• ARLP031 The ARRL Solar Report

    From ARRL@3:633/280.2 to All on Saturday, August 23, 2025 05:11:28
    SB PROP @ ARL $ARLP031
    ARLP031 The ARRL Solar Report

    ZCZC AP31
    QST de W1AW
    Propagation Forecast Bulletin 31 ARLP031
    From ARRL Headquarters
    Newington CT August 22, 2025
    To all radio amateurs

    SB PROP ARL ARLP031
    ARLP031 The ARRL Solar Report

    On August 22, Spaceweather.com [ http://Spaceweather.com ] reports a fast-moving Coronal Mass Ejection, or CME, left the Sun on August 21.
    However, it is not Earth-directed, and is predicted to strike the planet
    Mars.


    Solar activity has decreased back to low levels with a few weak C-class
    flares observed from areas located in the northeast quadrant of the solar
    disk. There are currently three sunspot regions on the solar disk with the largest being Region AR4187. This region showed some weak leader spot growth. The remaining two regions were quiet and stable.


    Solar wind parameters reflected negative polarity coronal hole high-speed stream (CH HSS) influences. A disturbed solar wind environment is likely to continue through August 22.


    There is a slight chance for R1 (Minor) radio blackouts through August 23 due to the anticipated return of old active regions. Probabilities increase slightly to a chance for an isolated event, most likely from the east limb,
    on August 24 as old active regions return to view.


    Active conditions are likely again on August 28 due to negative polarity Coronal Hole High Speed Stream influences. Periods of G1 to G2
    (Minor-Moderate) storming are likely on September 5, with active conditions likely on September 4 and 6, due to positive polarity Coronal Hole High Speed Stream influences. The remainder of the period is expected to be at quiet or quiet to unsettled levels.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere, August 21, 2025, by F. K. Janda, OK1HH:


    "Higher solar activity in the first half of August was caused mainly by two sunspot groups (out of a total of 11-13), whose magnetic configuration
    allowed for the occurrence of moderately powerful eruptions (class M). After their disappearance, the number of groups dropped to three to five, while
    only energetically insignificant eruptions sporadically occurred.

    Changes in the speed of the solar wind and the concentration of particles in
    it had a significant impact on the Earth's ionosphere.

    As usual, the source on the Sun was the boundaries of coronal holes.

    "After a brief calm in the geomagnetic field from August 13 to 15, turbulent developments followed from August 19. At the beginning, the speed of the
    solar wind rapidly increased from 350 to 650 km/s, which was accompanied by a change in the polarity of the longitudinal component of the interplanetary magnetic field Bz to positive in a relatively long interval from 1130 to 1630 UT. Therefore, the deterioration of shortwave propagation conditions was only slight, while the MUF decline was delayed.

    We are now likely to see a series of relatively calm days, probably until August 27.


    Major disturbances are not expected to occur until around September 5, when
    the Earth will enter the same stream of solar particles as it did around
    August 9."


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


    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 August 23 to 29 is 5, 5, 8, 8, 10, 12,
    and 8, with a mean of 8. Predicted Planetary K Index is 2, 2, 3, 3, 3, 4, and 3, with a mean of 2.9. 10.7 centimeter flux is 120, 125, 120, 120, 125, 125, and 130, with a mean of 123.6.

    NNNN
    /EX

    ARRL The National Association for Amateur Radio(R)
    Unsubscribe [ http://www.arrl.org/opt-in-out?utm_source=Informz&utm_medium=Email&utm_campaign=ARRL
    ]



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    * Origin: American Radio Relay League (3:633/280.2@fidonet)
  • From ARRL@3:633/10 to All on Friday, July 31, 2026 22:18:24
    SB PROP @ ARL $ARLP031

    ARLP001 Propagation Forecast

    ZCZC AP31
    QST de W1AW
    Propagation Forecast Bulletin 1 ARLP001
    From ARRL Headquarters
    Newington, CT July 31, 2026
    To all radio amateurs

    SB PROP ARL ARLP031
    ARLP031 The ARRL Solar Report

    Solar activity has remained at low levels. Region 4494 exhibited decay in its trailing spots as its flare activity subsided. Region 4498 rotated into
    better viewing positioning, revealing mixed polarity just behind its large leading spot, and was responsible for a handful of low-level C-class flares.


    Region 4499 underwent evolution, gaining additional spots and producing a low-level C-class flare. Region 4501 rapidly emerged this period, developed rudimentary penumbra on its leading and trailing spots, produced a low-level C-class flare and was thus subsequently numbered. The remaining numbered
    active regions were unremarkable in relation.


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

    Solar activity is expected to be low with a chance for M-class flares (R1-R2, minor-moderate) through August 1.


    Solar wind parameters were at nominal levels. Solar wind speeds roughly
    ranged from 310 km/s to 401 km/s. A disturbed solar wind environment will likely return July 30 due to the prospect of combined positive polarity
    coronal high speed stream (CH HSS) effects and coronal mass ejection (CME) arrivals from events that left the Sun on July 26 27. An additional
    disturbance is likely on August 1 with the arrival of an additional CME that left the Sun late on July 27.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere, July 30, 2026, by F. K. Janda, OK1HH:


    During the last third of July, solar activity initially rose, while remained
    at a higher level until the end of the month.

    Although solar flares occasionally reached moderate intensity, while were exceptionally accompanied by coronal mass ejections, the Earth was not
    affected by them (though this could still happen by the end of July or early August, partly because there is a coronal hole in the southwestern part of
    the disk). There is only one active region on the far side of the Sun.

    Therefore, as the nine regions currently being observed fade, overall
    activity will decline shortly after the beginning of August.


    Shorter periods of increased geomagnetic activity may still occur in late
    July and at the beginning and end of the first third of August. Following the expected decline in solar activity, these will be followed at irregular intervals by shorter periods of deteriorated ionospheric conditions for shortwave propagation.


    The predicted Planetary A Index for July 31 to August 6 is 8, 5, 5, 5, 12,
    15, and 10, with a mean of 8.6. The predicted Planetary K Index is 3, 2, 2,
    2, 4, 3, and 3, with a mean of 2.7. Predicted 10.7 centimeter flux is 135,
    130, 125, 125, 125, 120, and 125, with a mean of 126.4.


    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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