CME Scoreboard |
|
Prediction for CME (2021-08-23T06:36:00-CME-001)CME Observed Time: 2021-08-23T06:36ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/17559/-1 CME Note: The CME is a partial halo in SOHO LASCO C2/C3 and is in the NW of STA COR2A. The source is a filament eruption north of disk center seen at 02:00Z in SDO AIA 171/193/304. The L1 arrival signature seen by DSCOVR is characterized by a simultaneous jump in SW density, magnetic field and speed (from 360 to 420 km/s), as well as rotation of magnetic field components. CME Shock Arrival Time: 2021-08-27T00:25Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2021-08-27T09:00Z Prediction Method: WSA-ENLIL + Cone (Met Office) Prediction Method Note: Met Office ENLIL settings. ENLIL version: 2.7 Resolution: medium-res (512x60x180) (X1=0.1-1.7/uniform X2=30.-150./uniform X3=0.-360./uniform) Ambient settings: a3b2-sa1 WSA version: 2.2 Please specify following CME input parameters. Time at 21.5Rs boundary: 2021-08-23T15:57Z Radial velocity (km/s): 375 Longitude (deg): W005 Latitude (deg): N16 Half-angular width (deg): 31 Notes: CME originating from a large filament eruption in NE quadrant. Faint halo in Lasco C2 but obvious in STEREO A. High confidence in speed as confirmed with COR2 speed calculator Space weather advisor: Jay MerrellLead Time: 65.22 hour(s) Difference: -8.58 hour(s) Prediction submitted by Met Office (Met Office) on 2021-08-24T07:12Z |
|
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 |