Super‐Intense Geomagnetic Storm on 10–11 May 2024: Possible Mechanisms and Impacts

One of the most intense geomagnetic storms of recent times occurred on 10–11 May 2024. With a peak negative excursion of Sym‐H below −500 nT, this storm is the second largest of the space era. Solar wind energy transferred through radiation and mass coupling affected the entire Geospace. Our study revealed that the dayside magnetopause was compressed below the geostationary orbit (6.6 RE) for continuously ∼6 hr due to strong Solar Wind Dynamic Pressure (SWDP). Tremendous compression pushed the bow‐shock also to below the geostationary orbit for a few minutes. Magnetohydrodynamic models suggest that the magnetopause location could be as low as 3.3RE. We show that a unique combination of high SWDP (≥15 nPa) with an intense eastward interplanetary electric field (IEFY ≥ 2.5 mV/m) within a super‐dense Interplanetary Coronal Mass Ejection lasted for 409 min–is the key factor that led to the strong ring current at much closer to the Earth causing such an intense storm. Severe electrodynamic disturbances led to a strong positive ionospheric storm with more than 100% increase in dayside ionospheric Total Electron Content (TEC), affecting GPS positioning/navigation. Further, an HF radio blackout was found to occur in the 2–12 MHz frequency band due to strong D‐ and E‐region ionization resulting from a solar flare prior to this storm. Plain Language Summary Life and a habitable atmosphere are sustained on Earth thanks to the protective and far‐stretched magnetic shield around the Earth, known as the Magnetosphere, which protecting the humanosphere from the hazardous solar wind particles that are continuously emanated from the Sun. However, massive solar wind ejections from the Sun often disturb the Earth's magnetosphere and affect mankind and critical space‐ and ground‐based technological infrastructure. When higher amounts of the solar wind traveling with supersonic speeds impact, the Earth's magnetosphere compresses significantly, and the crucial satellites in space become directly exposed to hazardous solar wind. Further, strong and rapid disturbances in the geomagnetic field and ionosphere could significantly affect the operations of various technical systems on ground, like electrical power grids, GNSS‐based precise navigation, etc. The strongest geomagnetic storm of the past three decades has recently occurred on 10–11 May 2024. This study investigates the solar sources and the possible mechanisms responsible for the occurrence of such an intense geomagnetic s