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Prediction for CME (2026-03-22T16:23:00-CME-001)

CME Observed Time: 2026-03-22T16:23Z
DONKI Link: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/45244/-1
CME Note: This somewhat asymmetric bright CME is visible to the SE in STEREO A COR2 for a few frames before a usual overnight data gap and in SOHO LASCO C2/C3 and GOES CCOR-1. Its source is a significant filament eruption with associated brightening/dimming starting around 2026-03-22T15:30Z, followed by high rising post-eruptive arcades, as seen in GOES SUVI 304, 284, and 195 centered around S20E15, south of Active Region 14398, and seen as ejecta and opening of field lines seen in STEREO A EUV 195/403 on/close to the SE limb. It appears that there may be some SE deflection/directionality to it,. as it erupts and progresses outward in the GOES SUVI 284 field of view. There is a bright bulk front and a wider faint shock front seen in all three coronagraphs. | Arrival information: Increase in B_total from 3.88 nT to 7.21 nT increasing to a maximum of 10.19 nT. Solar wind speed increased from roughly 530 km/s to roughly 600 km/s. Minor increase in solar wind temperature and density were also observed. This signature is likely associated with the arrival of CME with ID 2026-03-22T16:23:00-CME-001 which was modeled to impact missions near Earth at 2026-03-25T08:55Z (+/- 7 hours).
CME Shock Arrival Time: 2026-03-25T05:53Z
Observed Geomagnetic Storm Parameters due to CME:
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Predicted Arrival Time: 2026-03-25T05:31Z (-3.767h, +4.867h)
Confidence that the CME will arrive: 19.0%
Predicted geomagnetic storm max Kp range due to CME: 3.0 - 5.0
Prediction Method: Ensemble WSA-ENLIL + Cone (NASA M2M)
Prediction Method Note:
Ensemble modeling estimates the spread/uncertainty in CME arrival time predictions using the WSA-ENLIL+Cone model due to uncertainties in CME input parameters.  This is achieved by measuring N CME input parameters, then performing an ensemble of N runs of WSA-ENLIL cone model.  This gives an ensemble of N CME arrival times and impact estimates.

NASA GSFC SWRC ENLIL settings:
ENLIL version: 2.7
Resolution: low2 (256x30x90)
Ambient settings: a3b1f
WSA version: 2.2
(Enlil 2.7 w/res:low2 ambient:a3b1f, WSA2.2)

Please enter a copy of the entire notification here:

## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME update (ensemble) (Missions Near Earth)
##
## Message Issue Date: 2026-03-23T11:11:33Z
## Message ID: 20260323-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:

BETA PRODUCT. ENSEMBLE PRODUCT IS STILL IN DEVELOPMENT MODE. PLEASE LET US KNOW IF YOU HAVE ANY SUGGESTIONS FOR MODIFICATIONS.  

Ensemble modeling update on CME with ID 2026-03-22T16:23:00-CME-001 (see previous notification 20260323-AL-001).

Based on heliospheric ensemble modeling carried out at the Moon to Mars Space Weather Analysis Office, it is estimated that the CME may impact NASA missions near Earth. Out of 26 ensemble members (see notes section), 5 (19%) indicate impact at NASA missions near Earth. Ensemble simulations indicate that the leading edge of the CME will reach NASA missions near Earth between about 2026-03-25T01:45Z and 2026-03-25T10:23Z (average arrival 2026-03-25T05:31Z). The ensemble-based forecast indicates that there is a 60% chance for the maximum Kp index to be in the 3-5 range (below minor to minor).

Links to the ensemble details of the modeled event:
https://iswa.gsfc.nasa.gov/ENSEMBLE/2026-03-22_ncmes1_sims26_M2M-SWAO077/20260322_162300_ncmes1_sims26_M2M-SWAO077_anim_tim-den.gif
https://iswa.gsfc.nasa.gov/ENSEMBLE/2026-03-22_ncmes1_sims26_M2M-SWAO077/20260322_162300_ncmes1_sims26_M2M-SWAO077_arrival_Earth.gif
https://iswa.gsfc.nasa.gov/ENSEMBLE/2026-03-22_ncmes1_sims26_M2M-SWAO077/20260322_162300_ncmes1_sims26_M2M-SWAO077_Earth_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/2026-03-22_ncmes1_sims26_M2M-SWAO077/Detailed_results_20260322_162300_ncmes1_sims26_M2M-SWAO077.txt
###



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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: 42.70 hour(s)
Difference: 0.37 hour(s)
Prediction submitted by Tony Iampietro (M2M SWAO) on 2026-03-23T11:11Z
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