• ARLP020 The ARRL Solar Report

    From ARRL@3:633/280.2 to All on Sat May 31 11:53:22 2025
    SB PROP @ ARL $ARLP020
    ARLP020 The ARRL Solar Report

    ZCZC AP20
    QST de W1AW
    Propagation Forecast Bulletin 20 ARLP020
    From ARRL Headquarters
    Newington CT May 30, 2025
    To all radio amateurs

    SB PROP ARL ARLP020
    ARLP020 The ARRL Solar Report

    Solar activity reached moderate levels early this past week with several flares. An X1-class flare erupted mid-week, but activity has slowed down with the majority of the low-level C-class flares. A coronal mass ejection (CME)
    was observed on May 27 with a flare from Region AR4100.


    Modelling determined the CME to be well behind Earth's orbit. No other potentially Earth-directed CMEs were detected in available coronagraph
    imagery. M-class flare activity, minor - moderate, is likely, with a slight chance for X-class flare events, strong or greater, through May 30.


    The forecast of Solar and Geomagnetic Activity to June 21, 2025

    Solar activity is likely to reach moderate levels
    (R1-R2/Minor-Moderate), with a chance for R3 (Strong), over the next three
    days as Region AR4098, the most productive region on the visible disk, makes its way to the west limb of the Sun. A chance for M-class X-ray activity (R1-R2) will persist throughout the outlook period due to multiple regions on the visible as well as multiple active regions scheduled to return from the
    far side of the Sun.


    No proton events are expected at geosynchronous orbit.

    The Geomagnetic field activity is expected to be at a mostly elevated level
    due to anticipated influence from multiple, recurrent coronal holes. G1
    (minor) geomagnetic storms are likely on June 13-14; active conditions are likely over June 2, June 5, June 10 and 11, and June 15 to 17.


    Unsettled conditions are likely over June 3 and 4, June 6 and 7, and June 18
    to 21. Quiet conditions are only expected on June 8 and 9.


    On May 30, Spaceweather.com reports on a Super-Fast Solar Wind, and a 24-hour Geomagnetic Storm.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere - May 29, 2025, from F. K, Janda, OK1HH:


    "On May 29, geomagnetic activity reached the level of a strong storm (Kp 7) worldwide, which came as no surprise to those who had been monitoring the recurring disturbances during the last four solar rotations, and especially
    the developments on the Sun over the last five days or so.


    "Solar flares were observed, only occasionally with coronal mass ejections (CMEs).

    Although the large coronal hole in the southwest of the solar disk
    disappeared, other coronal holes appeared across the solar disk in the meantime.

    The largest of these extends from the southwest to the northeast and has been crossing the central meridian since May 26.

    It has negative polarity and is associated with the arrival of a high-speed stream (up to about 730 km/s).

    Even in the coming days, after the current disturbance subsides, mild active storm conditions (Kp 4) will continue.


    "Overall solar activity will increase slightly in the coming days, and geomagnetically active days will alternate irregularly with calmer ones. Ionospheric conditions for shortwave propagation will improve, but at best
    only to average levels."


    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 ]

    The Predicted Planetary A Index for May 31 to June 6 is 8, 10, 12, 8, 10, 12, and 10, with a mean of 10. The Predicted Planetary K Index is 3, 3, 4, 3, 3,
    4, and 3, with a mean of 3.3. Predicted 10.7 centimeter flux is 125, 120,
    115, 110, 110, 115, and 120, with a mean of 116.4.

    NNNN
    /EX

    ARRL The National Association for Amateur Radio(R)
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    * Origin: American Radio Relay League (3:633/280.2@fidonet)
  • From ARRL@3:633/10 to All on Sat May 16 10:55:51 2026
    SB PROP @ ARL $ARLP020
    ARLP020 Propagation Forecast

    ZCZC AP20
    QST de W1AW
    Propagation Forecast Bulletin 20 ARLP020
    From ARRL Headquarters
    Newington, CT, May 15, 2026
    To all radio amateurs

    SB PROP ARL ARLP020
    ARLP020 The ARRL Solar Report

    Solar activity remained at low levels this past week. Region 4436 was responsible for the majority of the C-flare activity, including the largest flare of the period, a C2.3 that peaked on May 13. Region 4432 rotated off
    the west limb. Two new regions were numbered during the past 24 hours. Region 4437, which has since decayed to plage, and 4438, resulting in a total of 4 numbered regions now on the visible disk.


    No Earth-directed CMEs were observed in available coronagraph imagery.

    Solar activity is expected to remain predominately at low levels with a
    chance for M-class (R1-R2/minor-moderate) flares through May 16.


    The solar wind parameters reflected possible combined effects from a coronal hole high-speed stream (CH HSS) influence and a coronal mass ejection (CME) that left the Sun on May 10. The speeds and densities also increased during
    the period, reaching a maximum speed of 490 km/s, though these had decreased
    to 450 km/s by the end of the period.


    Solar wind parameters are expected to remain slightly disturbed through May
    14, as the glancing influence of the May 10 CME wanes and a positive polarity CH HSS remains geoeffective. On May 15 - 16, a corotating interaction region (CIR) associated with a negative polarity CH HSS is anticipated to arrive
    near Earth, likely resulting in more disturbed solar wind conditions.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere, May 14, 2026, by F. K Janda, OK1HH


    The decline in solar activity during the first two weeks of May was expected and correctly predicted, although it occurred later than during the previous solar rotation.

    The sunspot groups were small, and the magnetic fields and their
    configurations were mostly simple.

    Nevertheless, several solar flares occurred, the largest of which,
    accompanied by a CME, was observed on May 10 in the northeast of the solar disk.

    The time of observation (maximum of the event at 1339 UT) corresponds to the occurrence of the Dellinger effect.


    The distance of active regions on the Sun from coronal holes served as a relatively reliable indicator for predicting geomagnetic activity. This is
    one reason why the increase on May 13 was predicted with considerable
    accuracy. The forecast of the subsequent disturbance, expected on May 15¤17,
    is supported not only by developments during the previous solar rotation (on April 18¤21) but also by observations of a CME that could impact Earth.


    In the last third of the month, an increase in solar activity can be expected without major geomagnetic disturbances, i.e., favorable conditions regarding the state of the ionosphere.


    The latest solar report from Dr. Tamitha Skov, WX6SWW, can be found on
    YouTube at https://www.youtube.com/watch?v=qLnkogEGx5A [ https://www.youtube.com/watch?v=qLnkogEGx5A ]


    The Predicted Planetary A Index for May 16 to May 22 is 20, 18, 15, 5, 5, 8, and 10 with a mean of 11.6. The Predicted Planetary K Index is 5, 5, 4, 2, 2, 3, and 3 with a mean of 3.4. 10.7 centimeter flux is 125, 120, 122, 130, 130, 130, and 120 with a mean of 125.3.


    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://www.arrl.org/propagation-of-rf-signals?utm_source=Informz&utm_medium=Email&utm_campaign=ARRL
    ] . For an explanation of numbers used in this bulletin, see www.arrl.org/the-sun-the-earth-the-ionosphere [ http://www.arrl.org/the-sun-the-earth-the-ionosphere?utm_source=Informz&utm_medium=Email&utm_campaign=ARRL
    ] . 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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