CME Scoreboard |
|
Prediction for CME (2024-08-01T07:24:00-CME-001)CME Observed Time: 2024-08-01T07:24ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/32420/-1 CME Note: This CME is visible as a partial halo to the west in SOHO LASCO C2/C3 and STEREO A COR2 coronagraph imagery. The source is an M8.2 flare and eruption from Active Region 13768 (S15W80) starting around 2024-08-01T07:00Z as seen in GOES SUVI 131, 171, 195, 284, 304 imagery. A wide opening of field lines is visible in GOES SUVI 171, 195, and 284 imagery at this time as well. Arrival: there is a clear ICME arrival signatures with a shock (according to analysis by the LASSOS team (Carlos Perez Alanis). During the shock B total reaches 19.5 nT and density gets increased to 20p/cc, followed by a period of significant negative Bz reaching -17nT. This signature of ICME shock is preceded by a less clear disturbance in the magnetic field at L1 with Btotal increasing from 8nT at 2024-08-04T04:48Z to 15nT at 06:11Z followed by a protracted period of negative Bz. CME Shock Arrival Time: 2024-08-04T13:21Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2024-08-03T12:02Z Predicted geomagnetic storm max Kp range due to CME: 4.0 - 6.0 Prediction Method: SARM Prediction Method Note: CME observed at 21.5 Rs: 2024-08-01 10:49 â- Time at C2: 2024-08-01 07:24 â- Radial speed: 1100.0 km/s â- Half angle: 50 deg â- Eruption location: N07W50 âInferences: ââ - No flare association was found âPredictions for Earth: ââ - In-situ shock speed: 736.00 km/s ââ - Shock arrival time: 2024-08-03 12:02 (i.e. predicted transit time: 52.65 hours)Lead Time: 61.52 hour(s) Difference: 25.32 hour(s) Prediction submitted by Marlon Nunez (UMA) on 2024-08-01T23:50Z |
|
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 Collection Consent Agreement |