CME ScoreBoard Header

CCMC CME Scoreboard

CME Scoreboard: Prediction Detail

Prediction for CME (2026-03-25T00:45:00-CME-001)

CME Observed Time: 2026-03-25T00:45Z
DONKI Link: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/45291/-1
CME Note: CME visible to the southwest in GOES CCOR-1 and in limited available SOHO LASCO C3 imagery in real-time during a data downlink period. Not visible in STEREO A COR2 imagery due to a data gap starting at 2026-03-24T13:53Z. The source is a C2.9 flare and associated eruption from AR 14400 (approximately S14W52) starting at 2026-03-24T23:52Z as seen in GOES SUVI 195/284 with rapidly opening field lines and possible EUV wave.
CME was not detected at Earth.
Observed Geomagnetic Storm Parameters due to CME:
----

Predicted Arrival Time: 2026-03-27T01:00Z (-12.0h, +12.0h)
Confidence that the CME will arrive: 20.0%
Predicted geomagnetic storm max Kp range due to CME: 3.0 - 5.0
Prediction Method: Other (SIDC)
Prediction Method Note:
CME start time: 2026-03-25T00:12:00Z

#--------------------------------------------------------------------#
# DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC     #
# (RWC Belgium)                                                      #
#--------------------------------------------------------------------#
SIDC URSIGRAM 60325
SIDC SOLAR BULLETIN 25 Mar 2026, 1245UT
SIDC FORECAST
SOLAR FLARES  : C-class flares expected, (probability >=50%)
GEOMAGNETISM  : Active conditions expected (A>=20 or K=4)
SOLAR PROTONS : Quiet
PREDICTIONS FOR 25 Mar 2026  10CM FLUX: 128 / AP: 008
PREDICTIONS FOR 26 Mar 2026  10CM FLUX: 130 / AP: 021
PREDICTIONS FOR 27 Mar 2026  10CM FLUX: 135 / AP: 014

Solar Active Regions and flaring: Solar flaring activity was low over the
past 24 hours, with six C-class flares identified. SIDC Sunspot Group (SG)
832 (NOAA Active Region [AR] 4403) produced the brightest flare, a C7 (SIDC
Flare 7253) on 24 March at 17:54 UTC. SIDC SG 830 (NOAA AR 4401, Beta-Gamma
magnetic configuration) and SIDC SG 826 (NOAA AR 4400, Beta magnetic
configuration) also produced X-ray flares.
More C-class flaring activity is expected in the next 24 hours.

Coronal mass ejections: A CME seen in LASCO-C2 images as launched on 25 Mar
at 00:12 UTC is associated with SIDC SG 826 (NOAA AR 4400) and is expected
to deliver a glancing blow on Earth the first half of 27 Mar.

Solar wind: During the past 24 hours, the Solar Wind (SW) conditions were
affected a glancing blow, on 25 Mar at 05:55 UTC, from a Coronal Mass
Ejection (CME). This is the predicted arrival of the the CME launched on 22
Mar at 16:00 UTC and was associated with a filament eruption.
As results of the effect, the SW speed increased from 500 to 630 km/s, the
interplanetary magnetic field (B) increased to 10 nT, and its North-South
component (Bz) varied from -8 nT to 8 nT.
Another glancing blow, associated with SIDC CME 642 is expected to arrive
in the next 24 hours and have a similar effect.

BT

#--------------------------------------------------------------------#
# Solar Influences Data analysis Center - RWC Belgium                #
# Royal Observatory of Belgium                                       #



Expected arrival time: 2026-03-27T01:00:00Z

Arrival time uncertainty: 12


Estimated peak K: 4

Peak K uncertainty: 1


Probability of arrival: 20


CME start time: 2026-03-25T00:12:00Z
Lead Time: 14.28 hour(s)
Difference: -----
Prediction submitted by Elizabeth Juelfs (LASSOS) on 2026-03-26T10:43Z
CME Scoreboard Footer

CCMC Rules of the Road: CCMC requests that users notify the CCMC, CME model/technique developers and submitting forecasters/researchers before performing event and validation studies with data from the CME Arrival Time Scoreboard. It is recommended that such studies be performed with the knowledge and collaboration of developers and submitting forecasters/researchers.

If you are looking for the official U.S. Government forecast for space weather, please go to NOAA's Space Weather Prediction Center (https://swpc.noaa.gov). This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy