• ARLP016 Propagation de K7RA

    From ARRL Web site@3:633/280.2 to All on Sat Apr 22 04:05:37 2023
    SB PROP @ ARL $ARLP016
    ARLP016 Propagation de K7RA

    ZCZC AP16
    QST de W1AW
    Propagation Forecast Bulletin 16 ARLP016
    From Tad Cook, K7RA
    Seattle, WA April 21, 2023
    To all radio amateurs

    SB PROP ARL ARLP016
    ARLP016 Propagation de K7RA

    Again this week sunspot numbers and solar flux were higher than the
    week before.

    Average daily sunspot numbers more than doubled, from 70.6 to 146.9,
    and average daily solar flux increased from 141 to 164.5. Both
    figures represent a substantial increase in solar activity.

    Planetary A index averages went from 7.6 to 8.1, while middle
    latitude A index advanced from 6.4 to 7.3.

    Three new sunspot groups emerged on April 13, one more on April 16,
    and another on April 17.

    Predicted solar flux over the next few weeks is 145, 140 and 135 on
    April 21-23, 130 on April 24-25, 125 on April 26-27, 160 on April
    28-29, 165 on April 30, 172 on May 1-3, 170 on May 4, 172 on May
    5-7, 178 on May 8, 182 on May 9-12, then 175, 178 and 170 on May
    13-15, 168 on May 16-17, 175 on May 18, then 172 on May 19-21, then
    168 and 162 on May 22-23, 160 on May 24-26, 165 on May 27, and 172
    on May 28-30.

    Predicted planetary A index is 20, 16, 12 and 8 on April 21-24, 5 on
    April 25-27, 15 on April 28-30, then 12 and 10 on May 1-2, 8 on May
    3-4, 5 on May 5-6, 12 on May 7, 5 on May 8-10, then 8 on May 11-12,
    5 on May 13-18, then 10, 8, 5 and 5 on May 19-22, 15 and 18 on May
    23-24, 15 on May 25-27, then 12 and 10 on May 28-29.

    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
    Ionosphere - April 20, 2023 from OK1HH.

    "Of the fifteen sunspot groups observed over the past week, AR3272
    and AR3282 were the source of most of the flares. Both had a
    beta-gamma magnitude configuration. 61 C-class flares and 4 M-class
    flares were observed.

    "The partial halo CMEs on 15 and 16 April were the source of
    particles that reached Earth on 18 April, when the solar wind speed
    increased abruptly at 1308 UTC and a geomagnetic disturbance
    developed.

    "A positive phase of the ionospheric disturbance was recorded on the
    afternoon of 18 April, followed by a negative phase on 19 April.
    This was followed on 20 April with a significant increase in f0F2
    and improved shortwave propagation conditions before noon UTC.

    "The outlook looks promising for the first half of May, when solar
    activity should increase further."

    Dan Handa, W7WA commented on the news last week about the current
    solar cycle reaching a peak earlier than predicted, perhaps by the
    end of this year.

    I told him I hoped it would not peak early, because I wanted to see
    several more years of increasing activity.

    Dan sent a very detailed graph of Solar Cycle 19 from 1954 to 1966,
    and wrote: "I have read, and more than once, a slow rise means a low
    sunspot max. The previous Solar Cycle 24 took five years to reach a
    relatively low maximum. A rapid increase can mean a high sunspot
    maximum. The granddaddy of our lifetime, Solar Cycle 19 peaked in
    three years!"

    I did not know this.

    In a subsequent message, Dan further commented:

    "There was a lot of short term variation in the Solar Cycle 19
    sunspot number, just like we're seeing now. From the graph the
    timing of the Solar Cycle 19 peak can be defined three different
    ways: the daily peak, the smoothed monthly peak or the smoothed
    yearly peak, take your pick."

    Another Solar Cycle 19? Many hams have dreamed of this for the past
    six decades.

    Dale, WB6MMQ reported that the solar images in the ARRL Letter with
    a preview of our Friday bulletin show a blank Sun. I wasn't sure
    what he was talking about, but now I realize this must be a stock
    image (not from me!) used in the Letter.

    I sent Dale links to some recent images from Spaceweather.com:

    https://www.spaceweather.com/images2023/20apr23/hmi1898.gif

    https://www.spaceweather.com/images2023/19apr23/hmi1898.gif

    https://www.spaceweather.com/images2023/18apr23/hmi1898.gif

    https://www.spaceweather.com/images2023/17apr23/hmi1898.gif

    I hope this clears up the confusion.

    An odd correlation between an ancient epidemic and solar activity:

    https://bit.ly/3Lsqfxf

    A story about a possible early Solar peak:

    https://www.space.com/sun-solar-maximum-may-arrive-early

    A story about possible M-class solar flares:

    https://bit.ly/3KVc1n1

    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 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/ .

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

    Sunspot numbers for April 13 through 19, 2023 were 154, 153, 151,
    155, 162, 140, and 113, with a mean of 146.9. 10.7 cm flux was
    159.5, 171.3, 175.8, 177.8, 166.6, 153.2, and 147, with a mean of
    164.5. Estimated planetary A indices were 6, 7, 9, 4, 6, 13, and 12,
    with a mean of 8.1. Middle latitude A index was 5, 10, 8, 4, 6, 9,
    and 9, with a mean of 7.3.
    NNNN
    /EX


    --- MBSE BBS v1.0.8 (Linux-x86_64)
    * Origin: American Radio Relay League (3:633/280.2@fidonet)
  • From ARRL Web site@3:633/280.2 to All on Sat Apr 20 00:17:53 2024
    SB PROP @ ARL $ARLP016
    ARLP016 Propagation de K7RA

    ZCZC AP16
    QST de W1AW
    Propagation Forecast Bulletin 16 ARLP016
    From Tad Cook, K7RA
    Seattle, WA April 19, 2024
    To all radio amateurs

    SB PROP ARL ARLP016
    ARLP016 Propagation de K7RA

    Solar activity increased dramatically this reporting week (April
    11-17), and thirteen new sunspot groups emerged. One appeared on
    April 11, two more on April 13, three more on April 14, another two
    on April 15, one more on April 16 and another two on April 17. On
    April 18 an additional two sunspot groups emerged, and the daily
    sunspot number increased to 247.

    The daily sunspot number was 199 on April 17, the highest value
    since July 12, 2023 when it was 219. On April 18, when the sunspot
    number was 247, it was the highest sunspot number since July 6, 2014
    when it was 256. That was back in Solar Cycle 24, so 247 is a new
    record for Solar Cycle 25.

    Average daily sunspot numbers jumped from 67.9 to 142.7, and average
    daily solar flux from 123.2 to 177.4.

    Predicted solar flux over the near term is 225 on April 19, 220 on
    April 20-21, 215 and 205 on April 22-23, 190 on April 24-25, then
    140, 130, 125 and 120 on April 26-29, then 125 on April 30 to May 6,
    and 130, 140, 150, 160 and 175 on May 7-11, then 180 on May 12-14,
    175 on May 15, 170 on May 16-17, then 167 and 165 on May 18-19, 160
    on May 20-21, then 155, 140, 135, 125 and 120 on May 22-26.

    Predicted planetary A index is 6, 10, 12 and 8 on April 19-22, 5 on
    April 23-27, 8 on April 28-29, 7 on April 30, 10 on May 1-3, 5 on
    May 4, 8 on May 5-7, 5 on May 8-11, 10 and 8 on May 12-13, then 5 on
    May 14-24, and 8 on May 25-26.

    "Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
    Ionosphere - April 18, 2024:

    "Over the past weekend, active sunspot regions began to emerge on
    the eastern limb as expected. Curiosity about what we would actually
    see was heightened because their flare activity during the last
    rotation was somewhat higher than usual. Therefore, the CME from a
    moderate eruption in the northern hemisphere of the Sun on April 11
    with a maximum at 1706 UTC was not a surprise. The arrival of the
    particle cloud on April 14 was therefore expected, but it missed the
    Earth.

    "Another CME was ejected towards Earth on 12 April. Although neither
    CME was particularly strong, a G1 class geomagnetic storm was
    expected. This occurred on 16 April, so either the particle cloud
    moved more slowly or traveled along a longer path toward the Earth.
    Either way, the disturbance worsened shortwave propagation on April
    16. But the improvement was rapid, starting as early as April 17.
    The credit for this goes to the increasing solar radiation coming
    from the active regions we can observe on the Sun this week and
    next.

    "Another weak CME left the Sun on April 15, and the Earth's impact
    was calculated for April 18. However, all predictions of
    disturbances at the current stage of the 11-year cycle are
    unreliable. They are usually either late (by a day or so) or not at
    all. The important thing is the result - due to the relatively high
    solar activity and at the same time the small number of geomagnetic disturbances, the shortwave propagation conditions are mostly above
    average. F.K. Janda, OK1HH."

    Check out these videos and an article on flare activity from
    EarthSky:

    https://bit.ly/3W4GTID

    On April 16, Samuel, K5KJ called ARRL headquarters about unusual
    propagation he experienced.

    He said flare activity caused a radio blackout, and on 40 meters he
    could not hear any local or regional signals.

    But he noticed foreign broadcast stations from Asia with good
    signals.

    He said this is just the opposite of what he expected during a
    blackout.

    Durango Herald article about sunspots and prominences:

    https://bit.ly/3Q3VDnh

    NASA on Space Weather:

    https://go.nasa.gov/49YFhDX

    From Science.Nasa.gov, Solar Moss:

    https://go.nasa.gov/4b3n4Wn

    See sunspots with eclipse glasses:

    https://bit.ly/4cXc5Qp

    I tried this, but had no luck, as the images were too tiny.

    The latest video from Dr. Tamitha Skov, WX6SWW, for April 14:

    https://youtu.be/Z1OClNvDg2o

    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 April 11 through 17 2024 were 81, 83, 115, 152,
    193, 176, and 199, with a mean of 142.7. 10.7 cm flux was 143.7,
    151.5, 161, 178.4, 191.9, 198.7, and 216.5, with a mean of 177.4.
    Estimated planetary A indices were 6, 7, 5, 6, 8, 31, and 7, with a
    mean of 10. Middle latitude A index was 6, 6, 6, 5, 7, 17, and 8,
    with a mean of 7.9.
    NNNN
    /EX


    --- MBSE BBS v1.0.8.4 (Linux-x86_64)
    * Origin: American Radio Relay League (3:633/280.2@fidonet)