Space Weather Forecast - Discussion
Issued: 2025 Apr 13 0030 UTC
Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center and processed by SpaceWeatherLive.com
Solar activity
24 h Summary
Solar activity was at high levels due to frequent low-level R1 (Minor)
events. Region 4055 (N04W64, Ekc/beta-gamma-delta) held a monopoly on
the flare activity, producing all six of the M-class flares, the largest
being an M2.7 flare at 12/1143 UTC. The region continued to grow in
size, spot count, and magnetic complexity. Regions 4058 (N13W65,
Dao/beta), 4060 (N09E34, Dso/beta), and 4061 (N17W04, Dso/beta) all
exhibited growth during the period, but all remained mostly inactive.
The remaining numbered active regions were mostly unchanged.
From approximately 12/1107-1117 UTC, dimming was observed in GOES-19
SUVI 195 imagery near N31W05. This is believed to be associated with an
approximately six degree long DSF as reported by a USAF solar
observatory. The corresponding CME was observed in LASCO C2 coronagraph
imagery at 12/1202 UTC, but had a northerly trajectory. Initial analysis
indicated a miss to the north of Earth, with no impacts expected at this
time. No Earth-directed CMEs were observed in available coronagraph
imagery.
Forecast
Solar activity has a high likelihood of seeing M-class (R1-R2,
Minor-Moderate) flares, with a slight chance for isolate R3 (Strong)
events, on 13-15 Apr, due primarily to the flare potential from Region
4055.
Energetic Particles
24 h Summary
The greater than 2 MeV electron flux at geostationary orbit was at high
levels, reaching 3,905pfu at 12/1630 UTC. The greater than 10 MeV proton
flux remained at background levels.
Forecast
The 2 MeV electron flux is expected to remain at moderate to high levels
through 15 Apr. There is a slight chance the greater than 10 MeV proton
flux could reach S1 (Minor) levels due to the flare potential of Region
4955.
Solar Wind
24 h Summary
Solar wind parameters remained enhanced as influence from the negative
polarity CH HSS continued. Total magnetic field strength was between
6-10 nT. The Bz component was mostly negative, but did fluctuate between
-9 and +5 nT. Solar wind speeds were predominantly between 400-500 km/s
through 12/2100 UTC when they began to push over the 500 km/s mark. Phi
angle was oriented in the negative sector.
Forecast
The solar wind environment is expected to continue under a negative
polarity CH HSS regime through 13-14 Apr. CH effects should begin to
taper off by late on 15 Apr.
Geospace
24 h Summary
The geomagnetic field reached G1 (Minor) storm levels due to continuing
CH HSS effects.
Forecast
The geomagnetic field is expected to reach active levels, with a chance
for G1 (Minor) storm levels, on 13 Apr due to influence from a negative
polarity CH HSS. Unsettled to active conditions are expected to continue
into 14 Apr, with a slight chance for isolated G1 (Minor) periods, as CH
effects wane. Conditions are then expected to return to quiet to
unsettled levels on 15 Apr as the CH HSS moves from its geoeffective
location.