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Comprehensive Magnetohydrodynamic Modeling of 10 Successive Coronal Mass Ejections Driving a Historic Geomagnetic Storm—the 2024 Mother’s Day Event

  • Authors: Shirsh Lata Soni, Anwesha Maharana, Sanchita Pal, Stefaan Poedts

Shirsh Lata Soni et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure A3.

EUHFORIA simulation of the CMEs 1–3, 1–4, 1–5, and 1–6 (top) and CMEs 1–7, 1–8, and 1–9 (bottom) overplotted on the Wind measurements (black). The dashed vertical green lines demarcate the observed shock signatures (S1, S2) and the shaded patches correspond to the observed intervals of the magnetic ejecta (E1, ..., E5) as characterized in Table 3. The plot shows top to bottom: the speed v, the proton number density np, the magnetic field components Bx, By, Bz, the total magnetic field strength ∣B∣, the disturbance storm index Dst, and the plasma beta β.

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