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Prediction for CME (2022-08-18T11:00:00-CME-001)

CME Observed Time: 2022-08-18T11:00Z
iSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/21261/-1
CME Note: The CME has a separate shock that is wider than the bulk of the CME. The bulk is visible to the SW in SOHO LASCO C2, C3 and STEREO A COR2. The shock is wider and more faint. There is a visible EUV wave along the SE of the source location as seen in SDO/AIA 193, moving/opening field lines are visible in SDO/AIA 193 and 171. Filament material is seen ejecting from the source location in SDO/AIA 304 and STEREO A EUVI 195. The eruption begins around 10:10Z with a flare as the potential trigger. The arrival is characterized by a rapid increase in solar wind density, magnetic field intensity, temperature, and speed with some component rotations present in the magnetic field after a period of very little to no rotation present in the magnetic field starting around 2022-08-20T17:24Z. These arrival signatures may be that of an ICME sheath that is followed by a flux rope beginning 2022-08-21T03:55Z but may also include more than one ICME arrival given the complexity of the solar wind signature.
CME Shock Arrival Time: 2022-08-20T17:24Z
Observed Geomagnetic Storm Parameters due to CME:
Max Kp: 4.0

Predicted Arrival Time: 2022-08-21T03:00Z (-7.0h, +7.0h)
Predicted geomagnetic storm max Kp range due to CME: 3.0 - 4.0
Prediction Method: WSA-ENLIL + Cone (NASA M2M)
Prediction Method Note:
## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (Parker Solar Probe, STEREO B, Mars, STEREO A, Missions Near Earth)
##
## Message Issue Date: 2022-08-18T16:48:07Z
## Message ID: 20220818-AL-003
##
## 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:

O-type CME detected by STEREO A / SOHO. 

Start time of the event: 2022-08-18T11:00Z.

Estimated speed: ~1076 km/s.

Estimated opening half-angle: 35 deg.

Direction (lon./lat.): 17/-30 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2022-08-18T11:00:00-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 this CME may affect Parker Solar Probe, STEREO B, Mars (glancing blow), and STEREO A (glancing blow).  The leading edge or flank of the CME will reach Parker Solar Probe at 2022-08-19T13:44Z, STEREO B at 2022-08-21T02:13Z, Mars at 2022-08-22T08:00Z, and STEREO A at 2022-08-21T04:00Z (plus minus 7 hours). 

The simulation also indicates that the CME may have a glancing blow at NASA missions near Earth. Simulations indicate that the flank of the CME will reach NASA missions near Earth at about 2022-08-21T03:00Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 3-4 (below minor).
   
  
Links to the movies of the modeled event (includes CME: 2022-08-18T11:00:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_anim.tim-den-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_anim.tim-vel-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_ENLIL_CONE_PSP_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_ENLIL_CONE_STA_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_ENLIL_CONE_STB_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220818_141000_2.0_ENLIL_CONE_Mars_timeline.gif


## Notes: 

This CME event (2022-08-18T11:00:00-CME-001) is associated with an M1.3 flare with ID 2022-08-18T10:04:00-FLR-001 which peaked at 2022-08-18T10:09Z from AR 13078 (S25W35) and possibly the M1.5 flare with ID 2022-08-18T10:37:00-FLR-001 which peaked at 2022-08-18T10:55Z from AR 13078 (S25W35).


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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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.
Lead Time: 48.60 hour(s)
Difference: -9.60 hour(s)
Prediction submitted by Carina Alden (M2M Office) on 2022-08-18T16:48Z
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