cameras and
neutron monitors operated by the Korea Astronomy and Space Science Institute
(KASI). The extensive observations of the G5-level storm offer crucial insights
into Sun-Earth interactions during extreme space weather events and may help
establish better preparation for future space weather challenges.