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Prediction for CME (2025-09-30T09:24:00-CME-001)CME Observed Time: 2025-09-30T09:24ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/41522/-1 CME Note: CME seen to the SW in SOHO LASCO C2, STEREO A COR2, and GOES CCOR-1. Source is a large filament eruption seen near the SW limb of the Earth-facing disk, and in the SW quadrant of the STEREO-A-facing disk. The filament can be seen spanning S35W60 to S15W108 and beginning to show movement at 2025-09-30T08:36Z. An associated M2.6 flare peaking at 2025-90-30T09:40Z and a narrow jet of ejecta, both from AR 14227 (S17W58), can be seen in GOES SUVI 304. Liftoff of material and post-eruptive brightening can also be seen in STEREO A EUVI 195/304 imagery. CME was not detected at Earth. Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2025-10-03T00:00Z Confidence that the CME will arrive: 20.0% Predicted geomagnetic storm max Kp range due to CME: 5.0 - 5.0 Prediction Method: Other (SIDC) Prediction Method Note: Expected arrival time: 2025-10-03T00:00:00Z
Arrival time uncertainty: 15
Estimated peak K: 5
Peak K uncertainty: 1
Probability of arrival: 20
CME start time: 2025-09-30T09:30:00Z
:Issued: 2025 Oct 01 1231 UTC
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# DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC #
# (RWC Belgium) #
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SIDC URSIGRAM 51001
SIDC SOLAR BULLETIN 01 Oct 2025, 1230UT
SIDC FORECAST
...
Coronal mass ejections: Further analysis of the Coronal Mass Ejection (SIDC
CME 565) that lifted off at 09:45 UTC on September 30, suggests a small
chance for a glancing blow arrival starting from the UTC evening on October
02, but with low confidence.
Lead Time: 53.40 hour(s)Difference: ----- Prediction submitted by Anna Chulaki (M2M SWAO) on 2025-09-30T18:36Z |
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