SB PROP @ ARL $ARLP021
ARLP021 The ARRL Solar Report

ZCZC AP21
QST de W1AW
Propagation Forecast Bulletin 21 ARLP021

From ARRL Headquarters

Newington CT June 6, 2025
To all radio amateurs

SB PROP ARL ARLP021
ARLP021 The ARRL Solar Report

Solar activity remained at moderate levels earlier this week. There was an approximately 20-degree filament eruption on June 4 and a possibly related Coronal Mass Ejection (CME). The CME is unlikely to have an Earth-directed component, but analysis is in progress.


The geomagnetic field is expected to be quiet to unsettled on June 7 as High Speed Stream (HSS) activity continues. G1 (Minor) storm levels are likely
with the anticipated onset of a CME - that left the Sun on June 3 - around mid-to-late on June 7. On June 8, unsettled to active levels are expected.


Unsettled to active conditions are likely June 10 to 12 due to recurrent negative polarity Coronal Hole High Speed Stream (CH HSS) influences.
Unsettled to G1 (Minor) conditions are likely on June 13 to 22 due to
positive polarity CH HSS influences. Unsettled to G1 (Minor) conditions are likely on June 23 to 28 due to negative polarity CH HSS influences.


Solar activity is expected to be low with a chance for M-class flares (R1-R2/Minor-Moderate) and a slight chance for an X-class flare (R3-Strong)
on June 7.


Solar wind speed parameters increased from approximately 550 km/s to nearly
810 km/s before decreasing to around 760 km/s. This could either be transient influence or a transition back into the Coronal Hole High Speed Streams.


Quiet to active levels are expected to prevail on June 7.

Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere - June 5, 2025, from F. K. Janda, OK1HH:


"When assessing solar activity based on the sunspot, or more modernly based
on the intensity of solar radio noise, we can tentatively conclude that the maximum of the 25th cycle occurred last spring and summer, or early autumn
(the highest smoothed sunspot number was in October 2024: R12 = 160.8, and
then declined). Even so, it was much higher than most astronomers had predicted.


"But that's not the end of the story.
In May of this year in particular, there was a surprising increase in the number and energy of particles in the solar wind, especially during larger solar flares.

Particle ionization also affects the Earth's ionosphere, although not as
nicely as we would like given the state of the Earth's ionosphere.

In short, shortwave propagation conditions were rarely good during May and especially early June 2025. They were mostly unstable, disrupted, with irregular daily cycles and frequent occurrences of increased attenuation.


"An exceptional phenomenon is the so-called Forbush effect, also known as the 'Forbush decrease' in the intensity of galactic cosmic rays after the arrival of a CME in the vicinity of Earth.

The largest decrease in cosmic ray intensity in more than 20 years, by as
much as 25%, was recorded on June 1, 2025 (the last time this happened was on October 30, 2003). Particles ejected by the Sun will remain in our vicinity
and reduce the intensity of cosmic rays of galactic origin for another week
or two.


"A decline is generally expected in the further development of solar
activity. Only optimists admit that there will be one more increase this
year, probably in the northern half of the solar disk."


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 June 7 to 13 is 10, 8, 5, 15, 12, 10, and 35, with a mean of 13.6. Predicted Planetary K Index is 3, 3, 2, 4, 4, 3, and 6, with a mean of 3.6. Predicted 10.7 centimeter flux is 155, 155, 155, 155, 150, 150, and 155, with a mean of 153.6.

NNNN
/EX

ARRL The National Association for Amateur Radio(R)
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SB PROP @ ARL $ARLP021
ARLP021 Propagation Forecast

ZCZC AP21
QST de W1AW
Propagation Forecast Bulletin 21 ARLP021

From ARRL Headquarters

Newington, CT May 22, 2026
To all radio amateurs

SB PROP ARL ARLP021
ARLP021 The ARRL Solar Report

Solar activity continued at low levels during the past 24 hours with four active regions on the visible disk.

The largest events were a C1.0 on May 20 from the northeast limb and a
C1.0/Sf, also on May 20, from Region 4439 that was accompanied by Type-III radio sweeps. This region was responsible for the majority of the periods activity, which otherwise included a B8.7 flare on May 20 from Region 4436. Region 4441 showed some development during the period while 4443 remained stable. Coronal activity was observed in CCOR-1 imagery after May 20, but additional data is needed for further analysis.

Solar wind parameters trended toward background conditions with speeds
reaching a peak of 542 km/s on May 20 and then decreasing steadily throughout the reporting period, ending at ~450 km/s.


Weekly Commentary on the Sun, the Magnetosphere, and the Earth's Ionosphere
May 22 - May 28, 2026 by F. K. Janda, OK1HH


The number of sunspot groups on the solar disk ranged from three to seven
over the past week; their total area was not large, while their magnetic structure was relatively simple.

Nevertheless, isolated C-class flares were recorded.
In addition, there was even an M-class flare recorded on Sunday, May 17 (in
AR 4435 near the northwestern limb of the solar disk, peaking at 0339 UT). Thanks to the Solar Orbiter probe, however, we know that the situation will change.

Because, in a location where there was no group of sunspots during the
previous solar cycle, not only is there a group now, but it is also quite extensive.

Its edge is already slowly beginning to appear on the southeastern limb of
the solar disk.

While a week later, we can expect the peak of activity within the current
solar rotation.


The geomagnetic field will be mostly quiet to unsettled in the coming days, after which its activity will rise, initially slightly, and a disturbance can be expected toward the end of the month. This will result in a generally favorable development for the ionosphere for the remainder of May. This includes increases in geomagnetic activity, during which, depending on the timing, MUF values may temporarily rise.


The Predicted Planetary A Index for May 23 to May 29 is 5, 5, 5, 5, 12, 10,
and 8 with a mean of 7.The Predicted Planetary A Index for May 23 to May 29
is 5, 5, 5, 5, 12, 10, and 8 with a mean of 7.1. The Predicted Planetary K Index is 2, 2, 2, 2, 4, 3, and 3 with a mean of 2.6. 10.7 centimeter flux is 112, 112, 115, 115, 115, 120, and 125 with a mean of 116.3.


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 webpage 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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