:Product: Weekly Highlights and Forecasts
:Issued: 2025 Sep 15 0137 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
# Product description and SWPC contact on the Web
# https://www.swpc.noaa.gov/content/subscription-services
#
#                Weekly Highlights and Forecasts
#
Highlights of Solar and Geomagnetic Activity
08 - 14 September 2025

Solar activity was at low levels with only C-Class flares observed.
The largest flare of the period was a C7.6 from Region 4207 (N28,
L=48, class/area=Cso/80 on 11 Sep) at 11/1521 UTC. No significant
CME activity was observed. 

No proton events were observed at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels on 09, 13, and 14 Sep due to influences from multiple
coronal hole high speed streams (CH HSS). Normal to moderate levels
were observed on 08, 10, 11, and 12 Sep. 

Geomagnetic field activity reached G2 (Moderate) storm levels on 09
Sep due to sustained period of southward Bz. G1 (Minor) storm levels
were observed on 14 Sep due to influences from a negative polarity
CH HSS. Quiet to active levels were observed on the remaining days
of the highlight period. 

Forecast of Solar and Geomagnetic Activity
15 September - 11 October 2025

Solar activity is expected to be at low levels with a chance for
isolated M-class flares throughout the outlook period. 

No proton events are expected at geosynchronous orbit.

The greater than 2 MeV electron flux at geosynchronous orbit is
expected to reach high levels on 18-21 Sep and 06-11 Oct due to
recurrent CH HSS influences. Normal to moderate levels are expected
for the remainder of the outlook period. 

Geomagnetic field activity is expected to be at G2 (Moderate) storm
levels on 15 Sep due to influences from negative polarity CH HSS.
Active to G1 (Minor) storm levels are expected on 16 Sep, 28-29 Sep,
03-07 Oct, and 11 Oct all due to recurrent CH HSS influences. Quiet
to unsettled levels are expected for the remaining days in the
outlook period.