|
|
Prediction for CME (2022-06-02T06:09:00-CME-001)CME Observed Time: 2022-06-02T06:09ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/20403/-1 CME Note: The likely source for this CME is a filament eruption which is centered around on S35W40 best seen in SDO AIA 193/171/304 A starting around 2022-06-02T05:20Z, though it was noted in SDO 171 that faint field lines were seen leaving the disk which were out-ahead of the eruption off the limb and not associated with the filamentary material. Clear arrival signature at L1: sudden increase in B total to approximately 11.5 nT (eventually going to over 14 nT), accompanied by a sharp temporary increase in density to 51 n(cm^-3) and ion temperature. Clear shock in the magnetic field, rotation of the Bz component (briefly reaching -11 nT), gradual rotation of Bx. Solar wind speed jumped from 260 km/s to approximately 315 km/s. CME Shock Arrival Time: 2022-06-06T09:20Z Observed Geomagnetic Storm Parameters due to CME: Max Kp: 3.0 Predicted Arrival Time: 2022-06-05T14:34Z Confidence that the CME will arrive: 61.5% Predicted geomagnetic storm max Kp range due to CME: 3.33333 - 5.33333 Prediction Method: Average of all Methods Prediction Method Note: This is the auto generated average of all submitted predictions for this CMELead Time: -22715.60 hour(s) Difference: 18.77 hour(s) Prediction submitted by Auto Generated (CCMC) on 2025-01-07T20:56Z |
|
CCMC
Rules of the Road: CCMC requests that users notify the CCMC, CME
model/technique developers and submitting forecasters/researchers before
performing event and validation studies with data from the CME Arrival
Time Scoreboard. It is recommended that such studies be performed with
the knowledge and collaboration of developers and submitting
forecasters/researchers. Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy |