• Weekly Highlights of Solar and Geomagnetic Activity, 09 - 15 February 2

    From SWPC.Webmaster@3:633/10 to All on Mon Feb 16 13:00:07 2026
    Subject: Weekly Highlights of Solar and Geomagnetic Activity, 09 - 15 February 2026

    :Product: Weekly Highlights and Forecasts
    :Issued: 2026 Feb 16 0314 UTC
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    # Weekly Highlights and Forecasts
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    Highlights of Solar and Geomagnetic Activity
    09 - 15 February 2026

    Solar activity reached moderate levels on 09, 11, 12, and 13 Feb and
    was at low levels on 10, 14, and 15 Feb. Region 4366 (N14, L=203,
    class/area Fkc/950 on 09 Feb) continued to be the most prolific spot
    group, producing five out of the six M-class flares during the
    period. The largest flare was an M2.8 flare that occurred at 09/0227
    UTC, followed by an M1.2 at 10/0009 UTC, an M1.1 at 11/0044 UTC, an
    M1.4 at 11/1312 UTC, and finally an M1.4 at 12/0240 UTC. Region 4373
    (N09, L=110, class/area Hax/140 on 10 Feb) was the only other region
    to contribute to the M-flare activity, adding an M1.0/Sf flare at
    13/0858 UTC. There were 35 C-class flares, with the largest being a
    C9.2/Sf at 09/2302 UTC from Region 4374.

    CME activity included a large filament (located near N15W25) that
    lifted off and disappeared from GONG H-alpha imagery at around
    10/1910Z. Initial coronagraph imagery from LASCO C2 at 10/1948Z
    revealed the eruption likely coincided with a separate eruption from
    S22W80 (first visible in C2 at 10/1924Z). This event is thought to
    have passed near Earth late on 14 Feb, slightly enhancing the
    geomagnetic field. Additionally, a CME associated with the M1.0 on
    13 Feb first became visible off the NW in LASCO C2 at 13/0924Z and
    first visible in STEREO COR2 imagery at 13/0938Z. This event likely
    arrived at Earth on 15 Feb, possibly embedded in the CH HSS.

    No proton events were observed at geosynchronous orbit on 09-15 Feb.

    The greater than 2 MeV electron flux at geosynchronous orbit was at
    high levels on 09, 10, 12, and 13 Feb, reaching a peak flux value of
    1,764 pfu at 09/1500 UTC. Flux levels were at moderate levels on 11,
    14, and 15 Feb.

    Geomagnetic field activity was at quiet to unsettled levels on 09
    and 12 Feb, reached active levels on 10, 11, 13, and 14 Feb, and
    reached minor storm levels on 15 Feb. The elevated levels starting
    on 09 Feb and lasting through 14 Feb were likely associated with
    negative polarity coronal hole (CH) high speed stream (HSS)
    influences combined with intermittent transient effects. The
    increase in activity on 15 Feb is thought to be the result of a
    co-rotating interaction region ahead of a positive polarity CH HSS,
    possibly mixed with glancing effects from the CME that left the Sun
    on 13 Feb.

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    Forecast of Solar and Geomagnetic Activity
    16 February - 14 March 2026

    Solar activity is expected to continue at low levels, with a slight
    chance for M-class (R1-R2, Minor-Moderate) flares on 16-21 Feb.
    Activity is expected to increase to moderate levels with M-class
    (R1-R2, Minor-Moderate) flares expected and a chance for X-class
    (R3-Strong or greater) on 22 Feb through 07 Mar as Region 4366
    returns to the visible disk. Activity should then decrease to low
    levels, with a chance for M-class (R1-R2, Minor-Moderate) flares on
    08-09 Mar as Region 4366 transits the western limb. Low levels, with
    a chance for M-class flares, are expected to return on 10-14 Mar as
    old Region 4366 rotates to the far side once again.

    The greater than 10 MeV proton flux levels are likely to be below
    the S1 (Minor) level on 16-21 Feb and again on 08-14 Mar. There is a
    chance for the 10 MeV proton flux to reach S1-S2 (Minor-Moderate)
    storm levels from 22 Feb-07 Mar as old Region 4366 returns to the
    visible disk.

    The greater than 2 MeV electron flux at geosynchronous orbit is
    expected to be at high levels on 16 Feb through 03 Mar, 06-08 Mar,
    and 11-12 Mar as CH HSS influence sporadically continues. Moderate
    levels are likely on 04-05, 09-10, and 13-14 Mar, outside of CH HSS
    influence.

    Geomagnetic field activity is expected to be at unsettled to active
    levels on 16-21 Feb, 24-25 Feb, 05-07 Mar, and 10 Mar due to
    recurrent negative polarity CH HSS effects. Active conditions are
    likely on 12 Mar following a solar sector boundary crossing, then
    again on 14 Mar with the onset of a positive polarity CH HSS.
    Barring the potential for CME activity, mostly quiet to unsettled
    levels are expected from 19-23 Feb, 26 Feb - 04 Mar, and 08, 09, 11,
    and 13 Mar.


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