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Главная » 2024 » Февраль » 24 » ARLP008 Propagation de K7RA
18:22
ARLP008 Propagation de K7RA

SB PROP @ ARL $ARLP008
ARLP008 Propagation de K7RA

ZCZC AP08
QST de W1AW 
Propagation Forecast Bulletin 8 ARLP008
From Tad Cook, K7RA
Seattle, WA February 23, 2024
To all radio amateurs 
SB PROP ARL ARLP008
ARLP008 Propagation de K7RA
"ASWFC GEOMAGNETIC DISTURBANCE WARNING ISSUED AT 0237 UTC/22
FEBRUARY 2024 BY THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE.
"A solar filament has erupted from the northwest solar quadrant and
a component of the predominately westward associated CME is expected
to arrive at the Earth during the second half of 24-Feb. G1
conditions, with the chance of G2 periods are possible during the
second half of 24-Feb and first half of 25-Feb. Modeling shows the
bulk of the CME missing the Earth.
"INCREASED GEOMAGNETIC ACTIVITY EXPECTED DUE TO CORONAL MASS
EJECTION FROM 24-25 FEBRUARY 2024."
Spaceweather.com wrote on February 22:
"TWO MAJOR SOLAR FLARES: Giant sunspot AR3590 just unleashed two
major X-class solar flares. The double blast approximately coincided
with a widely reported outage of cell phone service; however,
experts agree that the flares were probably not responsible. More
flares are in the offing. The sunspot has an unstable 'delta-class'
magnetic field, and it is turning toward Earth."
Sunspot numbers and solar flux values dropped over the past week,
with average daily sunspot numbers down from 134.6 to 84.4 and
average daily solar flux dropping from 190 to 164.
Geomagnetic conditions were very quiet. Planetary A index declined
from the low value of 7.4 to 4.4, and middle latitude A index from
6.1 to 3.5.
Only four new sunspot groups appeared, three on February 15 and one
on February 18.
Spaceweather.com says all their content is written by humans, with
no Artificial Intelligence at all.
I decided to ask an AI bot when Solar Cycle 25 will peak:
From Gemini AI bot:
"There are two main perspectives on when Solar Cycle 25 will reach
its maximum:
"Original prediction:
"An expert panel convened by NOAA, NASA, and ISES in 2019 predicted
a peak in July 2025 with a maximum sunspot number of 115.
"This prediction assumed a similar strength to the weak Solar Cycle
24.
"Revised prediction:
"In October 2023, NOAA's Space Weather Prediction Center (SWPC)
released a revised prediction based on observed activity. This new
prediction suggests a faster rise and higher peak, likely between
January and October 2024, with a sunspot number between 137 and 173.
"However, it's important to note that the timing could still fall
within the broad error range of November 2024 to March 2026.
"So, the answer depends on which prediction you consider:
"Original prediction: July 2025
"Revised prediction: Between January and October 2024 (more likely
than July 2025).
"It's important to stay updated on the latest information as
scientists continue to monitor the Sun's activity. You can find more
details and updates on the NOAA Space Weather Prediction Center
website:
"https://www.swpc.noaa.gov/products/solar-cycle-progression
"END AI BOT CONTENT."
I have bookmarked that last link.
IES stands for the International Space Environment Service.
Here is a revised outlook for the next month, from USAF via NOAA.
Predicted solar flux is 175 on February 23, 180 on February 24-29,
then 160 and 165 on March 1-2, 170 on March 3-9, 165 on March 10-16,
then 162, 160, and 165 on March 17-19, 170 on March 20-21, 172 on
March 22-23, 165 on March 24-26, and 155, 160, and 165 on March
27-29, and 170 on March 30 into the first week in April.
Predicted planetary A index is 6, 5, 20 and 10 on February 23-26,
and 5 on February 27 through March 23, 8 and 7 on March 24-25, and 5
on March 26 through the first week in April.
Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
Ionosphere - February 23-29, 2024 from F.K. Janda, OK1HH:
"During the last seven days, based on helioseismological
observations we first expected the rise of a larger active region at
the northeastern limb of the solar disk.
"Meanwhile, gradually most of the sunspot groups on its western half
have faded, whereby the solar flux has dropped to 152.
"The larger active region came out, was designated AR3590, and is
large enough to observe with the naked eye (in relation to the area
over 700 millionths of the solar disk), for example, using a solar
eclipse filter. However, its beta-gamma magnetic configuration was
not conducive to larger flares. All the more surprising were two
successive X-class flares: X1.8 on 21 February with a maximum at
2307 UT and X.1.7 on 22 February with a maximum at 0632 UT. However,
they were short-lived and not accompanied by CMEs. During the first
of these, shortwave propagation subsided, particularly in the
western USA and the Pacific (the Dellinger effect).
"Expect an increase in solar X-ray and ultraviolet radiation in the
coming days and mostly geomagnetically quiet conditions. As Spring
approaches, shortwave propagation will be mostly above average or
even better."
K7BTW posted this to the Western Washington DX Club email list on
February 20:
"Fantastic band conditions.
"If you're not taking advantage of these band conditions, you are
missing a lot. On 20 meters FT8 in the last few minutes around 8pm
(0400 UTC) I worked Middle East stations in Lebanon, Jordan, Saudi
Arabia, and Qatar, plus several UN and many Russians. Over the pole
conditions are incredible.
"Take advantage of the sunspot cycle. We know what it will be like
in 5 years!"
Jeff, N8II wrote on February 16:
"If we are at the peak, I would think this is a poor cycle.
"Not long ago the flux dropped below 130 briefly.
"10 meter conditions are excellent now with much better conditions
to East Asia in the evening than the first 3 weeks of January.
"Today at 2400 UTC 10 meters was open well to Taiwan working BX5AA
and also a BD4 around 0030 UTC. Japanese signals were excellent
until just before 0100 UTC. I heard 8R7X in Guyana running many
Japanese until 0100 UTC on 10 CW."
Here in Seattle where I (K7RA) live we have always had a pipeline to
Japan, which at times can seem overwhelming.

NNNN
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