Subj : The K7RA Solar Update
To   : QST
From : ARRL de WD1CKS
Date : Fri Apr 05 2024 04:12 pm

 04/05/2024 

With the big increase in sunspot numbers and solar flux reported in
last week's Propagation Forecast Bulletin ARLP013, I hoped the trend
would continue, but numbers this week were lower.

Five new sunspot groups emerged, one each day from March 30 through
April 3.

Average daily sunspot numbers went from 147 to 60, and average daily
solar flux declined from 191.9 to 136.9.

Geomagnetic numbers were much quieter. Average daily planetary A
index softened to 7.6 from 25.4.

Predicted solar flux is 115 on April 5-8, 120 on April 9-10, 125 on
April 11, 140 on April 12-13, 150 on April 14-16, 160 on April
17-18, 170 on April 19-24, then 160, 150 and 140 on April 25-27,
then 130 on April 28 through May 4 then 160, 150, and 140 on May
5-10, then 150 on May 11-13.

The predicted flux values this week are much lower than in last
week's forecast for the same period.

Predicted planetary A index is 16 and 10 on April 5-6, 5 on April
7-8, 8 on April 9-10, 5 on April 11-18, 8 and 10 on April 19-20, 8
on April 21-23, 5 on April 24-26, 10 on April 27-28, 8 on April 29,
and 12 on April 30 through May 2, then 8, 5 and 5 on May 3-5, 8 on
May 6-8, and 5 on May 9-15.

The Weekly Commentary on the Sun, the Magnetosphere, and the Earth's
Ionosphere - April 4, 2024 from OK1HH:

"The two large and very active sunspot groups, AR3614 and AR3615,
bade us farewell last week by going beyond the western limb of the
solar disk. AR3615 still unleashed two powerful M-class flares and
an X1 flare that ionized the upper part of the Earth's atmosphere
and caused the Dellinger effect (shortwave fade) over the Pacific
Ocean on March 28 (with a maximum at 2053 UTC).

"AR3615 still managed to produce an M9.4-class solar flare on March
30, which was only one percent weaker than an X-class flare. After
that, we expected particles originating from solar radiation to
arrive in the vicinity of Earth, but this did not happen. The
development in the following days was therefore relatively quiet.

"Due to the calming of the geomagnetic field, we expected an
improvement in shortwave propagation. This occurred from 2 April
onwards but was only very slight due to the rapid decrease in solar
activity. After the return of active regions to the solar disk, we
expect an improvement in propagation, especially in the third decade
of April."

(I think he refers to a decade as a ten day period, so this would be
the last ten days of April).

Angel Santana, WP3GW, sent an email about last week's contest:

"WPX for me was pretty good even though I did not reach my goal.
There were openings toward Europe during Saturday midnight on 20
meters.

"Now on Sunday at midday, I noticed a reduction of stations on 10
meters, just like 2 weeks ago, but there were many strong stations
from South America and an hour later back to normal. My friend Jose,
KP4JRS (who operated as NP3YL) noticed this over the two days on 10
meters.

"Also noticed when a big contest is on the air, the bands tend to be
almost 'noiseless.'

"Not sure if because the SFI has gone down but today Thursday at
1500 UTC there is much noise on the bands. Hope the weekend fares
better."

WX2R reminds us that coming up on Monday, April 8 is the HamSCI
Solar Eclipse QSO Party:

"Join with thousands of your fellow amateurs as part of the largest
crowd-sourced event for ham radio scientific exploration ever! The
SEQP is part of 'The Festivals of Eclipse Ionospheric Science' and
is for learning more about how the ionosphere works. Use any mode,
any band for all or part of the day!

"Participation can be from everywhere - you need not be near the
path of the eclipse to contribute valuable data by participating.

"Are you a contester? For details on the SEQP contest and rules go
to www.hamsci.org/contest-info[1]. Don't forget to send in your log.

"For the Gladstone Signal Spotting Challenge using CW, WSPR and
FST4W modes, go to www.hamsci.org/contest-info[2].

"If you're an SWL or AM DX'er, there is the 'Medium Wave Recording
Event' for you as well. Go to www.hamsci.org/mw-recordings/[3].

"Or just get on the air and help provide the data to better