075
FXXX12 KWNP 061231
DAYDIS

:Product: Forecast Discussion
:Issued: 2026 May 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
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#             Forecast Discussion
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Solar Activity

.24 hr Summary...
Solar activity was at low levels during the reporting period. Occasional
low-level C-class flaring was observed from Region 4425 (N06W82,
Hsx/alpha), with isolated flaring noted from the remaining regions.

There are currently six numbered regions on the visible disk. Most
regions showed various stages of decay and consolidation. Region 4429
(S05W40, Cso/beta) exhibited minor decay, particularly in the trailing
spots. Region 4431 (S16W08, Eso/beta) showed notable submergence,
particularly within its trailing spots which lost all penumbra as the
region simplifies toward a unipolar state. Region 4432 (N13E05,
Cso/beta) experienced minor decay in its intermediary spots following a
recent growth phase. Region 4433 (S16E36, Dso/beta) showed consolidation
within its leading spot group alongside decay and a near-total loss of
penumbra in its trailing spots. All other regions were stable.

No Earth-directed CMEs were observed in available coronagraph imagery.

.Forecast...
Solar activity is expected to be at low levels through 08 May, with a
chance for isolated M-class flares (R1-R2/Minor-Moderate), primarily due
to Region 4429 and an active region (likely old Region 4419) near L=330
(seen in Solar Orbiter imagery and expected to rotate into view on 08
May).


Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux at geosynchronous orbit was at low
to moderate levels, with a peak flux of 337 pfu observed at 05/1520 UTC.
The greater than 10 MeV proton flux remained at background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to remain at low to
moderate levels on 0607 May with the transition back toward a slow
solar wind regime. An increase to high levels is expected by 08 May due
to the anticipated onset of a positive polarity coronal hole high-speed
stream (+CH HSS). The greater than 10 MeV proton flux is expected to
remain at background levels through 08 May.

Solar Wind

.24 hr Summary...
Solar wind parameters reflected the continued passage of a slow-moving
CME that initially arrived at approximately 04/1200 UTC. Total magnetic
field (Bt) was sustained near 1011 nT early in the period, then
decreased to 5 nT, while the North-South component (Bz) initially ranged
-7 nT and -10 nT. A gradual rotation was observed early in the period,
with Bz recovering toward near-zero and turning northward by 05/0600
UTC. Bz briefly strengthened to 10 nT around 05/1400 UTC. Solar wind
speed steadily declined throughout the day, decreasing from
approximately 450 km/s to 350 km/s. The phi angle switched from a
negative to positive orientation at ~06/0500 UTC.


.Forecast...
Solar wind parameters are expected to continue declining toward nominal
background levels on 06 May. Minor enhancements are possible due to
potential glancing influences from a CME that departed the Sun on 30
April, though confidence in this impact is low. On 07 May, a solar
sector boundary crossing is anticipated, followed by the onset of a +CH
HSS that is expected to persist through 08 May.

Geospace

.24 hr Summary...
The geomagnetic field started the reporting period at G1 (Minor)
storming levels. Following the storming, the field experienced a single
unsettled period before returning to quiet levels for the remainder of
the period.


.Forecast...
The geomagnetic field is anticipated to be at mostly quiet to unsettled
levels on 06 May as CME influences wane, though isolated active periods
remain possible due to the low-confidence 30 April CME. Active
conditions are likely on 07 and 08 May following the onset of the +CH
HSS, with isolated G1 (Minor) storming periods possible.