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Prediction for CME (2026-03-30T03:24:00-CME-001)CME Observed Time: 2026-03-30T03:24ZDONKI Link: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/45395/-1 CME Note: Large partial-halo CME visible to the SE in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery. The source is an X1.4 flare from Active Region 14405 (S27E45) peaking at 2026-03-30T03:19Z. The source is associated with brightening, dimming, moving/opening field lines, and EUV wave as seen in GOES SUVI 195, 304, 284, 131, 094, and 171 starting around 2026-03-30T02:56Z. CME Shock Arrival Time: 2026-04-01T11:29Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2026-03-31T12:00Z (-12.0h, +12.0h) Confidence that the CME will arrive: 85.0% Predicted geomagnetic storm max Kp range due to CME: 6.0 - 8.0 Prediction Method: SIDC Prediction Method Note: #--------------------------------------------------------------------#
# HALO CME ALERTS from the SIDC (RWC-Belgium), generated by CACTUS #
#--------------------------------------------------------------------#
A halo or partial-halo CME was detected with the following characteristics:
t0 | dt0| pa | da | v | dv | minv| maxv|
2026-03-30T03:24:22.828 | 5.0 | 132 | 150 | 1024 | 318 | 385 | 1562
t0: onset time, earliest indication of liftoff
dt0: duration of liftoff (hours)
pa: principal angle, counterclockwise from North (degrees)
da: angular width of the CME (degrees),
v: median velocity (km/s)
dv: variation (1 sigma) of velocity over the width of the CME
mindv: lowest velocity detected within the CME
maxdv: highest velocity detected within the CME
#--------------------------------------------------------------------#
# Solar Influences Data analysis Center - RWC Belgium #
# Royal Observatory of Belgium #
#--------------------------------------------------------------------#
# DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC #
# (RWC Belgium) #
#--------------------------------------------------------------------#
SIDC URSIGRAM 60330
SIDC SOLAR BULLETIN 30 Mar 2026, 1248UT
SIDC FORECAST
SOLAR FLARES : M-class flares expected (probability >=50%)
GEOMAGNETISM : Major (ISES: Severe) magstorm expected (A>=100 or K>=7)
SOLAR PROTONS : Warning condition (activity levels expected to increase, but no numeric forecast given)
PREDICTIONS FOR 30 Mar 2026 10CM FLUX: 160 / AP: 007
PREDICTIONS FOR 31 Mar 2026 10CM FLUX: 160 / AP: 007
PREDICTIONS FOR 01 Apr 2026 10CM FLUX: 160 / AP: 007
Coronal mass ejections: A coronal mass ejection (SIDC CME 644) was detected
in SOHO/LASCO-C2 on 30 March at 03:24 UTC. Automated CACTus detection
reports a full halo CME (width 360 degrees) with a principal angle of 132
degrees and a projected speed of 1024 km/s. This CME is associated with the
X1.4 flare (SIDC Flare 7290), which peaked at 03:19 UTC from SIDC Sunspot
Group 836 (NOAA Active Region 4405). This event was also accompanied by a
Type II radio emission, indicating the presence of a shock wave propagating
through the solar corona, with an estimated velocity of 1872 km/s. Initial
3D analysis suggests a propagation direction towards (S15E30) with an
angular width of approximately 45 degrees and a speed of about 1835 km/s.
The source region is consistent with the flare location at approximately
(S27E42). Given its source location and propagation direction, this CME is
expected to impact Earth in about 25-35 hours.
Lead Time: 38.75 hour(s)Difference: 23.48 hour(s) Prediction submitted by Melissa Kane (M2M SWAO) on 2026-03-30T20:44Z |
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