Routine Space Environment Product (Daily)
Issued by NWS

Home |  Current Version |  Previous Version |  Text Only |  Print | Product List |  Glossary On
Versions: 1 2 3 4 5 6 7 8 9 10 11 12 13 14
466
FXXX12 KWNP 071231
DAYDIS

:Product: Forecast Discussion
:Issued: 2026 Jul 07 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 returned to low levels, with only low-level C-class
flaring observed. This flaring consisted primarily of occulted events
from beyond the west limb, alongside occasional flares from Region 4482
(S09E49, Eki/beta-gamma). The largest event of the period was a C3.8
flare on the northwest limb, likely from old Region 4479 (N17, L=90).

There are currently three numbered regions on the visible disk. Region
4482 showed the most significant development with new spot growth in its
intermediate sections, consolidation within its leading group, and an
overall expansion in spatial extent and complexity. Region 4481 (N14E14,
Bxo/beta) consists of unremarkable pores that showed minor new emergence
following a period of decay. Region 4485 (N11W07, Bxo/beta) is showing
some new flux emergence as well and is characterized by spots appearing
and disappearing quickly.

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

.Forecast...
Solar activity is likely to remain at low to moderate levels through 09
July. The probability of M-class (R1-R2/Minor-Moderate) or greater
flaring drops on 08 Jul as old Regions 4478 (S05, L=83) and 4479
continue their transit beyond the western limb.

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels, with a peak flux of 2,940 pfu observed at 07/1130 UTC. The
greater than 10 MeV proton flux at geosynchronous orbit remained at
background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to remain at moderate
to high levels 07-09 July. A slight chance for an S1 (Minor) or greater
solar radiation storm remains for 07 July as old region 4478 is
presently in a highly geoeffective position just beyond the west limb.


Solar Wind

.24 hr Summary...
Solar wind parameters continued trending back toward nominal levels.
Solar wind speeds held steady through most of the period, averaging near
425 km/s, outside of a distinct and temporary enhancement observed
around 06/1700 UTC that drove speeds to a peak of nearly 550 km/s. Total
magnetic field strength (Bt) remained stable between 5 and 7 nT. The
North-South (Bz) component was slightly variable, with early southward
deflections as far down as -5 nT before transitioning northward at
approximately 07/0000 UTC. The phi angle was predominantly in the
positive (away from the Sun) orientation.

.Forecast...
Slightly enhanced solar wind parameters are expected to continue a
gradual decline toward ambient background speeds through the remainder
of 07 July and early 08 July. Enhanced and disturbed conditions are
likely to return on 09 July, with initial enhancements arriving as early
as late on 08 July, due to the anticipated impact of a co-rotating
interaction region (CIR) ahead of a negative polarity coronal hole
high-speed stream (-CH HSS).

Geospace

.24 hr Summary...
Geomagnetic field activity was quiet.

.Forecast...
Geomagnetic conditions are expected to remain mostly quiet to unsettled
through 08 July. Conditions are anticipated to increase to unsettled and
active levels on 09 July under the onset of -CH HSS influences, with a
slight chance for isolated periods of G1 (Minor) storming possible.