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Subject: [Propagation+Space Weather] Today's Space Weather Forecast Discussion on 2023 Jan 25 1230 UTC
From: nw7us@sunspotwatch.com
Reply-to: Practical radio-wave propagation and space weather <propagation@contesting.com>
Date: Wed, 25 Jan 2023 20:07:08 +0000
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Here is the current forecast discussion on space weather and geophysical activity, issued 2023 Jan 25 1230 UTC.

Solar Activity

24 hr Summary: Solar activity reached moderate levels with a long duration M4.6 flare peaking at 25/1011 UTC. The source region appears to be 3190 (S14W85, Dkc/beta-gamma). No significant radio reports accompanied this flare. Updated coronagraph imagery is needed for any CME analysis for this event.

A long duration C9/Sf flare was observed at 24/1435 UTC, likely associated with the eruption of an approximately 14° long filament centered near N29W58. Analysis indicated that the bulk of the material was ejected well north of the Sun-Earth line, with no impacts expected at Earth. Another C9 flare was observed at 25/0453 UTC from Region 3192 (N16W76, Cao/beta). Additional low-level C-class flares were also observed during the period from a variety of different regions.

Region 3190 remained the most magnetically complex region, but did show signs of decay as it approached the western limb. Regions, 3196 (N15W40, Cso/beta), 3197 (N20W30, Dao/beta) and 3199 (N16W01, Cao/beta) all had minor growth, but were mostly inactive. Regions 3198 (N26W16, Cso/beta) and 3200 (N23E29, Cao/beta) remained quiescent. New spot group 3201 (N25E52, Hsx/alpha) was numbered, but was unremarkable during the period.

No Earth-directed CMEs were observed in available imagery.

Forecast: Solar activity is expected to be low, with a chance for M-class flares (R1-R2 Minor-Moderate) and slight chance for an isolated X-class flare (R3-Strong) on 25-26 Jan as Region 3190 remains magnetically complex. Probabilities drop slightly by 27 Jan as more of these two regions exit the solar disk.

Energetic Particles

24 hr Summary: The greater than 2 MeV electron flux was normal to moderate and the greater than 10 MeV proton flux remained at background levels.

Forecast: The greater than 2 MeV electron flux is expected to continue at normal to moderate levels on 25 Jan, with a likely increase to moderate to high levels late on 25/early 26 Jan due to CH HSS influence. There is a slight chance for a greater than 10 MeV proton event all three days.

Solar Wind

24 hr Summary: Solar wind parameters reflected a return to mostly background conditions. Total field averaged near 5 nT for most of the period, while the Bz component was variable between +/- 5 nT. Solar wind speeds were mostly between 400-450 km/s. Phi was positive.

Forecast: The solar wind environment is expected to see enhancements on 25-26 Jan due to positive polarity CH HSS influence, and any weak peripheral transient effects. Conditions should begin to weaken by 27 Jan as CH/CME effects dissipate.

Geospace

24 hr Summary: The geomagnetic field was at quiet levels.

Forecast: The geomagnetic field is expected to be at unsettled to isolated active levels, with a chance for an isolated G1 period over 25-26 Jan, in response to positive polarity CH HSS effects combined with possible CME influence. By 27 Jan, conditions should begin to return to more nominal levels.

Don't forget to visit our live space weather and radio propagation web site, at: http://SunSpotWatch.com/

Live Aurora mapping is at http://aurora.sunspotwatch.com/

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Today's Space Weather Forecast Discussion - 2023 Jan 25 20:07 UTC

Live data: SunSpotWatch.com

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