Routine Space Environment Product (Daily)
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745
FXXX12 KWNP 061231
DAYDIS

:Product: Forecast Discussion
:Issued: 2026 Sep 06 1230 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# http://www.swpc.noaa.gov/wwire.html
#
#             Forecast Discussion
#
Solar Activity

.24 hr Summary...
Solar activity was at moderate levels following an M1.0/1f (R1-Minor)
flare at 05/1518 UTC from an area of plage (formerly Region 4520 (S12,
L=340)). Associated with this flare were 10 MeV (S1-Minor) and 100 MeV
proton events. A further description of these proton events are
highlighted below. Other flare activity consisted of C-class flares
observed from Region 4524 (N12E40, Cso/beta), the three largest being a
C6.4/1n at 05/1045 UTC, a C8.5/2n event at 05/1746 UTC and a C5.0/1n at
06/1042 UTC. This region continued to exhibit weak decay, while the
remaining existing regions on the disk were quiet and stable. Two new
regions were observed rotating onto the visible disk from the east limb
and were numbered as Region 4528 (S12E76, Hsx/alpha) and 4529 (N11E73,
Hsx/alpha). Both were stable and inactive during the period.

Several CMEs were observed this period. First, a filament just SE of
disk center started erupting around 05/0530 UTC and an associated
structure became visible in STEREO coronagraph imagery at 05/0638 UTC
and very faintly in LASCO C2 at roughly 05/0825 UTC. Second, a CME
associated with the C6.4 from Region 4524 at 05/1045 UTC first became
visible in LASCO C2 at roughly 05/1112 UTC and in STEREO coronagraph
imagery at 05/1108 UTC. Third, a CME associated with the M1.0 flare from
Plage Region 4520 first became visible in LASCO C2 imagery at 05/1536
UTC and in STEREO coronagraph imagery as a halo at 05/1608 UTC. Modeling
suggests that this eruption will pass ahead of Earths orbit. Lastly, a
CME associated with the C8.5 first became visible in LASCO C2 imagery at
05/1800 UTC and in STEREO coronagraph imagery at 05/1808 UTC. Modeling
suggests a possible combined arrival for these eruptions on early 08
Sep.

.Forecast...
Solar activity will likely be at low levels due to occasional C-class
flare activity, with a slight chance for M-class flares
(R1-R2/Minor-Moderate) through 08 Sep.

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux was at normal to moderate levels.
The greater than 10 MeV (S1-Minor) proton flux began rising at 05/1530
UTC and exceeded the 10 pfu event level at 05/1615 UTC with a peak
flux of 17.8 pfu observed at 05/1645 UTC. Levels remained elevated
but continued to diminish at the end of the reporting period.

The greater than 100 MeV proton flux began rising at 05/1530 UTC and
also exceeded the 1 pfu event threshold at 05/1545 UTC, reaching a max
of 1.16 pfu at 05/1550 UTC. Levels decayed below the 1 pfu levels at
05/1615 UTC and ended the period near background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to be at normal to
moderate levels on 06-08 Sep. The greater than 10 MeV proton flux is
expected to continue decreasing towards background levels through early
08 Sep. Levels could increase back up to equal or exceed threshold
levels by midday on 08 Sep if the anticipated CMEs impact Earth.

Solar Wind

.24 hr Summary...
Solar wind parameters were at nominal levels. Total field averaged near
6 nT, Bz fluctuated between +/-5 nT, and solar wind speeds averaged
around 350 km/s. Phi was predominantly negative with isolated
oscillations into a positive orientation.

.Forecast...
Solar wind conditions are expected to remain near background levels
through 06 Sep. Enhancements due to a solar sector boundary crossing
(SSBC) are anticipated by late on 06 Sep to early 07 Sep. Further
enhancements are possible on 08 Sep with the anticipated arrival of the
multitude of CMEs from the past couple of days combined with the onset
of the CH HSS.

Geospace

.24 hr Summary...
The geomagnetic field was quiet.

.Forecast...
Mostly quiet levels are expected to prevail through 06 Sep. Isolated
unsettled conditions are likely by late on 06 Sep with unsettled to
periodic active levels on 07 Sep due to aforementioned SSBC effects.
Unsettled to active levels are then expected on 08 Sep, with isolated G1
(Minor) periods likely if the CMEs mentioned above impact Earth as
forecast. Confidence is low on the timing and magnitude of the CME
arrivals.