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:Product: Forecast Discussion :Issued: 2026 Sep 15 1230 UTC # Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center # Solar Activity .24 hr Summary... Solar activity continued at very low levels with occasional B-class flaring. There are four numbered sunspot regions on the visible disk. All but Region 4531 (S08W02, Bxo/beta), which was numbered this period, are stable unipolar groups. No Earth-directed CMEs were observed in available coronagraph imagery. .Forecast... Solar activity is expected to remain at very low levels, with a decreasing chance for isolated C-class flares and a slight chance for M-class flares through 17 Sep. Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux was at high to moderate levels, with a peak flux of 4,650 pfu observed at 14/1315 UTC. The greater than 10 MeV proton flux has declined but remains slightly elevated following a peak of 4 pfu observed at 14/1520 UTC. .Forecast... The greater than 2 MeV electron flux is expected to continue at high levels through 17 Sep. The greater than 10 MeV proton flux is anticipated to undergo a slow decline toward background levels through 17 Sep. Solar Wind .24 hr Summary... Solar wind parameters were slightly enhanced throughout the period, consistent with transient passage and the likely onset of a negative polarity coronal hole high-speed stream (-CH HSS). Total field strength (Bt) gradually rose to a peak of 14 nT after 14/1800 UTC before reaching as high as 16 nT late in the period. The North-South (Bz) component was variable in the first half of the period and reached a maximum southward deflection of -9 nT before turning and remaining northward after 14/2230 UTC. Solar wind speeds held relatively slow between 350 and 380 km/s before climbing sharply after 15/1114 UTC to over 600 km/s. This wind speed increase was a notable sharp rise in temperature. The phi angle shifted into a predominantly negative (towards the Sun) early in the period. .Forecast... Negative polarity CH HSS effects are anticipated to persist through 17 Sep. Additional enhancements are likely on 16 and 17 Sep due to flanking influences from CMEs that departed the Sun on 13 and 14 Sep. Geospace .24 hr Summary... The geomagnetic field was at quiet to active levels in response to transient influences. .Forecast... Geomagnetic activity is expected to reach active to G1 (Minor) storm levels on 15 and 16 Sep, with G1 conditions remaining possible on 17 Sep due to combined CH and CME effects.

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:Product: Forecast Discussion :Issued: 2026 Sep 15 0030 UTC # Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center # Solar Activity .24 hr Summary... Solar activity was at very low levels during the period with only B-class flares observed. There are currently four numbered regions on the visible disk with none exhibiting magnetic complexity. A CME that was most likely associated with dimming near Region 4528 (S11W44, Hsx/alpha) was observed off the W Limb. Modeling results indicated a possible glancing arrival on 17 Sep. .Forecast... Solar activity is expected to be at very low levels, with a chance for isolated C-class flares and a slight chance for M-class flares through 17 Sep. Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux reached high levels with a maximum flux of 1,827 pfu observed at 13/1800 UTC. The greater than 10 MeV proton flux was at background levels until approximately 14/0430 UTC when it began to rise, eventually reaching a peak of 4 pfu near 14/1500 UTC. .Forecast... The greater than 2 MeV electron flux is expected to reach high levels on 15 Sep before returning to moderate levels on 16-17 Sep. The greater than 10 MeV proton flux is expected to see a slow decline to background levels through 17 Sep. However, a slight chance (20%) for a rise above the 10 pfu threshold is possible due to its elevated state. Solar Wind .24 hr Summary... Solar wind parameters were enhanced and are possibly a reflection of the filament that departed the Sun on 09 Sep combined with the anticipated SSBC. Total field strength slowly increased to a peak of 14 nT after 14/1800 UTC. The Bz component was variable and briefly deflected southward to a maximum of -8 nT near 14/1435 UTC. Solar wind speeds remained below 400 km/s. The phi angle was variable throughout the period. .Forecast... Negative polarity CH HSS effects are anticipated to continue through 17 Sep. CMEs from the 13 and 14 Sep are likely to have flanking influences on 16 and 17 Sep. Geospace .24 hr Summary... The geomagnetic field reached active levels during a period of southward Bz. .Forecast... The geomagnetic field likely to reach active to G1 (Minor) storm levels on 15 and 16 Sep, with a chance for G1 conditions on 17 Sep. All due to combined CH and CME influences.
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Space Weather Message Code: ALTK04 Serial Number: 2683 Issue Time: 2026 Sep 14 1802 UTC ALERT: Geomagnetic K-index of 4 Threshold Reached: 2026 Sep 14 1743 UTC Synoptic Period: 1500-1800 Active Warning: YES Comment: NOAA Space Weather Scale descriptions can be found at www.swpc.noaa.gov/noaa-scales-explanation Potential Impacts: Area of impact primarily poleward of 65 degrees Geomagnetic Latitude. Induced Currents - Weak power grid fluctuations can occur. Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
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Space Weather Message Code: WARK04 Serial Number: 5416 Issue Time: 2026 Sep 14 1654 UTC WARNING: Geomagnetic K-index of 4 expected Valid From: 2026 Sep 14 1653 UTC Valid To: 2026 Sep 14 2349 UTC Warning Conditions: Onset Comment: NOAA Space Weather Scale descriptions can be found at www.swpc.noaa.gov/noaa-scales-explanation Potential Impacts: Area of impact primarily poleward of 65 degrees Geomagnetic Latitude. Induced Currents - Weak power grid fluctuations can occur. Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
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Space Weather Message Code: WATA20 Serial Number: 1124 Issue Time: 2026 Sep 14 1547 UTC WATCH: Geomagnetic Storm Category G1 Predicted Highest Storm Level Predicted by Day: Sep 15: G1 (Minor) Sep 16: G1 (Minor) Sep 17: None (Below G1) THIS SUPERSEDES ANY/ALL PRIOR WATCHES IN EFFECT Comment: NOAA Space Weather Scale descriptions can be found at www.swpc.noaa.gov/noaa-scales-explanation Potential Impacts: Area of impact primarily poleward of 60 degrees Geomagnetic Latitude. Induced Currents - Weak power grid fluctuations can occur. Spacecraft - Minor impact on satellite operations possible. Aurora - Aurora may be visible at high latitudes, i.e., northern tier of the U.S. such as northern Michigan and Maine.
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