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Prediction for CME (2025-11-10T13:08:00-CME-001)CME Observed Time: 2025-11-10T13:08ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/42600/-1 CME Note: Seemingly narrow eruption to the N from SOHO LASCO C2/C3 perspective, but appears wider and more to the N/NE in STEREO A COR2's field of view. From STEREO A's perspective, it drifts N as it moves out in the field of view. The source appears to be an eruption associated with filament ejecta visible to the N/NW from AR 14274 around 2025-11-10T12:00Z as seen in GOES SUVI 304. | The arrival of this CME was likely observed at L1 by ACE/DSCOVR around 2025-11-12T18:52Z, characterized by an amplification of magnetic field components with Btotal increasing from 19nT at 2025-11-12T18:52Z to about 40nT at 2025-11-12T19:00Z. The magnetic field parameters were previously enhanced due to the interplanetary shock starting at 2025-11-11T22:11Z. An increase in solar wind speed from about 580 km/s to 820 km/s was observed starting at about 2025-11-12T19:45Z after a brief period of unreliably low solar wind speed data which had occurred during the initial shock arrival. An increase in temperature was seen starting at 2025-11-12T19:45Z from about 71,000 K to about 764,000 K. A significant increase in temperature was observed starting at 2025-11-12T21:55Z, which may have been erroneous or unreliable data. A corresponding sudden increase in density was observed at 2025-11-12T19:41Z from about 4 p/cc to a peak value of 24 p/cc at 2025-11-12T19:49Z. CME Shock Arrival Time: 2025-11-12T18:52Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2025-11-13T08:21Z Predicted geomagnetic storm max Kp range due to CME: 3.5 - 5.5 Prediction Method: Median of all Methods Prediction Method Note: This is the auto generated median of all submitted predictions for this CME.Lead Time: 22.38 hour(s) Difference: -13.48 hour(s) Prediction submitted by Auto Generated (CCMC) on 2025-11-11T20:29Z |
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