• ARLP012 Propagation de K7RA

    From ARRL Web site@3:633/280.2 to All on Sat Mar 23 02:23:44 2024
    SB PROP @ ARL $ARLP012
    ARLP012 Propagation de K7RA

    ZCZC AP12
    QST de W1AW
    Propagation Forecast Bulletin 12 ARLP012
    From Tad Cook, K7RA
    Seattle, WA March 22, 2024
    To all radio amateurs

    SB PROP ARL ARLP012
    ARLP012 Propagation de K7RA

    Over March 14-20, new sunspot groups emerged every day except March
    19. March 18 had two, and each of the other days saw one new sunspot
    group.

    It is now Spring in the Northern Hemisphere which is favorable to HF conditions, and solar and geomagnetic numbers both show improvement.

    Average daily sunspot numbers rose from 82.3 to 94.3, and average
    daily solar flux jumped from 130.4 to 153.3.

    Geomagnetic indicators were very quiet, with the average daily
    planetary A index dropping from 8.9 to 5.9, and middle latitude
    numbers from 7 to 5.

    Here is the outlook for the next month.

    Predicted solar flux is 180 and 178 on March 22-23, 174 on March
    24-25, then 176 on March 26-27, 178 on March 28, 165 on March 29-30,
    160 on March 31, 155 on April 1-3, then 158 on April 4, 160 on April
    5-6, then 162, 155, 150, and 145 on April 7-10, 148 on April 11-12,
    then 152, 155, 160, 162, 165 and 160 on April 13-18, then 155 on
    April 19-20, 152 on April 21, 160 on April 22-23, then 162, 165, 165
    and 160 on April 24-27, and 155 on April 28-30.

    Predicted planetary A index is 12, 5, 16, 18 and 8 on March 22-26,
    then 5, 5 and 8 on March 27-29, 5 on March 30 through April 2, then
    15, 12 and 12 on April 3-5, 5 on April 6-8, 8 on April 9-11, then 5
    on April 12-23, 10 on April 24-25, and 5 on April 26-29.

    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
    Ionosphere - March 21, 2024, from F.K. Janda, OK1HH:

    "Solar activity on average continues to increase toward the Solar
    Cycle 25 maximum. This included a shower of protons that came from
    the admittedly smaller in X-ray intensity but primarily long-lived
    flare on the morning hours UTC of March 15. The particle density
    peaked a day later when the proton event reached S1. High polar cap
    absorption of radio waves was recorded at the same time.

    "The geomagnetic field remains mostly calm, with the occurrence of
    short active intervals. An increase in geomagnetic activity was
    expected after the eruption of 17 March. A partial CME halo was
    observed and ejected particles were expected in the vicinity of the
    Earth first on 20 March, then on the evening of 20 March, and then
    on the morning of 21 March. The result was an increase in MUF
    already in the forenoon UTC. An increase in the Earth's magnetic
    field activity occurred in the afternoon.

    "The new sunspot group AR3615, which emerged in the southeast of the
    solar disk, although not yet large, has a complex magnetic
    structure. This configuration increases the probability of magnetic reconnection during a solar flare. Especially if an X-class solar
    flare occurs, the probability of CME will increase."

    Angel Santana, WP3GW wrote about conditions on March 16 in an email:

    "With much expectation worked the Russian DX contest on SSB, but
    then noticed rough conditions, so bad that after 1600 UTC signals
    were gone, not seen on my radio. After 1730 UTC saw them come back
    but conditions were still bad.

    "Next day did the BARTG RTTY contest after 1430 UTC and fared
    better.

    "Did it have to do with one of the six sunspots last week? Hope prop
    is good in a week from now."

    I replied that according to Spaceweather.com, departing sunspot
    AR3599 blasted protons toward Earth on March 14, causing a polar cap
    absorption event on March 16. The ionizing effect of the protons
    absorbed radio signals inside the arctic circle.

    Nasa Space Flight article about VLA detection of radiation above
    sunspots:

    https://bit.ly/4cDDref

    Article about Radio Blackout:

    https://bit.ly/3ILT6KH

    From Dr. Tamitha Skov, WX6SWW:

    "Dear Tad,

    "Recently our Sun gave us a surprise when a solar storm we thought
    would be a glancing blow, actually hit us pretty hard. That was back
    on March 3rd and some gorgeous aurora shows were seen in Tasmania
    and Australia (see my forecast from that week for some amazing
    pictures: https://youtu.be/2nWLAYL01FA).

    "Here we are several weeks later with yet another glancing blow set
    to hit us midday March 20th. The official forecast is calling for a
    weak impact, but our recent experience has left me wondering: Are we
    are going to make the same mistake twice?

    "These are the kinds of dilemmas that make space weather such a
    tough field today. Compared to terrestrial weather, there are so
    many things we simply cannot foresee.

    "Turning to the forecast, big flare activity is beginning again
    thanks to old Region 3590 rotating back into view along with some
    new players as well. Amateur radio bands are getting noisier and
    radio blackouts are resuming on the daylight side of Earth. Of
    course, the big story is the solar storm coming towards us. Will it
    be relatively mild at mid-latitudes, as the predictions suggest?
    This time, I'm not so sure. Either way, I will remain on the
    lookout.

    "Cheers, Tamitha."

    Here is her latest video report:

    https://youtu.be/O6vZDFaBfrc

    Send your tips, reports, observations, questions, and comments to k7ra@arrl.net. When reporting observations, don't forget to tell us
    which mode you were operating.

    For more information concerning shortwave radio propagation, see http://www.arrl.org/propagation and the ARRL Technical Information
    Service web page at, http://arrl.org/propagation-of-rf-signals . For
    an explanation of numbers used in this bulletin, see http://arrl.org/the-sun-the-earth-the-ionosphere .

    An archive of past propagation bulletins is at http://arrl.org/w1aw-bulletins-archive-propagation . More good
    information and tutorials on propagation are at http://k9la.us/ .

    Also, check this QST article about Solar Indices:

    https://bit.ly/3Rc8Njt

    Instructions for starting or ending email distribution of ARRL
    bulletins are at http://arrl.org/bulletins .

    Sunspot numbers for March 14 through 20 2024 were 88, 49, 67, 86,
    127, 123, and 120, with a mean of 94.3. 10.7 cm flux was 127.1, 129,
    144.1, 151.3, 177.4, 168.9, and 175.5, with a mean of 153.3.
    Estimated planetary A indices were 8, 8, 3, 3, 6, 9, and 4, with a
    mean of 5.9. Middle latitude A index was 7, 8, 3, 2, 5, 7, and 3,
    with a mean of 5.
    NNNN
    /EX


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    * Origin: American Radio Relay League (3:633/280.2@fidonet)