• The ARRL Solar Report

    From ARRL de WD1CKS@VERT/WLARB to QST on Friday, February 14, 2025 21:21:27
    02/14/2025

    NOAA reports a G1 (Minor) geomagnetic Storm Watch has been issued
    for 14 Feb, 2025. A coronal hole high speed stream is expected to
    move into a position favorable for enhanced interaction between the
    high speed stream and Earth's magnetosphere. These enhancements are
    likely to cause elevated geomagnetic responses, with G1 (Minor)
    storm levels likely.

    From Spaceweather.com[1]: Another solar wind stream is heading for
    Earth. It is flowing from a canyon-like hole in the Sun's
    atmosphere. First contact with the stream on February 14th could
    cause a minor G1-class geomagnetic storm with Arctic auroras for
    Valentine's Day.

    The greatest observed 3 hr Kp over the past 24 hours was 4.� The
    greatest expected 3 hr Kp for February 13 to 15 is 4.67.

    No Minor S1 or greater solar radiation storms are expected.� No
    significant active region activity favorable for radiation storm
    production is forecast.

    Radio blackouts reaching the R1 levels were observed over the past
    24 hours. The largest was at February 13 at 1109 UTC.

    Solar activity is expected to be low with a chance for R1 to R2, and
    Minor to Moderate activity on February 13 to 15.

    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
    Ionosphere - February 13, 2025, by F. K. Janda, OK1HH:

    "Total solar activity was highest last October in the current
    11-year cycle. Since then, it has been declining, but slowly. This
    is also true for flare activity. Medium strong solar flares were
    produced mainly by the active region of AR3981. Some of these were
    accompanied by CMEs, none of which hit the Earth directly, but
    passed close enough to affect its atmosphere.

    "NOAA predicted on February 8 that there was a possibility of G1
    class geomagnetic storms on February 10 and 11. The prediction
    turned out to be fairly accurate - although geomagnetic field
    activity increased as early as February 9, it was highest on
    February 10 and was elevated on February 11. Therefore, ionospheric
    shortwave propagation conditions were at their worst on 10 February
    and subsequently improved only very slowly in the following days.

    "We now observe a large coronal hole, resembling a canyon, on the
    Sun, which could be another source of enhanced solar wind. Earth
    should be hit by it on Valentine's Day, or February 14. The days
    ahead will also be rather unsettled, but the active regions now
    rising near the southeastern limb of the solar disk will cause an
    uptick in solar activity, nevertheless, causing improved propagation conditions.

    "The good news at the end: at https://www.solarham.com[2] on the bottom
    left, after an eleven-week hiatus, we can see a map of the entire
    Sun, especially the Sun's far side, under the 'Farside Watch'
    banner. So the JSOC glitch has been fixed, and after another click
    on http://jsoc.stanford.edu/data/timed[3] we can read more under the
    heading 'Time-Distance Helioseismic Far-Side Imaging.'"

    The latest report from Dr. Tamitha Skov, WX6SWW, can be found online
    at, https://youtu.be/v5H2QsbiCqo[4] .



    [1] http://Spaceweather.com
    [2] https://www.solarham.com
    [3] http://jsoc.stanford.edu/data/timed
    [4] https://youtu.be/v5H2QsbiCqo

    ---
    � Synchronet � Whiskey Lover's Amateur Radio BBS
  • From ARRL de WD1CKS@VERT/WLARB to QST on Friday, February 21, 2025 20:43:08
    02/21/2025

    Solar activity is expected to range from low to moderate levels
    through March 15.� There is a varying chance for R1 or R2 (Minor or
    Moderate) events, and a slight chance for R3 or greater events.

    Geomagnetic field activity is likely to reach G1 (Minor) levels on
    February 28, March 9, and March 12 to 14.� Active levels are
    predicted for March 1. Quiet, and quiet to unsettled conditions are
    expected to prevail throughout the remainder of the period.

    The NOAA Ap Index Forecast is 5 for February 21 and 22.

    The NOAA Space Weather Prediction Center reports no space weather
    storms predicted for the next 24 hours.

    For the last 24 hours, solar flare activity has been at low levels
    with only a C-Class observed.� The largest flare was a C8.1 on
    February 19.

    This flare was accompanied by a Type II radio emission and
    associated CME off the Southwest edge of the solar disk. Modelling
    efforts determined the bulk of the CME to miss ahead of Earth's
    orbit.� However, a weak glancing influence cannot be ruled out late
    on February 24.

    Region AR3996 is the largest and most complex region on the disk but
    was responsible for only one C-Class flare. Flux emergence and an
    increase in interior spots can be seen in Region AR3998 but overall
    the region has been fairly quiet.

    Spaceweather.com[1] has an article link from the "Advancing Earth And
    Space Sciences" website concerning an extreme compression of Earth's
    magnetic field that was caused by the May 2024 solar superstorm.

    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
    Ionosphere - February 20, 2025, by F. K. Janda, OK1HH:

    "The increase in geomagnetic activity following the decrease in
    solar activity is a simple phenomenon to explain: systems of
    magnetic field lines over active regions in the Sun open up and
    charged particles (both free electrons and the nuclei of hydrogen
    atoms, or protons themselves) slip through them more easily into
    space.

    "In Earth's orbit, we see an increase in the solar wind and,
    consequently, an increase in geomagnetic activity. At the same time,
    the ionization rate of the ionosphere is increasing, while the
    shortwave propagation conditions may not only worsen (due to
    scattering on inhomogeneities) but also improve as the MUF may grow.
    This was well known, for example, on Saturday 15 February on the
    Europe-North America route.

    "The only geomagnetically quiet days in the first half of the month
    were 3-7 February. Then the solar wind, blowing from the long
    canyon-shaped coronal hole, intensified and geomagnetic activity was
    elevated for most of the second third of February. A calm trend can
    be expected on most days of the last third of the month. Although
    there does not appear to be a significant increase in solar
    activity, it is sufficiently high. In addition, spring is
    approaching, which is good news for the state of the ionosphere."

    The predicted Planetary A Index is 5 for February 21 to 26, and 10
    on February 27.� The predicted Planetary K Index is 2 on February 22
    to 26, and 3 on February 27.� Predicted 10.7 cm solar flux is 170
    for February 22 to 23, 190 on February 24, 195 on February 25, 200
    on February 26, and 195 on February 27.

    Sunspot numbers for February 16 to 20, 2025 were 271, 218, 187, 119,
    and 123, with a mean of 183.6.




    [1] http://Spaceweather.com

    ---
    � Synchronet � Whiskey Lover's Amateur Radio BBS
  • From ARRL de WD1CKS@VERT/WLARB to QST on Friday, February 28, 2025 19:54:28
    02/28/2025

    A Coronal Mass Ejection (CME) associated with a filament eruption
    became visible on February 26 at 1448 UTC.� Model analysis
    determined this CME to be a miss ahead of the Sun/Earth line.

    Unsettled to active levels are likely on February 28 to March 1 as a
    Coronal Hole influence continues, and a glancing blow is possible
    from a Coronal Mass Ejection that occurred on February 25.

    Solar activity is forecast to range from low to moderate levels
    through March 22.

    Minor to Moderate activity (R1 to R2) is possible at different
    points throughout the period as active regions grow, evolve, and
    return from the far-side of the Sun. There is a slight chance for R3
    (Major) or greater events if any of the active regions develop
    additional complex magnetic structures.

    Geomagnetic field activity is expected to be at quiet to unsettled
    levels until March 6 with periodic, weak Coronal Hole influences.
    Unsettled to active levels, with isolated G1 (Minor) storming
    conditions are likely from March 7 to 18 as recurrent negative
    polarity Coronal Holes are expected to be in a geoeffective
    position.

    NOAA Space Weather[1] forecasts a 55% chance of a Class-M flare, and a
    10% chance of a Class-X flare, both within the next 48 hours
    (February 28 to March 1).

    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
    Ionosphere - February 27, 2025, by F. K. Janda, OK1HH:

    "Solar activity is now increasing, but the increase is irregular,
    which causes, among other things, a decrease in the reliability of
    forecasts. Geomagnetically quiet periods, especially when associated
    with an increase in total solar activity (such as 20-23 February),
    are accompanied by improved conditions for ionospheric radio wave
    propagation. A subsequent disturbance can cause even further
    improvement (which happened on 24 February).

    "Following the increase in solar flare activity (from 23 February),
    two proton flares were observed on 24 February. In the following
    days, the Earth's ionosphere was under the influence of a
    solar-derived proton rain, after which the density of free electrons
    in it decreased due to recombination.

    "However, the worsening of conditions was only noticeable on 25
    February. The very next day, 26 February, there was an improvement,
    in particular an increase in the MUF on a global scale. The jump in
    the solar wind speed also contributed. However, the changes were so
    rapid, even within a single day, that our assessment of the level of
    conditions could have been reversed, depending on the time of day
    and the frequency bands used.

    "The developments described can be considered as a harbinger of a
    March increase in solar activity. Since the Spring Equinox is
    approaching, it will contribute to an improvement in ionospheric
    shortwave propagation, more accurately called decameter waves. The
    possible shorter worse spells on March 1-2 and March 5-6 will make
    no difference, with the seasonal improvement not fully manifesting
    itself until the second half of the month."

    This weekend is the ARRL International DX SSB contest.� Information
    can be found at, https://www.arrl.org/arrl-dx[2] .

    For more information concerning shortwave radio propagation, see http://www.arrl.org/propagation[3] and the ARRL Technical Information
    Service web page at, http://arrl.org/propagation-of-rf-signals[4]. For
    an explanation of numbers used in this bulletin, see http://arrl.org/the-sun-the-earth-the-ionosphere[5] . Information and
    tutorials on propagation can be found at, http://k9la.us/[6] .

    Also, check this:

    https://bit.ly/3Rc8Njt[7]

    "Understanding Solar Indices" from September 2002 QST.

