Table 2
CMEs observed from AR 3664 08-11 May 2024. Approximate time of eruption, associated solar flare, CME location, speed, mass, angular width, radial width, and magnetic flux used in the simulations. The CME geoeffectiveness and parameters were assessed using SDO, SOHO/LASCO, and STEREO observations of the solar corona, CACTus CME detection, and the SOHO LASCO CME catalog. Not all parameters could be derived from the observations and qualitative assessment, and parameter assumptions were used, particularly for the CME mass and magnetic flux.
| Time [UT] | Solar flare | Location | Speed [km/s] | Mass [1012 kg] | Angular width [°] | Radial width [R0] | Magnetic flux [1020 Mx] | |
|---|---|---|---|---|---|---|---|---|
| 1 | 08 May 03:00 | M3.4 | S15W13 | 600 | 25 | 90 | 2 | 30 |
| 2 | 08 May 06:00 | X1.0 | S15W14 | 700 | 25 | 90 | 2 | 20 |
| 3 | 08 May 12:00 | M8.7 | S15W14 | 550 | 10 | 90 | 2 | 30 |
| 4 | 08 May 21:30 | X1.0 | S15W19 | 800 | 35 | 90 | 2 | 40 |
| 5 | 09 May 09:30 | X2.3 | S15W29 | 1700 | 25 | 90 | 2 | 30 |
| 6 | 09 May 18:30 | X1.1 | S15W29 | 1100 | 25 | 90 | 2 | 30 |
| 7 | 10 May 07:30 | X4.0 | S10W35 | 650 | 35 | 90 | 2 | 30 |
| 8 | 10 May 11:00 | M2.2 | S19W40 | 700 | 15 | 90 | 2 | 30 |
| 9 | 11 May 02:30 | X5.8 | S17W50 | 1400 | 35 | 90 | 2 | 30 |
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