• Weekly Highlights of Solar and Geomagnetic Activity, 24 - 30 March 2025

    From SWPC.Webmaster@noaa.gov@3:633/280.2 to All on Tue Apr 1 04:00:06 2025
    Subject: Weekly Highlights of Solar and Geomagnetic Activity, 24 - 30 March 2025

    :Product: Weekly Highlights and Forecasts
    :Issued: 2025 Mar 31 0224 UTC
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    # Weekly Highlights and Forecasts
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    Highlights of Solar and Geomagnetic Activity
    24 - 30 March 2025

    Solar activity was low on 24-25 Mar, moderate on 26-27 Mar and 29
    Mar, and high on 28 Mar and 30 Mar. High levels were reached on 28
    Mar as the strongest event of the period, an X1.1 (R3-Strong) flare
    at 28/1521 UTC from yet-to-be-numbered Region 4046 (N05, L=301, class/area=Dho/270 on 30 Mar), was produced on the Sun's eastern
    limb. Associated with the event was a Type IV radio sweep and a
    Tenflare (380 sfu). The resulting fast-moving CME was analyzed and
    modelled. The results suggested the far flank of the CME would pass
    close, but ultimately miss Earth. High solar activity levels were
    again reached on 30 Mar due to frequent R1 flares from Region 4048
    (S15, L=281, class/area=Eki/300 on 30 Mar). A total of six events
    were observed, the largest of which was an M1.6 (R1) flare at
    30/1642 UTC.

    Other activity included Type II radio sweeps on 25 Mar and 26 Mar.
    Both of these events were associated with non-Earth-directed CME
    events on or beyond the W. limb.

    No proton events were observed at geosynchronous orbit. However, an
    increase above background was observed two days after the X1.1 flare
    at 28/1521 UTC from the Sun's eastern limb. Although delayed,
    the rise in proton flux is likely related to this event.

    The greater than 2 MeV electron flux at geosynchronous orbit climbed
    to high levels on 27-30 Mar. This increase in electron flux was
    caused by the influence of a strong, positive polarity CH HSS, which
    began around 26 Mar.

    Geomagnetic field activity ranged from quiet to G2 (Moderate)
    geomagnetic storms. Active conditions on 24 Mar were associated with
    the passage of a CME that left the Sun on 21 Mar. On 25 Mar active
    conditions were again observed due to the onset of CIR ahead of a
    positive polarity CH HSS. Geomagnetic activity increased to G2
    (Moderate) levels on 26 Mar as total magnetic field strength reached
    a brief peak of 29 nT and the Bz component reached as far south as
    -27 nT. Wind speeds increased from above ~600 km/s on 26 Mar to
    above ~800 km/s on 27 Mar. The geomagnetic field responded with a
    mix of active to G1 (Minor) storm conditions. As total magnetic
    field strength and solar wind speeds declined on 28 Mar, geomagnetic
    conditions decreased to mostly unsettled to active levels. During
    the final waning stage of the positive polarity CH, an isolated
    period of active was last observed early on 29 Mar and only quiet
    conditions were observed over 30 Mar.

    Forecast of Solar and Geomagnetic Activity
    31 March - 26 April 2025

    Solar activity will continue at a chance for R1-R2 (Minor-Moderate)
    throughout the outlook period due to multiple complex regions on the
    visible disk as well as on the Sun's farside that are likely to
    return. A slight chance exists for R3 (Strong) events over the next
    three days primarily due to the flare potential from complex regions
    in the Sun's eastern hemisphere.

    No proton events are expected at geosynchronous orbit are likely to
    remain below the S1 (Minor) solar radiation storm threshold (>10
    MeV proton flux of 10 pfu).

    The greater than 2 MeV electron flux at geosynchronous orbit is
    expected to be at high levels on 31 Mar, 06-14 Apr, and 23-26 Apr in
    response to multiple, recurrent, CH HSSs. The remainder of the
    outlook period is expected to be at normal to moderate levels.

    Geomagnetic field activity is expected to range from quiet to G2
    (Moderate) geomagnetic storm conditions. G2 conditions are likely on
    05 Apr and 09 Apr; G1 (Minor) conditions are likely over 04 Apr, 08
    Apr, and 10 Apr, active conditions are likely over 11 Apr, 13 Apr,
    and 21-24 Apr; unsettled conditions are likely on 03 Apr, 06-07 Apr,
    12 Apr, 14-15 Apr, 17-20 Apr, and 25-26 Apr. All increases in
    geomagnetic activity are anticipated in response to multiple,
    recurrent, CH HSSs. The remainder of the outlook period is likely to
    mostly quiet.


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