Space Weather Forecast - Discussion
Issued: 2025 Aug 15 0030 UTC
Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center and processed by SpaceWeatherLive.com
Solar activity
24 h Summary
Solar activity has been at low levels with only C-class flares observed.
There are 13 regions on the disk with most being simple in magnetic
complexity. Region 4172 (N09W59, Dai/beta-gamma) continued to decay with
its magnetic field decreasing in complexity. Region 4178 (N09W90,
Dso/beta) looks to be decreasing in its complexity but due to the limb
effect, analysis has become difficult.
No Earth-directed CMEs were observed in available coronagraph imagery.
Forecast
Solar activity is likely to continue at low levels through 17 August.
Despite their decreasing activity, Regions 4172 & 4178 will help
maintain a slight chance (35%) for isolated M-class flares
(R1-2/Minor-Moderate radio blackouts) in the forecast through 15 Aug.
Chances decrease to 30% as the regions move beyond the western limb.
Energetic Particles
24 h Summary
Persistent high speed stream (HSS) influence from the large, positive
polarity CH in the southern hemisphere caused the greater than 2 MeV
electron flux to surpass - for the fifth day in a row - the 1,000
particle flux units (pfu) on both GOES satellites. The GOES-19 satellite
observed a peak of 3,820 pfu at 14/0500 UTC.
The greater than 10 MeV proton flux remained at background.
Forecast
Waning influences from the CH HSS will steadily decrease the flux of 2
MeV electrons, but concentrations at geostationary orbit will remain
high most likely through 17 Aug. Last rotation, electrons remained
significantly above the 1,000 pfu threshold for seven days with diurnal
maximas above threshold for 11 days.
The greater than 10 MeV proton flux is expected to remain at background
levels through 17 August. There remains a very slight chance (5%) for
radiation storming levels to reach the S1 threshold based on the
potential for significant flaring from Regions 4172 and/or 4178 as they
approach the western limb.
Solar Wind
24 h Summary
Solar wind parameters, as measured at Lagrange point 1 (L1) by the ACE
spacecraft, reflected a continued, but weakening positive polarity CH
HSS regime. Total field (Bt) remained around 5 nT with the north-south
(Bz) component oscillating between +/-5 nT. Solar wind speeds gradually
declined from about 500 km/s to around 450 km/s. Phi was predominantly
in the positive (away from the Sun) solar sector with a few excursions
into negative orientation.
Forecast
Waning influences from the CH HSS are expected through 16 August. Solar
wind analyses project wind speeds to be down towards 370 km/s by the
close of 16 August indicating a more nominal wind speed environment
thereafter.
Geospace
24 h Summary
The geomagnetic field has been at quiet to unsettled levels.
Forecast
As CH HSS influences wane, mostly quiet to unsettled conditions are
expected to persist through 17 Aug. There remains a slight chance for an
isolated period of active conditions on 15 Aug.
-Bri