Routine Space Environment Product (Daily)
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775
FXXX12 KWNP 300031
DAYDIS

:Product: Forecast Discussion
:Issued: 2026 Oct 30 0030 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 continued at very low levels. Region 4563 (S18W81,
Axx/alpha) decayed as rotates off the west solar limb. A new active
region rotated into the visible disk and was numbered during the period:
Region 4564 (N05E68, Axx/alpha).

A filament eruption at the SW quadrant was first observed by GOES/SUVI
304A around 29/0830 UTC, and later was visible in LASCO/C2 imagery after
29/1036 UTC. Preliminary analysis indicated a slow Earth-directed
component but further modeling suggested its trajectory is missing
Earth.

No Earth-directed CMEs were observed at the available coronagraph
imagery.

.Forecast...
Solar activity is expected to be at very low levels with a slight chance
for isolated C-class flares through 31 Oct.

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux reached high levels, with a peak
flux of 1,228 pfu observed at 29/1630 UTC. The greater than 10 MeV
proton flux remained steady at background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to decrease to normal
to moderate levels on 30 Oct Oct and remaining there through 01 Nov. The
greater than 10 MeV proton flux is anticipated to persist at background
levels through 01 Nov.

Solar Wind

.24 hr Summary...
Solar wind parameters reflected undisturbed conditions near Earth, with
the speeds decreasing from 375 km/s to 325 km/s levels during the
period. Total magnetic field (Bt) remained below 5 nT in the past 24h
with a Bz (north-south) component mostly near neutral or northward. A
sharp decrease of density at 29/1624 UTC was due to a data processing
isolated correction, and does not reflect any solar wind physical
transient. The phi angle was largely negative (towards the Sun).

.Forecast...
Solar wind disturbances are likely to occur late on 30 Oct, continuing
into 31 Oct - 01 Nov, due to a recurrent, equatorial positive polarity
CH HSS that is anticipated to become geoeffective.

Geospace

.24 hr Summary...
The geomagnetic field was quiet during the period.

.Forecast...
Unsettled to active geomagnetic levels are expected by late on 30 Oct as
the positive polarity CH HSS effects begin, with G1 (Minor) geomagnetic
storming becoming likely on 31 Oct and 01 Nov.