|
|
Prediction for CME (2024-05-23T07:12:00-CME-001)CME Observed Time: 2024-05-23T07:12ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/31098/-1 CME Note: This CME is visible to the SE in SOHO LASCO C2/C3 and STEREO A COR2 imagery. The source is likely a small filament eruption centered near S12E03 which begins to lift-off around 2024-05-23T06:45Z as seen in SDO AIA 131, 171, 193, 304 imagery. This eruption appears to deflect towards the southeast as it leaves the solar disk/initial source location. Post eruptive arcades begin to from in SDO AIA 171 and 193 imagery around 07:20Z. This event partially overlaps with CME: 2024-05-23T06:48Z. Possible arrival signature: Characterized by a minor amplification of magnetic field components with Btotal increasing from 3nT at 2024-05-26T14:35Z to 8nT at 20:13Z. There are a few minor increases in solar wind speed prior to the amplification magnetic field components, most notably an increase from ~350 km/s at 11:08Z to ~450 km/s at 13:05Z. There are no significant increases in temperature or density observed, beyond an increase in density to 8 N/cm^3 at 2024-05-27T03:31Z. An alternative arrival signature could be the one starting at 2024-05-27T02:42Z when it looks like the ICME crossed the spacecraft, with a slight descending profile in the plasma and magnetic field indicating a glancing blow and the possible start of the magnetic cloud around 06:12Z (according to Carlos Perez Alanis, LASSOS team). CME Shock Arrival Time: 2024-05-26T14:35Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2024-05-27T00:01Z (-12.0h, +12.0h) Confidence that the CME will arrive: 30.0% Predicted geomagnetic storm max Kp range due to CME: 2.0 - 5.0 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: 4.5 GONG: mrzqs Note that this arrival time forecast is based on the simulation but is then adjusted by a human-in-the-loop. Please specify following CME input parameters. Time at 21.5Rs boundary: 2024-05-23T15:53Z Radial velocity (km/s): 320 Longitude (deg): 025E Latitude (deg): 12S Half-angular width (deg): 25 Notes: Averaged fit for SE centre-disc disappearing filament, visible on e.g. Learmonth H-Alpha around 23/0630UTC, perhaps narrowly preceeded by a second event to its southeast 23/0600UTC. Modelled as an off-ecliptic southward lobe in the latter case, but in this (former) case as an on-ecliptic slightly eastward emission. Low confidence due to poorly-defined ejecta to fit to, but also questionable MOSWOC Enlil background wind field evolution (CH39/- onset or presence). Result is a slight glance, hence long error bars when all else considered. Space weather advisor: Michael LawrenceLead Time: 50.17 hour(s) Difference: -9.43 hour(s) Prediction submitted by Met Office (Met Office) on 2024-05-24T12:25Z |
|
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 |