Open Access

Table 1.

CMEs responsible for the great geomagnetic storm on 10 May 2024.

Events Date, Time Flare/ Source Time (UT) Height (R) Longitude Latitude Aspect Tilt Half Max Speed
(UT) filament region Initial-Final Initial-Final (deg) (deg) Ratio Angle Angle (km s−1)
(deg) (deg)
CME1 8, 5:36 X1.0 S18W10 05:48–10:18 5.8–26.9 16±3 −8±2 0.27±0.1 84±6 24±3 967

CME2 8, 12:24 M8.7 S19W11 12:36–15:54 5.4–22.4 13±2 −16±4 0.34±0.1 27±5 23±6 1142

CME3 8, 19:12 Filament N25E14 19:36–23:42 5.2–24.7 −27±5 4±6 0.24±0.1 79±2 15 ±5 991

CME4 8, 22:36 X1.02 S20W14 23:06–25:54 8.9–28.3 6±7 −18±3 0.26±0.12 15±10 18 ±7 1406

CME5 8, 22:36 M9.87 S19W28 23:06–26:42 4.6–22.5 38±6 −15±3 0.15±0.4 −83±8 16±8 1103

CME6 9, 9:24 X2.2 S20W22 09:24–12:06 3.9–25.4 27±3 −14±2 0.28±0.1 −77±4 23±3 1746

Notes. The second column shows the date and time for the first appearance of each CME in the SOHO/LASC0-C2 field of view. The GCS-model-fitted parameters for the CMEs are shown in Cols. 5 to 12. Columns 4 and 5 show the time and height range for which the GCS model fit was done. The last column shows the estimates of the maximum LE speed (v) of each CME during our observation duration in the coronagraphic field of view.

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