    The predicted 10.7 cm flux for February 28 to March 6 is 195, 195,
    190, 190, 190, 190, and 185, with a mean of 190.7.� The predicted
    Planetary A Index for February 28 to March 6 is 12, 10, 8, 5, 5, 5,
    and 5, with a mean of 7.1.� The predicted K Index for February 28 to
    March 6 is 4, 3, 3, 2, 2, 2, and 2, with a mean of 2.6.




    [1] https://www.swpc.noaa.gov/
    [2] https://www.arrl.org/arrl-dx
    [3] http://www.arrl.org/propagation
    [4] http://arrl.org/propagation-of-rf-signals
    [5] http://arrl.org/the-sun-the-earth-the-ionosphere
    [6] http://k9la.us/
    [7] https://bit.ly/3Rc8Njt

    ---
    � Synchronet � Whiskey Lover's Amateur Radio BBS
  • From ARRL de WD1CKS@VERT/WLARB to QST on Friday, March 07, 2025 19:10:48
    03/07/2025

    Spaceweather.com[1] is reporting "A Hole In The Sun's Atmosphere" that
    should reach Earth on March 9 and 10.

    Solar activity has been at moderate levels for the past 24 hours.
    The largest solar event of the period was a M1 event observed on
    March 5 at 1150z from Region 4016. There are currently 10 numbered
    sunspot regions on the disk.

    Solar activity is expected to be low with a chance for M-class
    flares and a slight chance for an X-class flare on March 7 and 8.

    There is a chance for isolated minor solar radiation storm levels
    throughout the period if any of the returning/developing
    magnetically complex regions are active and produce an event.

    Geomagnetic field activity is expected to be at quiet to unsettled
    levels on March 7 to 9, 19 to 24, and on March 29.� Active levels
    are expected on March 10 to 18, and then on March 25 to 28, with
    possible G1 (Minor geomagnetic storm) conditions on March 12 to 15
    associated with recurrent negative polarity Coronal Hole influences.

    Quiet to unsettled conditions are expected on as weak, glancing CME
    effects continue to wane with quiet conditions prevailing on March
    7.� Unsettled to active levels are expected on March 8 as CIR - a
    CIR is a Corotating Interaction Region, its primary effect creates
    disturbances in the solar wind by interacting between fast and slow
    streams of solar plasma - effects ahead of a recurrent, negative
    polarity Coronal Hole become geoeffective.

    The NOAA Space Weather Prediction Center with its Geomagnetic
    Activity forecast for March 7 to 9 has a 40% chance of Active
    activity on March 8, a 40% chance of a Minor storm on March 9, a 15%
    chance of a Moderate storm on March 9, and a 1% chance of a
    Strong/Extreme storm during this same reporting period.

    Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
    Ionosphere - March 6, 2025, by F. K. Janda, OK1HH:

    "The combination of relatively low total solar activity and a larger
    number of geomagnetic disturbances caused a worsening of shortwave
    propagation conditions in February. However, the outlook for March
    is better, not least because of the approaching equinox (which
    occurs on 20 March).

    "Solar activity will begin to increase more rapidly after the larger
    sunspot groups return to the Sun's disk (which is the half of the
    Sun's surface visible from Earth). At its eastern limb we should see
    their activity as early as mid-March. They will approach the centre
    of the disk just around the Vernal Equinox on March 20.

    "But even before that, the scenario may be somewhat different. In
    the north-west of the solar disk, we see a large coronal hole, which
    is likely to be the source of a strong solar wind that will probably
    affect the Earth's ionosphere sooner than we expect. But this too
    could be a harbinger of a further upsurge in solar activity. So -
    within reason - all good news."

    For more information concerning shortwave radio propagation, see http://www.arrl.org/propagation[2] and the ARRL Technical Information
    Service web page at, http://arrl.org/propagation-of-rf-signals[3]. For
    an explanation of numbers used in this bulletin, see http://arrl.org/the-sun-the-earth-the-ionosphere[4] . Information and
    tutorials on propagation can be found at, http://k9la.us/[5] .

    Also, check this:

    https://bit.ly/3Rc8Njt[6]

    "Understanding Solar Indices" from September 2002 QST.

    The forecast 10.7 centimeter flux for March 7 to 13 is 150, 150,
    150, 155, 160, 170, and 180, with a mean of 59.3.� The forecasted
    Planetary A Index for March 7 to 13 is 5, 5, 8, 15, 15, 25, and 30,
    with a mean of 14.7.� The forecast Planetary K Index for March 7 to
    13 is 2, 2, 3, 4, 4, 5, and 5, with a mean of 3.6.



    [1] http://Spaceweather.com
    [2] http://www.arrl.org/propagation
    [3] http://arrl.org/propagation-of-rf-signals
    [4] http://arrl.org/the-sun-the-earth-the-ionosphere
    [5] http://k9la.us/
    [6] https://bit.ly/3Rc8Njt

    ---
    � Synchronet � Whiskey Lover's Amateur Radio BBS