• Weekly Highlights of Solar and Geomagnetic Activity, 26 September - 02

    From SWPC.Webmaster@noaa.gov@21:1/5 to All on Mon Oct 3 13:00:09 2022
    XPost: rec.radio.amateur.space, rec.radio.shortwave, rec.radio.info

    :Product: Weekly Highlights and Forecasts
    :Issued: 2022 Oct 03 0500 UTC
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    # Weekly Highlights and Forecasts
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    Highlights of Solar and Geomagnetic Activity
    26 September - 02 October 2022

    Solar activity ranged from low to high levels during the period. Low
    levels occured from 26-29 Sep with numerous C-class flares observed
    from Regions 3105 (S17, L=210, class/area Dki/490 on 22 Sep), 3107
    (S25, L=113, class/area Fai/240 on 24 Sep) and 3112 (N23, L=052,
    class/area Fki/750 on 02 Oct), the largest region on the disk. The
    largest of these flares was a long duration C5.5 from Region 3112.

    Activity increased to moderate levels with three M-class flares from
    Region 3112 including an M2.9 at 30/1622 UTC. No Earth-directed CMEs
    were detected with these flares. Activity levels further increased
    to high with an M5.8/1b flare observed at 01/2010 UTC from Region
    3110 (N16, L=158, class/area Dhi/320 on 25 Sep). Analysis and
    modelling of the subsequent CME indicated a possible Earth-directed
    component. In addition, a slow rise and fall C3.5 x-ray event, with
    an associated filament eruption, was detected from Region 3113 (N16,
    L=154, class/area Dao/100 on 01 Oct). Analysis and modelling of the
    subsequent CME indicated a possible Earth-directed component.

    High levels continued with M-class activity from Regions 3110 and
    3112, the largest of these was an M8.7/1n from Region 3110.
    Associated with this event was a Type IV, a Tenflare (190 sfu) and a
    possible Earth-directed CME. Late on 02 Oct, the largest event of
    the highlight period was observed from Region 3110, an X1.0 with an
    associated Type II (1157 km/s) and 420 sfu Tenflare. Also associated
    with this event was a CME that had not been analyzed as of this
    writing.

    The greater than 2 MeV electron flux at geosynchronous orbit was at
    high levels on 26 Sep with a peak flux of 2,640 pfu observed at
    26/1640 UTC. The greater than 10 MeV proton flux at geosynchronous
    orbit was slightly elevated to near 2 pfu on the 27th and near 1 pfu
    on 01 and 02 Oct due to major flare activity.

    Geomagnetic field activity ranged from quiet to major storm levels.
    Mostly quiet levels were observed on 26 Sep. By 27 Sep, levels
    increased to unsettled to major storm due to negative polarity CH
    HSS effects coupled with CME effects from 24 Sep. Mostly quiet
    levels were observed on 28-29 Sep. Unsettled to active levels were
    observed on 30 Sep due to positive polarity CH HSS effects. Quiet
    levels returned on 01 Oct through midday or so on 02 Oct. Later on
    02 Oct, unsettled to minor storm levels were observed due to
    positive polarity CH HSS effects.





    Forecast of Solar and Geomagnetic Activity
    03 October - 29 October 2022

    Solar activity is expected to be low with M-class flares likely and
    a chance for X-class from 03-14 Oct and again from 18-29 Oct due to
    current active regions on the visible disk and returning active
    regions. Low levels are expected during the interim dates from 15-17
    Oct.

    A chance for proton events at geosynchronous orbit are possible from
    03-14 Oct and again from 18-29 Oct due to current active regions on
    the visible disk and returning active regions. No proton events are
    expected during the interim dates from 15-17 Oct.

    The greater than 2 MeV electron flux at geosynchronous orbit is
    expected to be at mostly normal to moderate levels during the
    outlook period.

    Geomagnetic field activity is expected to be at minor to major storm
    levels on 03-05 Oct due to combined positive polarity CH HSS and CME
    effects. Unsettled levels are possible on 10 Oct, 15-16 Oct and
    20-21 Oct with active levels possible on 15-16 Oct, all due to
    recurrent CH HSS effects.

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