CME Scoreboard

Prediction for CME (2022-03-10T00:12:00-CME-001)

## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CMEs (STEREO A, Missions Near Earth)
##
## Message Issue Date: 2022-03-10T16:09:44Z
## Message ID: 20220310-AL-002
##
## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.


## Summary:

Multiple CMEs have been detected as follows:
1: S-type CME detected by STEREO A / SOHO. 

Start time of the event: 2022-03-10T00:12Z.

Estimated speed: ~452 km/s.

Estimated opening half-angle: 29 deg.

Direction (lon./lat.): -34/-14 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2022-03-10T00:12:00-CME-001

2: C-type CME detected by STEREO A / SOHO. 

Start time of the event: 2022-03-10T02:00Z.

Estimated speed: ~551 km/s.

Estimated opening half-angle: 34 deg.

Direction (lon./lat.): -53/-21 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2022-03-10T02:00:00-CME-001

Based on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that the CMEs may affect STEREO A.  The combined leading edge of the CMEs will reach STEREO A at 2022-03-13T00:33Z (plus minus 7 hours). 
  
The simulation also indicates that the CMEs may have a glancing blow at NASA missions near Earth. Simulations indicate that the combined flank of the CMEs will reach NASA missions near Earth at about 2022-03-13T21:00Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 2-4 (below minor).
   
  
Links to the movies of the modeled event (includes CMEs: 2022-03-10T00:12:00-CME-001, 2022-03-10T02:00:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20220310_101500_2.0_afwa_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20220310_101500_2.0_afwa_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20220310_101500_2.0_anim.tim-den-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20220310_101500_2.0_anim.tim-vel-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20220310_101500_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220310_101500_2.0_ENLIL_CONE_STA_timeline.gif


## Notes: 
These two CMEs are products from the same filament eruption.  The earlier CME (2022-03-10T00:12:00-CME-001) is overtaken by the later and faster CME (2022-03-10T02:00:00-CME-001) in SOHO coronagraph imagery, but they remain separate features even after that time and they are separate features in STEREO A coronagraph imagery.

SCORE CME typification system:
S-type: CMEs with speeds less than 500 km/s
C-type: Common 500-999 km/s
O-type: Occasional 1000-1999 km/s
R-type: Rare 2000-2999 km/s
ER-type: Extremely Rare >3000 km/s


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