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        981 FXXX06 KWNP 030511 WEKHIL :Product: 7-day Space Weather Highlights :Issued: 2025 Nov 03 0428 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 # # 7-day Space Weather Highlights # Highlights of Solar and Geomagnetic Activity 27 October - 02 November 2025 Solar activity was at low levels on 27 Oct - 01 Nov. Solar activity reached moderate levels on 02 Nov due to a single M1.0 flare that occurred at 02/0026 UTC from a region beyond the East limb and became the largest flare of the week. All the active regions that crossed the visible solar disk this week presented a simple magnetic configuration (alpha or beta) and an unremarkable overall activity. Region 4267 (N04, L=60, class/area=Cso/120 on 28 Oct) was the most flaring region during the week, with three C-class flares: a C1.6 at 28/1626 UTC, a C4.7 at 01/1655 UTC and a C8.2 at 02/1246 UTC. Three Type-II radio bursts were observed on 29-31 Oct and were likely associated with far-sided activity: 29/0012 UTC (est. speed 1,357 km/s), 30/0424 UTC (est. 691 km/s) and 31/2013 UTC (est. 542 km/s). Multiple CMEs were observed in coronagraph imagery during the week, but they were mostly far-sided. The CME that erupted around 30/0645 UTC from a region near N21E32 presented a potential Earth-directed component, and its modeled propagation suggested a partial impact on Earth's magnetosphere arriving on 02 Nov. However, no clear CME influences were observed on the solar wind data near-Earth during the period. No proton events were observed at geosynchronous orbit. The greater than 2 MeV electron flux at geosynchronous orbit reached the 1,000 pfu threashold around 31/1200 UTC and remained at high levels until the end of the period. The maximum > 2MeV electron flux of 1,260 pfu was observed on 02/1650 UTC by the GOES-19 satellite. Geomagnetic field activity was quiet on 27 Oct and 01 Nov, and reached active levels on 28-31 Oct and 02 Nov. Five synoptic periods of minor storming (G1) levels were observed on 30-31 Oct due to the solar wind maximum disturbances caused by the high speed stream (HSS) associated to a positive coronal hole that dominated the geospace during the period.