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Prediction for CME (2021-08-23T06:36:00-CME-001)

CME Observed Time: 2021-08-23T06:36Z
iSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/17559/-1
CME Note: The CME is a partial halo in SOHO LASCO C2/C3 and is in the NW of STA COR2A. The source is a filament eruption north of disk center seen at 02:00Z in SDO AIA 171/193/304. The L1 arrival signature seen by DSCOVR is characterized by a simultaneous jump in SW density, magnetic field and speed (from 360 to 420 km/s), as well as rotation of magnetic field components.
CME Shock Arrival Time: 2021-08-27T00:25Z
Observed Geomagnetic Storm Parameters due to CME:
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Predicted Arrival Time: 2021-08-26T20:13Z (-3.0h, +3.0h)
Confidence that the CME will arrive: 100.0%
Predicted geomagnetic storm max Kp range due to CME: 2.0 - 4.0
Prediction Method: Ensemble WSA-ENLIL + Cone (NASA M2M)
Prediction Method Note:
Based on analysis by the Moon to Mars Space Weather Office and heliospheric ensemble modeling carried out at the Community Coordinated Modeling Center, it is estimated that the CME may impact STEREO A. For 24 ensemble members (see notes section), simulations indicate that the leading edge of the CME will reach:

- STEREO A between about 2021-08-26T21:43Z and 2021-08-26T23:43Z (average arrival 2021-08-26T22:55Z) for 12% of simulations.

Additionally the CME is estimated to reach NASA missions near Earth between about 2021-08-26T17:07Z and 2021-08-26T23:03Z (average arrival 2021-08-26T20:13Z) for 100% of simulations.  The ensemble-based forecast indicates that there is a 95% chance for the maximum Kp index to be in the 2-4 range (below minor to below minor).

Links to the ensemble details of the modeled event:
https://iswa.gsfc.nasa.gov/ENSEMBLE/2021-08-23_ncmes1_sims24_HILOX087/20210823_063600_ncmes1_sims24_HILOX087_anim_tim-den.gif
https://iswa.gsfc.nasa.gov/ENSEMBLE/2021-08-23_ncmes1_sims24_HILOX087/20210823_063600_ncmes1_sims24_HILOX087_arrival_Earth.gif
https://iswa.gsfc.nasa.gov/ENSEMBLE/2021-08-23_ncmes1_sims24_HILOX087/20210823_063600_ncmes1_sims24_HILOX087_Earth_stack.gif
https://iswa.gsfc.nasa.gov/ENSEMBLE/2021-08-23_ncmes1_sims24_HILOX087/20210823_063600_ncmes1_sims24_HILOX087_probabilistic_Kp_forecast_wdist.gif
https://iswa.gsfc.nasa.gov/ENSEMBLE/2021-08-23_ncmes1_sims24_HILOX087/20210823_063600_ncmes1_sims24_HILOX087_arrival_STA.gif
https://iswa.gsfc.nasa.gov/ENSEMBLE/2021-08-23_ncmes1_sims24_HILOX087/20210823_063600_ncmes1_sims24_HILOX087_STA_stack.gif

## Notes:
Ensemble CME modeling at M2M is performed by building sets of initial CME parameters and carrying out separate simulations for each set. This approach allows a mapping of initial CME parameter uncertainties into a statistical characterization of CME arrival times and impact at locations of interest.

Description of links: For each location, the first link shows the WSA-ENLIL+Cone model animation for the median CME input parameters, the second link shows the probabilistic distribution of predicted arrival times histogram, and the third link shows a stack plot of the WSA-ENLIL+Cone modeled magnetic field, velocity, density, and temperature for all ensemble members. For missions near Earth, a histogram of the probabilistic Kp forecast is also provided.

For the full details of the modeled event, please go here:
https://iswa.gsfc.nasa.gov/ENSEMBLE/2021-08-23_ncmes1_sims24_HILOX087/Detailed_results_20210823_063600_ncmes1_sims24_HILOX087.txt
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Lead Time: 63.42 hour(s)
Difference: 4.20 hour(s)
Prediction submitted by Carina Alden (M2M Office) on 2021-08-24T09:00Z
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