• ARLP006 The ARRL Solar Report

    From ARRL@3:633/280.2 to All on Sat Feb 22 09:12:56 2025
    SB PROP @ ARL $ARLP006
    ARLP006 The ARRL Solar Report

    ZCZC AP06
    QST de W1AW
    Propagation Forecast Bulletin 6 ARLP006
    From ARRL Headquarters
    Newington CT February 21, 2025
    To all radio amateurs

    SB PROP ARL ARLP006
    ARLP006 The ARRL Solar Report

    Solar activity is expected to range from low to moderate levels through March 15. There is a varying chance for R1 or R2 (Minor or Moderate) events, and a slight chance for R3 or greater events.


    Geomagnetic field activity is likely to reach G1 (Minor) levels on February
    28, March 9, and March 12 to 14. Active levels are predicted for March 1. Quiet, and quiet to unsettled conditions are expected to prevail throughout
    the remainder of the period.


    The NOAA Ap Index Forecast is 5 for February 21 and 22.

    The NOAA Space Weather Prediction Center reports no space weather storms predicted for the next 24 hours.


    For the last 24 hours, solar flare activity has been at low levels with only
    a C-Class observed. The largest flare was a C8.1 on February 19.


    This flare was accompanied by a Type II radio emission and associated CME off the Southwest edge of the solar disk. Modelling efforts determined the bulk
    of the CME to miss ahead of Earth's orbit. However, a weak glancing influence cannot be ruled out late on February 24.


    Region AR3996 is the largest and most complex region on the disk but was responsible for only one C-Class flare. Flux emergence and an increase in interior spots can be seen in Region AR3998 but overall the region has been fairly quiet.


    Spaceweather.com [ http://Spaceweather.com ] has an article link from the ''Advancing Earth And Space Sciences'' website concerning an extreme compression of Earth's magnetic field that was caused by the May 2024 solar superstorm.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere - February 20, 2025, by F. K. Janda, OK1HH:


    ''The increase in geomagnetic activity following the decrease in solar
    activity is a simple phenomenon to explain: systems of magnetic field lines over active regions in the Sun open up and charged particles (both free electrons and the nuclei of hydrogen atoms, or protons themselves) slip
    through them more easily into space.


    ''In Earth's orbit, we see an increase in the solar wind and, consequently,
    an increase in geomagnetic activity. At the same time, the ionization rate of the ionosphere is increasing, while the shortwave propagation conditions may not only worsen (due to scattering on inhomogeneities) but also improve as
    the MUF may grow. This was well known, for example, on Saturday 15 February
    on the Europe-North America route.


    ''The only geomagnetically quiet days in the first half of the month were 3-7 February. Then the solar wind, blowing from the long canyon-shaped coronal hole, intensified and geomagnetic activity was elevated for most of the
    second third of February. A calm trend can be expected on most days of the
    last third of the month. Although there does not appear to be a significant increase in solar activity, it is sufficiently high. In addition, spring is approaching, which is good news for the state of the ionosphere.''


    The predicted Planetary A Index is 5 for February 21 to 26, and 10 on
    February 27. The predicted Planetary K Index is 2 on February 22 to 26, and 3 on February 27. Predicted 10.7 cm solar flux is 170 for February 22 to 23,
    190 on February 24, 195 on February 25, 200 on February 26, and 195 on
    February 27.


    Sunspot numbers for February 16 to 20, 2025 were 271, 218, 187, 119, and 123, with a mean of 183.6.

    NNNN
    /EX

    ARRL The National Association for Amateur Radio(R)
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  • From ARRL@3:633/10 to All on Fri Feb 6 20:03:05 2026
    SB PROP @ ARL $ARLP006
    ARLP006 The ARRL Solar Report

    ZCZC AP06
    QST de W1AW
    Propagation Forecast Bulletin 6 ARLP006
    From ARRL Headquarters
    Newington, CT February 6, 2026
    To all radio amateurs

    SB PROP ARL ARLP006
    ARLP006 The ARRL Solar Report

    Solar activity was at high levels for most of the week, dominated by Region 4366. The most notable event was an impulsive X4.2 flare from that region on February 4. Throughout the period, Region 4366 continued to exhibit a slight reduction in area and a modest simplification of its magnetic complexity. The remaining numbered regions on the visible disk remained stable or in a state
    of slight decay.


