• ARLP039 The ARRL Solar Report

    From ARRL@3:633/10 to All on Fri Oct 17 15:35:44 2025
    SB PROP @ ARL $ARLP039
    ARLP039 The ARRL Solar Report

    ZCZC AP39
    QST de W1AW
    Propagation Forecast Bulletin 39 ARLP039
    From ARRL Headquarters
    Newington CT, October 17, 2025
    To all radio amateurs

    SB PROP ARL ARLP039
    ARLP039 The ARRL Solar Report

    Region AR4246 underwent significant evolution, growing in overall size while gaining multiple new spots. Subsequently, AR4246 was the main provider of activity, which included an M1.2 flare on October 13. Several coronal mass ejections (CMEs) with potential Earth-directed components are in the mix at this time.


    Additional modeling efforts are underway to perhaps confirm those suspicions. The largest flare was a long-duration M4.8/2n on October 15. Modeling efforts showed the ejecta to be on a northward trajectory and not on an Earthward course.


    Other notable activity included a prominence eruption off the ENE limb-first visible in LASCO C2 imagery on October 14. Given the location of the event, initial analysis suggests this ejecta to be well into foul-ball territory and not Earth-directed. Additional modeling efforts are underway to perhaps
    confirm this suspicion.


    Slight decay was observed in the intermediate portion of Region AR4248 as it grew in length. Region AR4247 was in decay as well. The remaining regions
    were unremarkable in comparison. No new regions were assigned numbers this period. Minor to moderate (R1-R2) radio blackouts are likely for the next 3 days, with a slight chance for an isolated R3 (strong) event, due to the current and potential flare activity of Regions AR4246 and AR4248.


    Solar wind parameters continued to reflect the influence of a negative
    polarity coronal hole high-speed stream (CH HSS). Solar wind speeds finally dipped below 600 km/s, and phi was predominantly in the negative solar
    sector.


    Solar wind parameters are expected to continue at enhanced levels, although gradually waning, and continuing through October 17, due to CME arrivals from the October 11 to 13 timeframe originating from AR4246. Solar activity
    reached moderate levels due to M-class flare activity.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere, October 16, 2025, by F. K. Janda, OK1HH:


    "In line with forecasts, solar activity continued to gradually increase, including several moderately strong flares. These were mostly observed in the active region NOAA 4246, located in the northwest of the solar disk, while approaching its limb.


    "The second of the two larger active regions is NOAA 4248, also located in
    the northwest, but closer to the central meridian and the solar equator,
    while relatively close to the extensive coronal hole No. 87. In the coming days, AR NOAA 4248 will move into the active longitudes. Therefore, its eruptive activity will increase. Between it and the aforementioned coronal hole, a source of intensified solar wind will form, which will hit Earth
    during the coming week.


    "Even earlier, on October 16, when this text is being written, we expect a G2 geomagnetic disturbance, which will first cause a brief improvement and then
    a deterioration in ionospheric propagation of short waves, which have been rather average so far. The exception was a shorter increase in MUF on October 15 between 1000 and 1200 UTC, probably caused by an intensification of the solar wind.


    "Solar activity should remain at current levels for the rest of the month. Fluctuations in propagation conditions, mostly around average with occasional deterioration, will depend on the irregular occurrence of geomagnetic disturbances."


    The latest video report from Dr. Tamitha Skov, WX6SWW, can be found
    on YouTube at: https://www.youtube.com/watch?v=pAZtua4DZUs [ https://www.youtube.com/watch?v=pAZtua4DZUs ] .


    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 October 18 to 24 is 5, 5, 15, 10, 8, 5,
    and 5, with a mean of 7.6. Predicted Planetary K Index is 2, 2, 5, 3, 3, 2,
    and 2, with a mean of 2.7. 10.7-centimeter flux is 150, 150, 150, 150, 145, 140, and 145, with a mean of 147.1.

    NNNN
    /EX

    ARRL The National Association for Amateur Radio(R)
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    --- PyGate Linux v1.0
    * Origin: Dragon's Lair, PyGate NNTP<>Fido Gate (3:633/10)
  • From ARRL@3:633/10 to All on Sun Oct 18 15:08:45 2026
    SB PROP @ ARL $ARLP039

    ARLP039 Propagation Forecast

    ZCZC AP39

    QST de W1AW

    Propagation Forecast Bulletin 39 ARLP039

    From ARRL Headquarters

    Newington, CT September 25, 2026

    To all radio amateurs

    SB PROP ARL ARLP039

    ARLP039 The ARRL Solar Report

    Solar activity is likely to continue at low levels with isolated to
    occasional C-class flare activity, along with a slight chance for R1-R2 (Minor-Moderate) M-class flare events, through September 25, according to NOAA”s Space Weather Prediction Center. The SWPC reports that nine sunspot regions are on the visible disk, including a new Region 4541. There were
    three solar flares observed in the past week, none of which was directed
    toward Earth.


    A disturbed solar wind environment was expected to arrive late yesterday, followed by positive polarity coronal hole high-speed stream (+CH HSS) influences continuing through September 25.


    Unsettled to active geomagnetic field conditions levels are expected as of today under early +CH HSS effects, including isolated periods of G1 (Minor) geomagnetic storming today and tomorrow.


    The Australian Space Weather Forecasting Centre”s global HF propagation forecast for middle latitudes is for mild degradation today due to forecast geomagnetic activity, followed by normal propagation in the days that follow. We are currently in a period of equinoctial propagation, during which conditions are relatively uniform around the world.


    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere, September 24, 2026, by F. K. Janda, OK1HH:


    After a prolonged period of calm activity on the Sun as well as in Earth”s magnetosphere¢spanning the entire second third of September¢solar activity began to rise first, followed by an increase in geomagnetic activity starting on September 24. On September 18 only, there were no sunspots on the Sun. The rise in solar activity on the 24th was accompanied by an intensification of
    the solar wind,


    while the geomagnetic disturbance began its so-called positive phase (the critical frequencies f0F2 increased significantly between 9:00 and 13:00 UT). Improved shortwave propagation conditions were observed on September 23¤24.


    Solar activity will remain at a higher level for several more days, while the geomagnetic disturbance will continue only briefly in the so-called negative phase of development. A calm period is expected to follow during the last few days of the month. Recovery from the disturbance will likely be rapid, while
    a return to improved shortwave propagation conditions can be expected for
    most of the remaining days of the month.


    The Predicted Planetary A Index for September 25 to October 1 is 18, 12, 8,
    5, 5, 5, and 5 with a mean of 8.3. The Predicted Planetary K Index is 5, 3,
    3, 2, 2, 2, and 2 with a mean of 2.7. 10.7 centimeter flux is 105, 105, 100, 105, 110, 115, and 115 with a mean of 107.9.


    For more information concerning shortwave radio propagation, see www.arrl.org/propagation and the ARRL Technical Information Service web page
    at www.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. Information and tutorials on propagation can be found at http://k9la.us?utm_source?RL&utm_campaign4937f7b69-EMAIL_CAMPAIGN_2026_09_25_02_16&utm_medium?ail&utm_term?-34937f7b69-443795558.


    Also, check this: "Understanding Solar Indices" from September 2002 QST. https://bit.ly/3Rc8Njt?utm_source?RL&utm_campaign4937f7b69-EMAIL_CAMPAIGN_2026_09_25_02_16&utm_medium?ail&utm_term?-34937f7b69-443795558


    NNNN

    /EX


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    --- PyGate Linux v1.5.19
    * Origin: Dragon's Lair, PyGate NNTP<>Fido Gate (3:633/10)