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Prediction for CME (2022-08-13T18:48:00-CME-001)

CME Observed Time: 2022-08-13T18:48Z
iSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/21175/-1
CME Note: This CME is visible in the SSE of SOHO LASCO C2/C3 and the SSW of STEREO A COR2. Source eruption is seen as an EUV wave and dimming near AR 13078 starting around 2022-08-13T15:30Z and best seen in SDO AIA 193 and STEREO A EUVI 195. There is a definite shock on 2022-08-17T02:16Z which indicates the arrival of a CME, but it is possible the arrival is also associated with a CME first seen on 2022-08-14T12:48Z. Apart from temperature, we observe sudden jumps in the total magnetic field, proton density, and bulk speed. A sheath region appears to follow the shock. The sheath region can be seen as having turbulent field components, elevated total magnetic field, proton density, and temperature compared to the background solar wind. The high-speed stream can be identifiable starting around 2022-08-17T14:34Z by looking at the compression in the total magnetic field and proton density and increasing bulk speed and temperature afterward.
CME Shock Arrival Time: 2022-08-17T02:16Z
Observed Geomagnetic Storm Parameters due to CME:
Max Kp: 6.0

Predicted Arrival Time: 2022-08-16T18:00Z (-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 update (Parker Solar Probe, STEREO A, STEREO B, Missions Near Earth)
##
## Message Issue Date: 2022-08-15T13:13:01Z
## Message ID: 20220815-AL-001
##
## 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:

Update on CME with ID 2022-08-13T18:48:00-CME-001 (see previous notification 20220814-AL-002).  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 (glancing blow), STEREO A (glancing blow), and STEREO B (glancing blow).  The flank of the CME will reach Parker Solar Probe at 2022-08-15T14:00Z, STEREO A at 2022-08-16T14:00Z, and STEREO B at 2022-08-17T06:00Z (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 2022-08-16T18:00Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 3-4 (below minor).
   

Updated CME parameters are:

Start time of the event: 2022-08-13T18:48Z.

Estimated speed: ~679 km/s.

Estimated opening half-angle: 26 deg.

Direction (lon./lat.): -9/-25 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2022-08-13T18:48:00-CME-001


Links to the movies of the modeled event (includes CME: 2022-08-13T18:48:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_anim.tim-den-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_anim.tim-vel-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_ENLIL_CONE_PSP_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_ENLIL_CONE_STA_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20220813_235200_2.0_ENLIL_CONE_STB_timeline.gif


## Notes: 

The previous simulation result did not include an arrival at STEREO A (see previous notification 20220814-AL-002) and included an S-type CME event with Activity ID 2022-08-13T19:48:00-CME-001.


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: 37.05 hour(s)
Difference: 8.27 hour(s)
Prediction submitted by Mary Aronne (M2M Office) on 2022-08-15T13:13Z
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