    Three eruptions were observed in coronagraph imagery during the period. First was a coronal mass ejection (CME) off the southeastern limb, first observed
    in C2 imagery on February 4, and was likely associated with flaring near Regions 4370 and 4371. This event was followed by post-eruptive arcades also
    on February 4 at the same location, which further confirmed the source region despite flare activity being partially obscured by Region 4366. Modeling indicates no Earth-directed component.


    The second was a narrow eruption to the NNW, first seen in C2 imagery on February 4. While potentially associated with the aforementioned X4.2 event,
    it dissipated quickly, and its analysis is low confidence. Lastly, there was another narrow eruption noted off the NE, first visible in SOHO/LASCO C2 imagery. This event was likely a sympathetic eruption triggered by the X4.2, starting between Regions 4366 and 4367.


    There is a slight potential of minor glancing blows from these eruptions
    early on February 8.


    Solar wind parameters initially reflected nominal background conditions
    before showing a clear disturbance beginning February 3. Solar wind speed remained in a slow-wind regime, gradually increasing from about 290 km/s to a peak near 340 km/s.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere, February 5, 2026, by F. K. Janda, OK1HH:


    Solar activity has increased again, so the maximum of the 25th eleven-year cycle continues.

    This time, active region No.
    4366 is primarily responsible for this.
    It suddenly emerged on January 30 in the southeast of the solar disk in a simple Beta magnetic configuration.

    The next day, it did not grow, but changed its configuration to Beta-Gamma-Delta, allowing for larger solar flares.

    Then, on February 1, it increased its area tenfold, while an extremely strong proton flare was observed in it, peaking on February 2 at 0002 UT.


    Until February 4, it had further doubled in size, with the magnetic configuration remaining Beta-Gamma-Delta, while the production of
    energetically significant flares continued. One to two X-class flares and several M-class flares are recorded daily, while on February 4, active region No. 4366 crossed the central meridian.


    This further increased the likelihood of the Earth being hit by an
    intensified solar wind and the occurrence of stronger geomagnetic
    disturbances.

    Their onset was mostly predicted for February 5, with the possibility of occurring one or two days earlier.

    This is what happened, with the arrival of the CME recorded on February 4 at 1421 UT, and a G1 (Minor) geomagnetic disturbance developing.

    It is expected to continue until February 6 or possibly February 7. At the
    same time, the production of energetically significant flares could continue
    in active region No.

    4366 until February 7. At the same time, there will continue a period of slightly increased probability of the Earth being hit by a proton of solar origin.

    A decrease in solar and geomagnetic activity is expected in the following
    days.


    The Predicted Planetary A Index for February 7 to February 13 is 8, 8, 10, 8, 8, 5, and 20, with a mean of 9.5. Predicted Planetary K Index is 3, 3, 3, 3,
    3, 2, and 5 with a mean of 3.1. 10.7-centimeter flux is 125, 130, 135, 140, 135, 140, and 145, with a mean of 135.7.


    For more information concerning shortwave radio propagation, see www.arrl.org/propagation [ http://www.arrl.org/propagation?utm_source=Informz&utm_medium=Email&utm_campaign=ARRL
    ] and the ARRL Technical Information Service web page at www.arrl.org/propagation-of-rf-signals [ http://arrl.org/propagation-of-rf-signals ] . For an explanation of numbers used in this bulletin, see www.arrl.org/the-sun-the-earth-the-ionosphere [ http://arrl.org/the-sun-the-earth-the-ionosphere ] . Information and
    tutorials on propagation can be found at http://k9la.us [ http://k9la.us/ ] .


    Also, check this: ''Understanding Solar Indices'' from September 2002 QST. https://bit.ly/3Rc8Njt [ https://bit.ly/3Rc8Njt ]

    NNNN
    /EX

    ARRL The National Association for Amateur Radio(R)


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