SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA
ZCZC AP24
QST de W1AW
Propagation Forecast Bulletin
24 ARLP024
From Tad Cook, K7RA
Seattle, WA June 28, 2024
To all radio amateurs
SB PROP ARL ARLP024
ARLP024 Propagation de K7RA
ASWFC GEOMAGNETIC DISTURBANCE
WARNING ISSUED
AT 0538UTC/28
JUNE 2024
BY THE AUSTRALIAN SPACE
WEATHER
FORECASTING
CENTRE:
"A glancing blow from a recent CME is expected to
arrive late on
UT day 28-Jun.
Additional to
this, solar
wind parameter
Bz has been
oriented
southward for
approximately
15 hours.
Combined this
may induce G1
geomagnetic
conditions. A
second CME is
expected to
arrive late on
UT day 29-Jun
and may also
cause G1
geomagnetic
conditions.
"INCREASED GEOMAGNETIC
ACTIVITY
EXPECTED DUE
TO CORONAL
MASS
EJECTION FROM 28-29 JUNE
2024."
Nine new sunspot groups
emerged over
this reporting
week, June
20-26.
Two appeared on June 21, four
on June 23,
two more on
June 25 and
one on June
26.
Average daily sunspot number
declined from
149.6 to
141.6, but
average daily
solar flux
increased from
178 to 195.1.
Average planetary A index
declined from
10.3 to 7.
Predicted solar flux for the
near term is
182 on June
28-30, then
180, 185, 180,
175, and 190
on July 1-5,
180 on July
6-7, then 165,
165 and 180 on
July 8-10, 170
on July 11-13,
then 180, 190
and 195 on
July 14-16,
then 200 on
July 17-18,
195 on July
19-20, 190 on
July 21-28, then 195, 190,
185 and 190 on
July 29
through August
1, and 180 on
August 2-3.
Predicted planetary A index
is 12 and 15
on June 28-29,
5 on June 30
through July
13, then 10,
10 and 8 on
July 14-16, 5
on July 17-19,
8 on July 20,
then 5 on July
21-26, 8 on
July 27-28,
and 5 on July
29 to August
9.
Geomagnetic activity forecast
for the period
June 28 - July
04, 2024, from
Tomas Bayer,
RWC Prague,
Institute of
Geophysics of
the ASCR,
Prague,
Department of
Geomagnetism
Budkov
observatory
(BDV):
"Quiet: June 30 to July 1, 3
and 4
"Unsettled: June 28 and 29,
July 1 and 2
"Active: possible June 28 and
29, July 2
"Minor storm: 0
"Major storm: 0
"Severe storm: 0
"Next week, we expect quiet
to unsettled
conditions.
Two unsettled
to active
events are
possible next
week.
"The first one is possible
about June 28
- 29, and the
other one, but
unlikely,
about July 2.
Other days, we
expect quiet
to unsettled
conditions."
George Hoffman, W7POE, wrote
in an email:
"A question some of us have
is, with the
quite high SFI
and SSN
numbers, why
is the MUF
around the
Washington
state region
never much
above 21 MHz
these days?
For me 10
meters was
totally dead
during Field Day. I haven't
seen MUFs in
the 30 MHz
region for
several weeks
now. Wonder if
you could shed
some light on
this puzzling
issue.
Thanks."
I replied that I suspect this
is because of
seasonal
variation.
I used the W6ELprop program
to estimate
MUF over a
specific path
(Dallas, Texas
from Seattle)
with an
estimated
smoothed
sunspot number
of 133.
For the current date (June
27) it shows
the MUF at
about 22 MHz,
day and night.
But when I change the date back closer to the
Spring Equinox
(just before
March 28), the
MUF is highest
from 2030-2100
UTC at 34.7
MHz.
It also shows MUF above 28
MHz from
1530-0230 UTC.
George also shared a very
useful link:
https://prop.kc2g.com
George replied:
"I also just ran W6ELprop and
got 22 MHz for
the Burien to
Dallas path
and 17.6 MHz
for the Burien
to New York
path. Anyway,
I will wait
around for 10
meter
openings.
Thanks again."
William Paul, KD6JUI, of
Dixon,
California
wrote in an
email:
"I was operating from my
kayak again on
Field Day. 10
watts into a
homebrew loop.
My ops were
all SSB.
"Only heard one (1!) station
on 10m, so all
my operating
was confined
to 15m. I had
enough
exchanges to
keep me happy
but there was
a lot of
fading. Didn't
hear any
foreign
stations
coming in.
"Did get some fine photos of
bees
pollinating
water flowers.
"Maybe if Field Day were held
in December
and with the
same high
solar flux, 15
and 10 meters
would've been
a lot more
active."
K7RA comment: There is Winter
Field Day in
January.
NASA images:
https://bit.ly/3LmluV7
Solar max and climate:
https://tinyurl.com/mu6wv455
Active sunspot returns:
https://tinyurl.com/nhcpu46h
https://tinyurl.com/fjea8zf8
Big sunspot:
https://tinyurl.com/tuc8kyee
Send your tips, reports,
observations,
questions, and
comments to
[email protected]. When reporting
observations,
don't forget
to tell us
which mode you
were
operating.
For more information
concerning
shortwave
radio
propagation,
see
www.arrl.org/propagation and the ARRL Technical
Information
Service web
page at
www.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.
An archive of past
propagation
bulletins is
at
www.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
June 20
through 26
2024 were 138,
133, 139, 176,
141, 129, and
135, with a
mean of 149.6.
10.7 cm flux
was 203.3,
196.9, 195.7,
195.8, 198.7,
193.7, and
181.4, with a
mean of 178.
Estimated
planetary A
indices were
7, 5, 4, 10,
5, 9, and 9,
with a mean of
10.3. Middle
latitude A
index was 8,
4, 6, 12, 7,
9, and 8, with
a mean of
10.1.
NNNN
/EX
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