CME ScoreBoard Header

CME Scoreboard

CME Scoreboard: Prediction Detail

Prediction for CME (2024-11-25T03:12:00-CME-001)

CME Observed Time: 2024-11-25T03:12Z
iSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/35303/-1
CME Note: CME first seen to the SSE in SOHO LASCO C2 starting at 2024-11-25T03:12Z. CME also seen to the SSE in SOHO LASCO C3 and STEREO A COR2. The source of this CME is likely a small filament eruption centered around S40-45E28 that is visible in SDO AIA 304 and SDO AIA 193 starting about 2024-11-25T01:30Z. Arrival on 2024-11-29T02:15Z is categorized by a quick increase in Bt from around 8 nT->12.5 nT, with Bz initially northward, with further enhancement possible as the signature develops. Small jump in solar wind speed from about 370 km/s->400 km/s with small bumps in density and temperature also observed. This is mainly the likely arrival of CME 2024-11-25T21:24Z, with possible additional influences from CMEs 2024-11-25T03:12Z and 2024-11-25T04:00Z.
CME Shock Arrival Time: 2024-11-29T02:15Z
Observed Geomagnetic Storm Parameters due to CME:
----

Predicted Arrival Time: 2024-11-28T20:00Z
Predicted geomagnetic storm max Kp range due to CME: 2.0 - 4.0
Prediction Method: Average of all Methods
Prediction Method Note:
This is the auto generated average of all submitted predictions for this CME
Lead Time: 81.95 hour(s)
Difference: 6.25 hour(s)
Prediction submitted by Auto Generated (CCMC) on 2024-11-25T16:18Z
CME Scoreboard Footer

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.

If you are looking for the official U.S. Government forecast for space weather, please go to NOAA's Space Weather Prediction Center (https://swpc.noaa.gov). This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement