CQ Amateur Radio - December 2021
CQ Amateur Radio - December 2021
CQ Amateur Radio - December 2021
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ON THE COVER:
HAPPY HOLIDAYS
FROM CQ !
26
FEATURES TECHNOLOGY SPECIAL: Wireless communication has always been at the
forefront of technology. This month, CQ salutes the role radio has played in
8 THE CENTENNIAL OF DXING expanding our technological universe from Marconi a century ago to modern
The East Coast Advantage to Europe wireless devices. Read all about it on pages 8, 11, 18, 22, 26, 31, 34, 38, 50,
Was First Observed 100 Years Ago 60, 66, and 75.
By Carl Luetzelshwab, K9LA
11 A JOURNEY TO THE MOON AND
BACK
By Stephen Werner, AG4W COLUMNS DEPARTMENTS
18 SATELLITE RAG CHEWING ON A
44 MATH’S NOTES: The Future Still 50 EMERGENCY COMMUNICATIONS:
SHOESTRING
Will Not Necessarily Be What We Using the Technology We Have
By Dennis Lazar, W4DNN
Think It Will By Stan Broadway, N8BHL
22 ARDUCON: AN ARDUINO-BASED By Irwin Math, WA2NDM 83 VHF PLUS: In Praise of FM Simplex
FOXHUNT TRANSMITTER
46 THE LISTENING POST: China Radio Activity
CONTROLLER
Gives Stations Genuine Names By Trent Fleming, N4DTF
By Charles E. Scharlau, NZØI &
By Gerry Dexter 86 AWARDS: YL Awards
Gerald Boyd, WB8WFK
53 KIT-BUILDING: A Trip West ... and By Steve Molo, KI4KWR
26 PY2GN: BRAZIL’S FIRST PUBLIC
Building Sputnik 89 DX: Get on the Air DX Challenge
WEBSDR STATION
By Joe Eisenberg, KØNEB Awards
By Martin Butera, PY2ZDX/LU9EFO
58 QRP: QRP is Contagious! By Bob Schenck, N2OO
31 AN FLDIGI COMPUTER INTERFACE
By R. Scott Rought, KA8SMA 94 CONTESTING: Getting An Assist
FROM SPARE PARTS
By Phil Karras, KE3FL 60 LEARNING CURVE: Inductors: A By Tim Shoppa, N3QE
Brief Primer 98 PROPAGATION: Solar Cycle
34 TRACKING AND ANALYZING
By Ron Ochu, KOØZ Progression and Forecast
DIGITAL TRANSMISSIONS OF
AIRCRAFT 64 ANALOG ADVENTURES: Haywire By Tomas Hood, NW7US
A Technical “Sidebar” for Hams State
By Murray Green, K3BEQ & John By Eric P. Nichols, KL7AJ 2 ANNOUNCEMENTS
Butler, GDØNFN 66 ANTENNAS: A Deep Dive into End- 3 HAM RADIO NEWS
38 UNINTERRUPTIBLE POWER Fed Half-Wave Antennas 6 ZERO BIAS
SUPPLIES FOR THE RADIO By Bob Glorioso, W1IS & 7 NEWSBYTES
AMATEUR Bob Rose, KC1DSQ 43 CQ HALL OF FAME
Or ... Why Aren’t You Using a UPS 75 MF/LF OPERATING: A New Theory of 54 SPURIOUS SIGNALS
Yet? Propagation for Long-Haul DX on
By Michael Tortorella, W2IY 54, 62 WHAT’S NEW
2200 Meters
By Roger Crofts, VK4YB 63 BEHIND THE BYLINES
42 ANNOUNCING: THE 2022 CQ
WORLD WIDE WPX RTTY CONTEST 79 HAM RADIO EXPLORER: Simply 106 CQ INDEX
By Ed Muns, WØYK Simplex 110 LOOKING AHEAD
56 2022 PERIODIC TABLE OF CONTESTS By Anthony A. Luscre, K8ZT 112 HAM SHOP
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ZERO BIAS: A CQ Editorial
BY RICH MOSESON,* W2VU
T
his is being written just a few weeks after all the hubbub Even everyday HF DX communications involve bouncing our
about the near-space trip of “Captain Kirk” (otherwise signals off different layers of the ionosphere, which — while tech-
known as actor William Shatner) aboard Jeff Bezos’s New nically part of Earth’s atmosphere — creates the boundary
Shepard space tourism capsule. Space, it seems, is cool again. between our atmosphere and outer space. In fact, William
But ham radio, it seems, is not … particularly in the eyes of many Shatner’s suborbital flight climbed to an altitude of 65 miles, the
hams. Our technology, in their view, isn’t very high compared lower boundary of the ionosphere’s E-layer. Our HF signals typ-
with such things as smartphones, tablets, and space travel. And ically travel much higher, to the F-layer.
many of these hams pass along this impression to neighbors, The first recorded use of ionospheric propagation for HF com-
friends, and reporters. “Well, it’s not very hi-tech but it still gets munication occurred 100 years ago this month (our second sig-
through …” This is the second big lie that hams tell about them- nificant anniversary this December) and the likely mechanics
selves and their hobby (the first is that ham radio is dying, when behind the paths those signals took is the subject of our lead
licensing numbers are at record levels and keep growing). article in this issue. Making the most of ionospheric propagation
Let me let you in on a little secret (and feel free to tell your requires at least a basic knowledge of “space weather,” as our
friends and neighbors) … if space is hi-tech, then so is ham ability to communicate over great distances depends heavily on
radio. Amateur radio is a spacefaring hobby — best as we can what’s happening on the sun and in the solar wind. Example: A
tell, the only spacefaring hobby — and has been since the dawn solar flare and Earth-directed coronal mass ejection (CME) two
of the space age (actually, even longer, but we’ll get to that). days before the CQ World Wide DX Contest’s SSB weekend at
This month marks a very important milestone in the history of the end of October threatened to severely degrade HF propa-
amateur radio space communications (actually, two, but we’ll gation. Fortunately for us, it missed us and propagation was
get to that, too). Sixty years ago this month, in December 1961, excellent on the contest weekend. But the well-prepared con-
the first amateur radio satellite, OSCAR-1, was launched into tester was aware and ready to make adjustments in strategy if
orbit. It was not only the first amateur radio satellite but the first needed. And our non-contesting colleagues in HamSCI
privately built satellite ever launched, period. <www.hamsci.org> were monitoring the CME’s impact on our
The birth of the amateur radio space program can be traced ionosphere with their personal space weather stations. (In what
to the pages of CQ in April 1959, when then-Semiconductors other hobby do people have personal space weather stations?)
Editor Don Stoner, W6TNS (SK), wrote about plans for a bal- All of this brings me around to the real reason for this rant:
loon-carried, solar-powered, transistor repeater and mused, This issue is our annual Technology Special, in which we spot-
“can anyone come up with a spare rocket for orbiting purpos- light not only the hi-tech aspects of our hobby but some of ham
es?” That throwaway line set in motion Project OSCAR (Orbiting radio’s vaunted tradition of repurposing existing technology for
Satellite Carrying Amateur Radio), in which Don and two other new functions. And in case you were wondering, in addition to
CQ columnists, George Jacobs, W3ASK, and Bill Orr, W6SAI analyzing propagation paths of a century ago, this issue’s arti-
(SK), became heavily involved. cles include just about everything we’ve discussed so far on this
Since 1961, over 100 satellites designed and built by hams page plus more: Moonbounce, satellites, a webSDR that will let
have been launched into orbit, providing long-range communi- you listen in on OSCAR-100 even if you aren’t in its footprint,
cations without worrying about the vagaries of propagation. microcontrollers and FLdigi, monitoring digital transmissions
OSCAR-100 is the first geosynchronous amateur radio satellite, from aircraft, a new look at old antenna technology, and a new
appearing to remain in one spot in the sky, just like those hi-tech theory on long-haul propagation on 2200 meters.
TV satellites. Its “footprint” covers all of Africa and Europe, most So, if you’re looking for a magazine about “making do” with
of Asia and some of South America. Oh, and did we mention aging technology to prop up a shrinking and aging hobby, you’ve
that OSCAR-94 is orbiting the Moon? come to the wrong place. But if you’re looking for a resource on
Nearly 40 years ago, in 1983, Astronaut Owen Garriott, W5LFL making the most of a spacefaring hobby that’s open to anyone,
(SK), took a 2-meter handheld with him into space aboard the that blends internet and RF technology to maximize your enjoy-
shuttle Columbia and made the first ham radio contacts from ment of what AA6JR calls the “magic in the sky,” then look no
Earth orbit. Today, amateur radio is a staple aboard the farther than right here. Because ham radio — and CQ — have
International Space Station, many astronauts hold ham licens- been taking you to “the final frontier” for decades and will con-
es and the ARISS (Amateur Radio on the International Space tinue to do so as we turn to the next page of our “captain’s log.”
Station) program has introduced thousands of young people to
both amateur radio and careers in science, technology, engi- Beyond Technology
neering, and math (STEM), not to mention space travel.
Of course, ham radio isn’t all about technology. It’s about using
Actually, amateur radio space communications extends back
technology to communicate, and having fun in the process.
even farther. The first two-way amateur radio moonbounce
Highlights of the communication-focused features in this issue
(EME) contact was made in 1960, and pioneering hams had
include our Periodic Table of Contests for 2022—a handy chart
been hearing their echoes off the moon since 1953. Hams began
of major on-air competitions for the entire year—and two looks
conducting experiments with meteor-scatter communications in
at making the most of simplex communication on VHF-FM.
the 1940s. The digital modes used for most meteor scatter con-
Finally, we want to wish all of our readers a Merry Christmas,
tacts today have their roots in software developed by K1JT for
Happy Hanukkah, Happy Kwanzaa, or whatever other holiday
cutting-edge radioastronomy.
you may celebrate to bring a little more THz-range radiation into
our lives in these dark winter months.
*Email: <w2vu@cq-amateur-radio.com> – 73, W2VU
T
hree major nominations by the
White House may shape the
face(s) of telecommunication pol-
icy for the next several years. Acting
FCC Chair Jessica Rosenworcel was
nominated by President Biden to anoth-
er full term on the commission and as
Chair. Once confirmed, she will be the
first woman to formally hold the FCC
Chairmanship. Rosenworcel has been
an FCC Commissioner since 2012.
According to the White House, she was
instrumental in creating the FCC’s
Emergency Broadband Benefit program
to help fight the “homework gap” during
pandemic lockdowns and help house-
holds struggling to afford internet ser-
vice stay connected. Prior to her
appointment to the FCC a decade ago,
she was Senior Communications Coun- FCC Acting Chair Jessica Rosen-
sel for the U.S. Senate Committee on worcel has been nominated for an addi-
Commerce, Science and Transporta- tional term on the Commission and as
tion, and previously practiced commu- Chair. She will be the first woman to be Open internet advocate Gigi Sohn has
nications law. a Senate-confirmed FCC Chair. (FCC been nominated to the FCC. (George-
(Continued on page 63) photo) town University photo)
You may read elsewhere about the centennial this month of the 1921
Transatlantic Tests from a historical perspective, and how they marked the
beginning of amateur radio DXing. In this article, K9LA looks at the
anniversary from the perspective of propagation and the beginning
of the “East Coast advantage” in both DXing and contesting.
* Email: Figure 1. Propagation paths from Ardrossan, Scotland to 1BCG and to 9ZJ. See
<carlluetzelschwab@gmail.com> text for details.
Summary
The Transatlantic Tests 100 years ago produced the first
observation of the East Coast advantage to Europe in ama-
teur radio. It is a sizable amount, and this continues to be
borne out a century later in contest results and DXing.
Notes:
1. See the comments in the left-hand column on page 12 of The Story
of the Transatlantics (K.B. Warner, QST, February 1922), and in the left-
hand column on page 27 of Official Report on the Second Transatlantics
(Paul. F. Godley, QST, February 1922). For details on the 9ZJ station,
see the comments on page 200 of A Study of Radio Signal Fading (J.H.
Dellinger, L.E. Whittemore, S. Kruse, Scientific Papers of the Bureau of
Standards, Vol 19).
2. It is generally acknowledged that the maximum distance for a sin-
gle hop at HF is 4,000 kilometers. But we have to watch it here. The
amount of refraction incurred by an electromagnetic wave from a given
electron density profile in the ionosphere is inversely proportional to the
square of the frequency. The lower you go in frequency, the more the
wave is bent and the wave doesn’t get as high into the ionosphere. Thus,
the wave ends up taking a shorter hop. The 4,000-kilometer limit for a
single hop is generally applicable to our higher HF bands (12 meters
and 10 meters). For 20 meters, 3,000 kilometers is a reasonable limit
for one hop. On 160 meters, 1,500-2,000 kilometers is likely. On 1.5
MHz (about where 9ZJ and 1BCG were operating), the hop distance will
be even less. This is the rationale for saying 9ZJ likely had an extra hop
compared to 1BCG.
3. With the nighttime E region critical frequency foE being around 0.35
MHz, elevation angles below about 13° will be confined to short and
lossy E hops. Higher elevation angles will go through the E region for
longer hops. Also, the higher elevation angles spend less time transit-
ing the absorbing region, so this results in a smaller amount of absorp-
tion. But as the elevation angle is increased, the more the hops, which
adds more absorption and more ground reflection loss (especially over
average ground, as is likely the case for the first hop out of 9ZJ).
A
fter hitting the Honor Roll and ing is unpredictable. If you don’t have which can result in 6-10 dB of loss. One
DXCC Challenge 2500, I decid- programmable polarity with your anten- of the biggest issues is sky noise. When
ed to take a different direction in nas, you must wait for polarity to shift. the moon is aligned with the Milky Way
ham radio. I have participated in near- Looking at the moon from different loca- or the Sun, the noise makes it impossi-
ly every aspect of the hobby over the tions puts the signal out of phase. That ble to communicate. There is also
last 50 years. During those 50 years, I spatial polarity relies on Faraday rota- Doppler shift which is greatest at moon-
mostly used existing or used equipment tion to make a contact. Libration fading rise or moonset. All of those factors
to gauge my interest. Some inexpensive is due to the rocking motion of the moon make each EME contact that much
starts, like my satellite station, turned into and bouncing off a jumbled surface more exciting.
a significant effort and investment.
In 2016, I started on another item on
my bucket list, moonbounce or Earth-
Moon-Earth (EME). I started with the
idea to do it as inexpensively as possi-
ble and let the other ham do the heavy
lifting. I had read that there were large
EME stations with 8 to 32 Yagis that could
hear single Yagis with a hundred watts.
It is amazing to see how much interest
European hams have invested in EME.
Some of their stations are spectacular!
Some would ask, why work EME? I am
a contester and DXer and this is the ulti-
mate DX contact, nearly 500,000 miles.
They are some of the most difficult con-
tacts that can be made. You will remem-
ber them like working Amsterdam Island
on 160 meters or multi-hop E-skip into
Japan on 6 meters. With sunspots still in
short supply despite Solar Cycle 25
commencing, it seemed like perfect tim-
ing. I am also an experimenter and there
is no part of the hobby that is better at
encouraging homebrew equipment and
experimenting.
Then there are the technical chal-
lenges. With EME, you have to deal with
Faraday rotation, spatial polarity, libra-
tion fading, sky noise, and Doppler shift.
Even working a station one state away,
the path has 251 dB of loss covering
nearly 478,000 miles. Now that is DX.
Only 6% of the radio signal that reach-
es the moon gets reflected back. With
Faraday rotation as the signal passes
through the ionosphere, it rotates in
polarity both on the way up and back.
The amount and speed of rotation shift-
Justin Johnson, GØKSC, is very gen- Receiver Research P144VDG <https:// na for the preamplifier. I suggest you
erous with sharing information on how to tinyurl.com/v2pdp8n4> that I used for make the preamplifier easily replace-
build LFA antennas. You can also buy satellites. It had a 0.5-dB noise figure. I able since they tend to get damaged
them from his company, InnovAntennas bought some surplus Ducommun high easily. I have been very pleased with
<www.innovantennas.com>. His web- power coaxial relays for $30 at a ham- the quick turnaround and support ARR
site, “GØKSC – Simple to build, High fest and made a switch box at the anten- provides in repairing its products.
Performance Yagi and Quad Antennas
– Home of the LFA Yagi – Free Yagi
Antenna Designs for Ham Radio”
<www.g0ksc.co.uk>, is amazing. He
has also been great for answering
questions.
The used Mirage amplifier I bought at
Dayton also had a GaAsFET preampli-
fier that needed work. I repaired the pre-
amplifier and started to hook it up to my
Yaesu FT-857. The only upgrade I
made to the FT-857 was adding a
TCXO-9 high stability crystal oscillator.
Most recommend putting the amplifi-
er and pre-amp right at the antenna. For
me, that would involve a number of
problems related to keeping it cool and
dry, and providing power at the anten-
na. I was able to obtain some hardline
which would significantly reduce the
attenuation so I planned to use the
amplifier in the shack to start out.
Then I was offered a 400-watt surplus
FAA amplifier that had been converted
to 2 meters at a price I could not refuse
(Photo B). So my initial rotors, antennas,
and amplifier were all upgraded from my
original plan before my first contact.
When I used the FAA amplifier, I upgrad- Photo E. The author’s EME antennas were originally set up with horizontal
ed the preamplifier to an Advanced polarization.
Former CQ Publisher Dick Cowan, ing Solid State Technology and, more recently, Vacuum
ex-WA2LRO, SK Technology and Coating. According to family members, he
had been battling Alzheimer’s disease for several years and
We recently learned of the passing last year of former CQ
passed away in June 2020 from complications of Covid-19.
Publisher Richard A. “Dick” Cowan, formerly WA2LRO. The
Our belated condolences to the Cowan family.
son of CQ‘s founding publisher, Sanford Cowan, Dick took
on the responsibilities of publisher in the late 1950s, even
though he wasn’t listed as such on the magazine’s mast-
head until mid-1967. In 1979, Cowan sold CQ to current
owner Dick Ross, K2MGA, and former Editor Alan Dorhoffer,
K2EEK (SK).
Recalling their relationship in the 50th anniversary issue of
CQ in 1995, Ross noted that Cowan, “was always extreme-
ly fair to me and … gave me the most important thing ever
– freedom. Freedom to learn and explore and see how things
happened and to become part of making them happen.”
Cowan was also founder and publisher of S9 magazine in
the heyday of the CB boom, as well as several others, includ-
EME. The second half of the ARRL EME contest was the
same weekend as CQWW CW DX Contest. I decided to work
the EME contest instead. It is fun working new countries and
grid squares on EME. During CQWW, I rarely get a new band Holiday
country, even on 160 meters. I made 45 contacts during the Rebates
first EME contest weekend in October. The previous year I 6KRSZLWK:HVW0RXQWDLQ5DGLRRU
made 44 contacts total over both weekends. By November DQ\RIRXUWUXVWHGGHDOHUVEHWZHHQ
2020, I had worked 185 unique stations on EME. Some of 1RYHPEHUWKDQG'HFHPEHUVW
those stations I have worked several times.
DQGVDYHRQDQ\SURGXFWRYHU
Some of my recent QSOs on 2-meter EME were China
XVLQJWKHFRGH
(BA4SI) and Trinidad (9Y4D). We have a short period of com-
mon moon with China, whereas the Trinidad station only runs
150 watts. Both stations took a lot of patience to work on
EME. I am always amazed at how courteous and helpful EME
Holiday21
stations are. Even with few sunspots and no DXpeditions dur- Visit westmountainradio.com for a
ing the pandemic, there is some good DX to be worked. full catalog of products
I was also able to work two stations with single Yagis and
400 watts on EME. One of them I have been trying to work Audioware RIGblasters
for four years. Was part of it luck? Absolutely, but it also helps ([SHULHQFHDXGLR ([SORUHGLJLWDOPRGHVZLWK
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that I don’t give up easy. EME is not for someone who enjoys EHIRUHZLWK:HVW WKDWNHHSVJLYLQJ
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In conclusion, EME operation is great for the experimenter,
DXer, and contester. Don’t be surprised if you enter into a
continuous state of upgrade to your station, some of which
may happen before the original approach is finished. You will RIGrunners CBA V
learn to develop patience making QSOs, but the rewards of (QMR\HDV\'&SRZHU
GLVWULEXWLRQZLWKRXUORQJOLQHRI *HW\RXUKDQGV
a QSO are amazing. You will also be pleasantly surprised by 5,*UXQQHUSURGXFWV RQWKHQHZ&%$9
how helpful other EME operators are to improve your station EDWWHU\DQDO\]HU
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One of the technical hallmarks of hams over the years has been
repurposing older technology to perform new tasks. In line with K8ZT’s new
column debuting this month on discovering new aspects of ham radio,
W4DNN shares his experience of getting started on amateur satellites with
a minimal investment in new gear.
L
ike many of us old time hams, over the past 60 years I derful hobby. But little by little, I felt that new radio itch: The
have moved from novice CW to AM phone, to that new- need for some new challenge. The answer came in the form
fangled SSB and FM repeaters. The past 20 years have of a magazine article about satellites.
been devoted to QRP, Straight Key Century Club, Summits Yes! That was it. I would work the world through the ham
on the Air, Parks on the Air, PSK-31, QRP, and QRO rag sats! However, my loving and supportive XYL Ruthie,
chewing and DXing, among many other aspects of this won- K4KLQ, while always sympathetic to my sometimes-eccen-
tric endeavors, said she was behind me all the way but with
* Email: <w4dnnradio@gmail.com> one caveat. As long as I didn’t spend any money, I could go
Figure 1. If you use compatible rigs, SatPC32 is available to you via the AMSAT website, <www.amsat.org>. This program
brings satellite ops into the 21st century.
normal sound, varying the transmitter while calling “CQ satel- trying to keep a voice intelligible on SSB. Until I can hone my
lite.” Then WOW … K8YSE answered and I attempted to tuning skills or spring for a new rig, I will stick mainly to oper-
reply while varying my voice on the uplink while I faded in ating CW.
and out. Later, in an email, John from Ohio said, “Congrats The wrap up to this tale is that I am able to achieve usable
on getting on sats. You were moving up the band and it was satellite QSOs in CW with my extremely minimal equipment
hard to follow you. Doppler control is something that is cru- and minimal operator skills. This has resulted in a happy ham,
cial to making contacts on the linear birds.” It was a disaster happy XYL, and any number of satellite operators who are
but I did end up making a first contact. I had done it! With a very happy that I am not messing up the SSB portions of the
weak signal to high-loss coax feeding a crummy antenna and pass bands — yet.
with a poor operator, it became plain that while I could make
contact, I might never be able to pull off an SSB rag chew
Epilogue: Since preparing this article, I found a 20-year-old
without a few station upgrades.
ICOM IC-910H satellite radio in great condition and for a
Then, on a pass of the CAS4B satellite, Bryan, K5CIS,
wife-approved $600. Coupling it with the Satpc32 program
answered my CQ in CW. I tried to call back but due to a com-
from AMSAT on an old XP laptop computer was flawless
bination of dirty contacts on my paddles (I had only planned
and easy (Photo C). Now I am making SSB and CW con-
to send dits) and my clumsy tuning, I only got out my call and
tacts with my longest rag chew lasting 8 minutes. My best
then lost him. A half hour later, however, on the XW-2A
DX QSO was Gustavo, HC2FG, in Guayaquil, Ecuador!
Chinese satellite, my CQ was answered by Howard,
However you begin your journey, you will find that working
WB2TQE, and, using a different key, we had a real QSO.
the sats is “out of this world.”
This experience was an epiphany for me. The spirit of QRP
came alive.
Resources
CW Forever – in Space You can find a great instructional from AMSAT explaining
As a diehard QRP enthusiast, former QRP Editor of CQ mag- how to operate the linear satellites using two radios without
azine, and author of many QRP-related articles, the name of computer control at <https://tinyurl.com/e99trrk9>. Another
the game had always been that CW can get through like no detailing taking Doppler tuning into the 21st century can be
other minimalist mode. I now learned that this can be applied found at: <https://tinyurl.com/4yej6jy8>. You will find a multi-
to satellites as well. part video presentation that is a how-to-do-it introduction to
First, CW cuts through the noise in satellite work much the satellite operation on a shoestring by KX9X at <https://
same as it does in low-band communications. The human tinyurl.com/3bzs7s3k>. You can download KEØPBR’s
ear can pull out a weak signal which is right at the noise level, Cheat Sheets from his web page at <https://tinyurl.com/
impossible to hear with SSB. Also, the CW signal is as read- d8xnedpv>. For an informative overview from ICOM, check
able at a high pitch as it is at a low pitch so it is not neces- out <https://tinyurl.com/3m9hpdyk>.
sary to keep the transmitter quite as precisely tuned as when
H
aving participated in and con- ancillary radio support positions often days. Notably, the International Amateur
ducted many transmitter hunts participate in these searches. Radio Union’s (IARU) official rules still
over the past 30 years, the The sport of amateur radio direction call for the use of AM modulation (A3A)
authors have long wished for a simple finding1 (ARDF) got its start shortly after for transmitters (or “foxes”) used in
way to conduct quality transmitter-hunt- the close of World War II, and has come competitions held on the amateur 2-
ing practice sessions. Simplicity, for us, a long way from those vacuum-tube meter band.
is defined as utilizing easy-to-obtain, beginnings. But this international sport Hams helping pinpoint locator bea-
reasonably priced equipment that is still clings to some vestiges of its early cons, and those participating in ARDF
easy to use. And a quality transmitter
hunting practice is one that provides a
realistic experience for the participants,
and is pulled off with nary a hitch. What
we’ve longed for is some reliable spe-
cialized equipment to make radio trans-
mitter practice hunts more realistic and
enjoyable for both the hunters and the
organizers.
The hunts we’re talking about are
practice sessions designed to provide
the participants with a genuine learn-
ing-by-doing experience. They are
intended to promote proficiency in find-
ing either of two transmitter varieties:
Locator beacons or ARDF (amateur
radio direction-finding) “foxes.”
Emergency locator transmitters (ELTs)
and personal locator beacons (PLBs) are
electronic, battery-operated transmitters
developed as a means of locating
downed aircraft and individuals experi-
encing an emergency while away from
normal emergency services. Many of
these devices transmit a low-power AM-
modulated signal on 121.5 MHz that can
be used by search and rescue (SAR) per-
sonnel to pinpoint the beacon’s location
using portable radio direction-finding
receivers. Radio amateurs serving in
# USA ARDF Co-coordinator Photo A. Photograph of Arducon installed on a handheld transceiver, with com-
Email: <wb8wfk@icloud.com> ponents labeled.
Arducon Design
Arducon takes advantage of the widely
available Arduino hardware platform
and free Integrated Development En-
vironment (IDE)2 to hold down costs
while making the project simple to mod-
ify and improve upon. An Arduino Pro
Mini is at the heart of Arducon, and all
the heavy lifting is done in software.
Only a simple interface board is added
to allow the Arduino Pro Mini to control
and be controlled by an HT. The inter-
face board includes “solder jumpers’’
that allow it to be configured for use with
a wide variety of HTs or even HF trans-
mitters for CW ARDF practice sessions.
The audio output from a connected
HT is fed into Arducon, which directly
samples it to decode any DTMF signals
it might contain. Upon receipt of a valid
tone sequence, Arducon will immedi-
ately perform a received command. In Figure 1. A simple diagram illustrating how Arducon connects to an HT.
Figure 2. A simple diagram illustrating how Arducon connects to a PC for configuration or programming.
R
adio transmissions have been with us for a long time. who were also hams bringing communication to isolated cor-
In the case of Brazil, since September 7, 1922. The ners of a giant country with continental distances such as
golden age of radio was responsible for the launch of Brazil.
many artists and changed the behavior of society. But times have changed and other communication tech-
Along with commercial radio broadcasts, Brazilian ama- nologies have been developed. But amateur radio has inte-
teur radio also played a large role, with high-level technicians grated many of those changes, such as WebSDR, or soft-
ware-defined radio accessible via the web. One of the most
* Email: <martin_butera@yahoo.com.ar> complete WebSDR servers in the world (Photo A) is locat-
Photo A. General view of the WebSDR station, belonging to William G. Schauff, PY2GN.
Photo C. On the left we can see the first SDR in Brazil, put up more than 15 years ago. The kit was sent directly from Japan
by Edson Wander, PY2SDR, to his friend PY2GN, who put it online in 2005 in the city of Pardinho. The photo on the right
shows the SDRShell software developed by PY2SDR in 2006.
Solar Energy
Pardinho’s WebSDR is so complete
that PY2GN has a backup power sys-
tem, made up of a 3Kva sinusoidal PHB
UPS (uninterruptible power supply).
The primary power source, though, is
solar. With an electricity consumption of
approximately 300 watts/hour, the
energy is generated in the field by 36
solar panels of 330-watts, 220-volts tri-
Photo E. WebSDR receivers phase, networked (Photo I).
A project built around a dental floss box and a mint tin … it practically
screams ham ingenuity! So improve your dental hygiene and build a fun
project all at the same time, courtesy of KE3FL.
T
his type of project may not be for the PC audio input port, unless your PC to find some way to reduce and / or elim-
everyone. But if you’re a “make do audio input port can be switched from inate the FLdigi noise and to keep back-
with whatever’s available” sort of stereo to mono input mode. ground noise out of the mic to keep from
ham, it could be right up your alley. It sending that noise, along with the
includes going into a special mic circuit About FLdigi FLdigi message, to the transmitter.
to bypass what the mic normally does, First let me explain just a little of what My first thought was to buy a box that
to use it for a direct data connection to FLdigi is. FLdigi is a computer program would hook up my computer to my
run FLdigi. But I found that everything I that allows one to use the sound card Yaesu FT-8900 radio. This would cer-
wanted to do could be done with parts I of a computer in order to send and tainly be easy to do, but then I looked
had on hand. For the most part, these receive digital communications wher- around my radio and electronics work
are electrical, not electronic, parts. I ever the FCC rules allow. In this case, rooms. I had a boatload of basic parts
used two switches, two 3.5-millimeter we’re using VHF frequencies, but oth- here, so I got the idea that I should see
stereo audio sockets, one 1-megohm ers have used this program to commu- if I could use some of these parts I’ve
resistor, and one 0.1-μF capacitor. Also, nicate on HF as well. The messages collected over the years to make some-
one empty dental floss box and one sent can be written words / forms, or thing that works. I figured it wouldn’t be
empty Altoids® tin. In all, I used far fewer data files like small low-resolution pic- pretty, but if it worked, I’d really love
electronic and mechanical parts / con- tures. There may be cables and boxes being able to say, “I did it my way.”
nectors than I expected. Also needed out there that can be purchased for your The first thing I attempted was to find
was a 3.5-mm mono-to-stereo convert- radio to do this type of communicating out which two wires coming from the mic
er for the audio from the transceiver to (my preference was to roll my own). For into the radio would be needed to put
more information on FLdigi, you can the computer FLdigi noise directly into
* Email: < ke3fl@yahoo.com> read articles about it on the web or you the radio. The Yaesu uses a CAT 5
Website: <http://cs.yrex.com/ke3fl> can peruse the FLdigi beginner’s User’s eight-wire connector, and I wanted to
MITY GO-BOX
9 to 20 Ah LiFePO4 Battery
Powerpole Port - DVM - USB Charger
I
t never ceases to amaze how ama-
teur radio operators use a diversity
of existing communications systems
to keep mentally active during periods
of low sunspot cycles and especially
during the COVID-19 lockdowns. Take
for example, a number of Ham Cam
International1 ham radio operators
located on the Isle of Man and in
England who decided to build and run
their own ADS-B ground stations that
can be installed anywhere and receive
real-time data directly from airplanes on
their computers.
By doing so, they join tens of thou-
sands of individuals, some hams, some
not, who track aircraft by detecting and
analyzing their digital transmissions as
they fly within receiving range of their
location. This data is also distributed
throughout the aviation industry by the
Photo A. L-R: Raspberry Pi, RTL SDR receiver, 1.090-GHz antenna
“FlightAware” organization as an elab-
orate information tool. There are over
30,000 ADS-B receiving stations in 197
countries providing this information.2
Interest to Hams?
You may ask: “How is this of interest to
amateur radio operators?” Fair enough.
For starters, it provides valuable edu-
cation about communication technolo-
gy in the low microwave bands. Hams
are able to detect and analyze 1.090-
GHz transmissions, learn about the
characteristics of that frequency (re-
member, there’s a ham band close by
at 1240-1300 MHz), what antenna is
best-suited for reception and assemble
the equipment necessary to receive
* Email: <k3beq@verizon.net>
# Email: <gd0nfn@gmail.com> Photo B. L-R: 5.2-volt, 2.5-amp power supply, Micro SD card reader, Micro SD card
The locations of aircraft within your receiving range will display on a map on
your computer (Figure 1). You can also track the number of flights tracked by your
More Watts per Dollar
SM
receiver by distance on a daily basis (Figure 2).
Summary
Experimenting has always been a part of the amateur radio community. Exploring Transmitting &
enables us to educate ourselves in new avenues of communications whether it is
directly or indirectly related to our hobby. Whether you live close to an airport or in
“flyover country,” you can track passing aircraft and hopefully have fun doing it.
Audio Tubes
®
COMMUNICATIONS
BROADCAST
INDUSTRY
AMATEUR
Immediate Shipment from Stock
Phone: 760-744-0700
Figure 2. The coverage graph shows the aircraft positions reported by distance Toll-Free: 800-737-2787
from the receiver. The majority of reports are from stations receiving data from (Orders only) 800-RF PARTS
aircraft 50-150 miles from the receiving station.
Website: www.rfparts.com
Notes: Fax: 760-744-1943
1. See Green, “Streaming Video Over Internet Protocol for Radio Amateurs,” CQ February
2021, p.52
888-744-1943
2. See <https://en.wikipedia.org/wiki/FlightAware> Email: rfp@rfparts.com
3. As a thank you from FlightAware, users sending ADS-B data receive the following:
• Live data on flightaware.com (subject to standard data processing delay of up to 2 minutes)
• Access to up-to-the-second live data received by the local device (accessible from the stats
page with a local network connection)
• Data from local device highlighted on FlightAware track logs
• Detailed statistics on site performance
• A free Enterprise Account (USD $89.95/month value)
• To claim benefits, go to Section 5 of “How to Build a PiAware ADS-B Receive”
Y
ou’re enjoying a friendly QSO with a fellow ham across
the continent. QRN is down, signals are strong, and
copy is easy. Then — all of a sudden — everything
shuts down. No lights, no air conditioning, and no signals.
What on Earth!? Simple, but painful: A utility outage. Forty
minutes pass with no AC coming into the shack. This doesn’t
happen every day, but this time Murphy’s Law reigns
supreme. The QSO is busted, and your friend is left won-
dering where you got off to. Worse yet, when the utility power
returns to normal, instead of hearing signals, you hear only
the hiss of electrons running around pointlessly. Something
in the receiver got fried by a voltage transient. Aargh! Can
anything be done? Read on…
CQ Communications, Inc.
Phone: 516-681-2922
http://store.cq-amateur-radio.com
Announcing:
2022 CQ World Wide WPX RTTY Contest
February 12-13, 2022
NEW! Starts 0000 UTC Saturday; Ends 2359 UTC Sunday
Youth
y
Categor Log Deadline: 2359 UTC February 18, 2022
Announcing:
2022 Nominations Open for the CQ Amateur Radio,
DX, and Contest Halls of Fame
E
ach year CQ recognizes those who have made Please include your name and contact information as well.
significant contributions to amateur radio in gener- Email to <hall-of-fame@cq-amateur-radio.com> or mail to
al, and to DXing and contesting in particular, cre- CQ Amateur Radio Hall of Fame, P.O. Box 1206, Sayville,
ating three categories of awards. Nominations for all three NY, 11782. The official nomination form is on the CQ web-
Halls of Fame open on January 1, 2022 and will close on site <www.cq-amateur-radio.com>. Please indicate in your
March 1, 2022. email subject line for which hall of fame the nomination is
being submitted.
CQ Amateur Radio Hall of Fame
Amateur radio operators have been responsible for many CQ DX and Contest Halls of Fame
advances in communications technology, and entire indus- Nominations for the CQ DX Hall of Fame and the CQ Contest
tries have been built on the foundation of amateur radio exper- Hall of Fame recognize those amateurs who have made
imentation and activity. In an effort to recognize outstanding major contributions to DXing and contesting, respectively.
amateurs and their achievements, and help the public appre- The activities and accomplishments that qualify one for mem-
ciate the far-reaching and longstanding value of amateur bership in these elite groups involve considerable personal
radio in our society, we have established the CQ Amateur sacrifice and can usually be described by the phrase “above
Radio Hall of Fame. Nominations for the 2022 “class” are now and beyond the call of duty.” Nominations for the Contest and
open. Members of the 2021 “class” were announced last May DX Halls of Fame may be made by clubs, organizations, or
and appeared in the July issue of CQ. individuals, and must be submitted by March 1 of each year
The CQ Amateur Radio Hall of Fame honors those whose to be considered.
technical or other accomplishments have helped propel ama- A maximum of two (2) people may be inducted into each
teur radio forward, or whose achievements in other areas of hall of fame (DX and Contest) each year. Nominations for the
life have helped improve ham radio’s reputation simply CQ Contest and DX Halls of Fame should be directed to CQ
through association. Nominees for the CQ Amateur Radio DX Hall of Fame or CQ Contest Hall of Fame, P.O. Box 1206,
Hall of Fame will be judged on the basis of qualifying in one Sayville, NY 11801; or via email to <hall-of-fame@cq-ama-
of two broad areas: Those individuals — whether licensed teur-radio.com>. Please indicate in your email subject line
amateurs or not — who have made significant contributions for which hall of fame the nomination is being submitted.
to the amateur radio hobby; and those radio amateurs who If you feel someone has earned this recognition, please
have made significant contributions to society in general. submit a nomination. Please don’t assume that someone else
Nominees must have made significant contributions of will nominate the person you may have in mind. Nominations
nationwide or worldwide impact. from past years will not automatically be carried over.
Nominations for the Amateur Radio Hall of Fame may be We plan to announce this year’s selections in May. Please
made by clubs, organizations, or individuals. State your can- help us recognize these “ham radio heroes” whose contri-
didate’s name, where to contact him/her if still living, for which butions have helped shape our hobby, our nation, or our
category you are nominating him/her, and a brief one- to two- world. Remember, the nomination deadline for all three CQ
paragraph description of this person’s accomplishments. Halls of Fame is March 1, 2022.
T
wenty-two years ago, we projected what we thought electrons could be controlled, everything up to and including
the future of our technology would be. Well, 22 years color television was possible. Even basic computers were
later it’s time to take another look! If the problems we manufactured at the time, albeit with a myriad of vacuum
agonized over for the past two years (Covid 19, political tubes but they did “calculate” nevertheless. In 1948, at Bell
unrest, and global warming) have not destroyed our civiliza- Labs in New Jersey, the transistor was developed and the
tion (as we know it) by the time you read this, the new year age of solid-state physics was born. This was another fun-
will be “just around the corner.” Since this is a time when damental discovery of the magnitude of the vacuum tube and
many people consider and predict the future, not to be out- the future shape of electronics would never be the same.
done, I would like to continue to present my point of view of Filament power was eliminated, the size of the amplifying
the technology to come as well as review how our thoughts element was reduced by magnitudes and the eventual out-
have either changed, remained the same or reversed. To growth was the integrated circuit. While the frequency
understand what I base my views on we must first consider response for vacuum tubes did eventually extend into the
where we have come from. GHz range, noise figures and costs were high. Today the
The growth of technology during the start of the 20th cen- transistor has made GHz operation at almost theoretical
tury has certainly been outstanding. In 1900, Marconi was noise figures an everyday occurrence (with devices that cost
first thinking about radio transmissions. The Wright brothers a dollar or so) which brings me to my first prediction. I believe
had not yet flown and horse-drawn vehicles were clogging that solid-state physics as we currently employ it will be
our roads, not the automobile. If you were fortunate enough replaced (or at least supplemented at some point during the
to have a wind-up Victrola, you could listen to recorded music late 21st century) with something else. Once frequencies of
on shellac coated disks and cylinders, but even the simple hundreds of GHz need to be routinely handled to accom-
vacuum tube had not yet been developed. The great Thomas modate our growing need to rapidly transfer vast amounts of
Edison dismissed the one-way flow of electrons from a fila- data, basic physics comes into play and the physical size of
ment to a metal plate in a vacuum as interesting (he dubbed the conventional electronic switch, amplifier or gate (as we
it the “Edison Effect”) but not of much use to help prevent know it) limits the maximum speed that it can operate at. I
blackening of the glass in his new electric lamp. Even basic believe, however, that we will learn how to switch, amplify
electrical service to many homes was rare. During the next and process light inexpensively the way we now do with con-
100 years, however, we would see the development of vac- ventional high frequencies or perhaps something else even
uum tube and then solid-state electronics, television, the air- more remote will suddenly be discovered that will do the job.
craft and space industry, orbiting satellites, nuclear physics, Remember, before 1895 (Marconi’s first transmission) the
the laser, the entire field of opto-electronics, the micro- entire field of wireless was only a mathematical equation on
processor and the computer revolution, both in hardware as James Maxwell’s desk and by 1903 the Atlantic had been
well as software. In 1900, predictions of where we would be spanned! Who knows what other equations or theories exist
in the year 2000 would fall far short of the mark. Even as late on someone’s desk today?
in the century as the 1939 World’s Fair, predictions of where As I said 22 years ago, the shrinking of electronic circuitry
our society would be, technologically, in the 1960s and ’70s has continued and we now have chips containing millions of
were not particularly accurate. transistors (in some cases). A great deal of current design is
Furthermore, only 35 years ago, the mass computer revo- with complete functional blocks as well as microprocessors
lution was just a dream in some minds and four-function cal- and software has become as important as standard elec-
culators were as close as we came to the state of the art. tronic circuit design. Along these same lines, external com-
The slide rule was still the sign of the “true engineer” just like ponents are often so small that in many cases they can only
the typewriter was the author’s best friend. The general pub- be interconnected with machines as human hands are not
lic did not even have a clue of what was to come. As a result steady enough to solder them on tiny circuit boards (even
of developments that we don’t even know of yet (but will sure- under microscopes) and only components limited to those
ly come), any specific prediction of where we will be in 2100 required for direct human interface (speakers, microphones,
by anyone, in my opinion, will also fall far from its mark. If switches, displays, power sources, etc.) remain. Along these
you still doubt this statement, a book previously offered by lines I still believe, as I did then that the use of basic com-
the New York Metropolitan Museum of Art entitled ponents such as resistors capacitors, diodes, etc. will dwin-
“Yesterday’s Tomorrows” is still available you should get or dle even more as the 21st century progresses and that a new
borrow a copy and read it. This book will give you a very good way of implementing electronic designs will come about.
idea of how future predictions (made in the early 20th I am sure that the physical size of power sources such as
Century) may have captured some of the “flavor” of what batteries (both chemical and solar), fuel cells and the like will
eventually would be but not the essence. continue to shrink to match the new products being devel-
Enough said. In the 20th century, there were some funda- oped. The portable devices I spoke about then, such as cel-
mental developments that shaped the current state of our lular-type communications links, have truly become “Dick
technology. The first was, of course the vacuum tube. Once Tracy wrist radios” (or communicators) with full color motion
video to boot. In some cases, some are actually really fully
functioning wrist sized (or at least pocket sized) computers,
*c/o CQ magazine far beyond simple telephones. I also think that revolutionary
The transmitter
room at the Voice
of America’s
Botswana site.
for anyone with just a passing interest Voz Missionaria via Florinapolis on
in the subject. The only hiccup is the 9665 at 2333 with presumed sermon.
price: A budget busting $46.95. The (Brossell, WI)
Kindle edition, however, is a more real- Radio Brazil Central via Goiania on
istic $9.95, which is a very reasonable 11815 at 2321 with talks. (Brossell, WI)
price for a fun, nostalgic read. CHINA—China Radio International on
A QSL from past pirate Radio Merlin 9675 via Shijiazhuang at 1330 in Russian;
International. Cool as long as he on 13630 via Mali with headlines at 2102.
doesn’t trip over his beard hooking up Listener Logs (Brossell, WI) On 9710 and 11660 via
Rudolph. Your shortwave broadcast station logs Kashi at 2210 in French with short talks
are always welcome. But please be and musical segments to close with sta-
~ The mainland Chinese seem to be sure to double or triple space between tion ID at 2227. (D’Angelo, PA) On 11725
moving away from labeling their domes- the items, list each log according to the via Xiangyang at 1750 in German with
tic services numerically. Instead of station’s home country and include your apparent German-to-Chinese lesson.
CNR-1 through 17, they’re being given last name and state abbreviation after (Barton, AZ)
actual names. Thus, CNR-2 has each. Also needed are spare QSLs, sta-
evolved into China Business Radio; tion schedules, brochures, pennants,
CNR-7 becomes Greater Bay Area station photos, and anything else you
Radio; CNR-14 the Voice of Hong think would be of interest. The same
Kong, and so on. Maybe someday a holds for you amateur radio operators
wizard will come along and sort it all out; who also listen to shortwave broadcasts
for now, it won’t be me. ... I know you’re out there! You, too, are
also most welcome to contribute!
~ Now that we’ve reached December, Here are this month’s logs. All times
things seem to have gone quiet in the are in UTC. If no language is mentioned
GLD shack. Except ... comes now English is assumed.
another new book by a longtime SWBC
DXer. Bruce Churchill has authored ASCENSION—BBC North Atlantic
Radio’s Global Voices, A Radio Relay on 11810 at 2153 on domestic vio-
Journey Across 7 Continents, a two- lence. (Brossell, WI)
part story about listening to exotic radio BOTSWANA—Voice of America (VOA)
stations on the shortwave bands. on 7460 via Mopeng Hill at 0420 with man
Essentially a beginner’s guide, it deals and woman speaking in Kinyarwanda /
with the whats, whys, and wherefores Kirundi. (Barton, AZ) On 15460 at 1544 in
of shortwave. In Part Two, Churchill Hausa. (Brossell, WI)
offers examples of the correspondence BRAZIL—(All in Portuguese – GLD)
he’s had with these stations, ranging Radio Clube do Para via Belem on 4885
from QSLs to letters, schedules, sou- at 0315 and 0330 with a conversation
venirs, etc. This should be a fun book between two men and time pips.
(D’Angelo, PA)
Radio Educacao Rural on 4925 via Tefe
at 1026 with a man talking and Brazilian Half of Bruce Churchill’s new book fea-
*c/o CQ magazine tures mouth-watering QSLs.
music. (Taylor, WI)
by John Figliozzi
Adventist World Radio’s tall towers overlook the Pacific Ocean on Guam.
Cheese Radio on 6935u at 0013 with Zeeky hosting a program of hard rock music.
Radio Irrational International on 6935u at 0052 faded out or something at 0059, sta-
tion ID and off at 0103. Lode Radio on 6970u at 0152 with rambling talk. WFDR on
6935u at 2038 with an FDR depression era speech, off with station ID at 2058. Black
Flag Radio on 6925u at 2131 with Zeeky rambling on about QRP radio, another song
at 0029 and off. Burry Cookie Hour on 5185 at 2332 with pop music, disco, etc., appar- The new, expanded 10th Edition of
ently transmitted through Radio Illumati. (Taylor, WI) John Figliozzi’s Worldwide Listening
Reported in previous columns: Outhouse Radio, Ballsmacker Radio, WTF Guide includes completely updated
Worldwide, Wolverine Radio, Radio Genix. listings of popular radio programs
ROMANIA—Radio Romania International on 13660 at 1545, (not usually heard here) that can be heard using traditional
with woman speaking in Arabic, IS at 1555, then off; on 15340 at 1340 with pop music
in Romanian. (Barton, AZ) shortwave receivers, as well as
SAO TOME—VOA Relay on 7265 via PInheira at 0530 with man and woman speak- today’s newer listening technologies.
ing in French. (Barton, AZ) Program listings are classified by
SWEDEN—IBRA Media / Radio Sama on 15510 via Woofferton at 1830 with man genre and tell you the time of
and woman speaking in Arabic with references to Afghanistan. (Barton, AZ) day and day of the week they are
UNITED STATES—VOA on 17700 via Vatican at 1505 in Hausa with hoarse-voiced on-the-air, and how to find them on
man reading the news. (Taylor, WI)
VOA/Deewa Radio on 12035 via Thailand with man and woman speaking in Pashto. your shortwave receiver, WiFi
(Taylor, WI) radio, computer, and other listening
Radio Liberty (RFE/RL) on 15310 via Woofferton at 1457 in Uzbek with alternating devices.
man and woman talking. (Taylor, WI)
Radio Farda on 12005 via Woofferton at 1700 in Farsi with pops and time pips at This new edition updates and reviews
the bottom of the hour. (Barton, AZ) all of the ways programs can be
Adventist World Radio on 15490 at 1645 with a long monologue in Tigrinya. (Barton, heard– “live,” on-demand, WiFi,
AZ) On 17570 via France at 1632-1659* with man speaking in Somali, vocals, anoth- podcast, satellite, internet, digital and,
er man giving a religious talk. (D’Angelo, PA) of course, analog AM, FM and SW.
Supreme Master TV on 5900 via Okeechobee at 0020 with many station IDs, talk
segments hosted by male and female announcers. (D’Angelo, PA) Spiral-bound to open in a flat, easy-
VATICAN— on 15565 with a choir to sudden close at 1727. (Barton, AZ) to-use format.
Back in the Day
~ Armed Forces Radio / AFRTS on 4319 via Diego Garcia at 2233 on January 9,
AVAILABLE NOW!
DAY!
2006; also on 7811 both in USB mode with AFRS programming. ORDER YOURS TO
Thanks for Your Logs $29.95 + shipping
With immense gratitude, I thank the following reporters: William Hassig, Mt.
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Until next month ... Keep on keepin’ on, and ... Celebrate Shortwave! www.w5yi.org
CQ 1-22
A
s things begin to open up, it is
good to see our in-person ama-
teur radio events also resuming.
Pacificon is one of those annual events,
and I’ll have more on it in a future col-
umn. This month’s kit was one sold by
the CalQRP group to promote interest
in the Friday and Saturday evening
QRP gatherings at Pacificon. Those
wanting to participate in the QRP
events were given an opportunity to
purchase a low cost 40-meter regener-
ative receiver kit to be assembled at
home and brought to the convention
where a companion QRP CW trans-
mitter would be built in a group setting.
The Sputnik 40 is a simple, yet
very sensitive receiver originated in
Romania by Ciprian Popica and modi-
fied by KI6DS for use at Pacificon.
When I first saw my kit, I wondered if it
would have enough sensitivity to allow
for QRP-to-QRP QSOs. My test results
showed it could easily hear signals at The Sputnik 40 PC board ready to begin assembly.
as low as 1 μV of signal. The circuit
revolves around the use of a three-sec-
tion toroidal transformer which includes
both coupling and the “tickler” that
allows for regeneration. As in all regen-
erative receivers, this one can receive
CW, SSB, and AM.
A few weeks before the gathering in
California, the kits were sent out. The
tuning is controlled by a 10-turn poten-
tiometer varying voltage to one or two
varicap diodes. There are also trimmer
capacitors to help in centering the tun-
ing range to cover the 40-meter band.
There are a few modifications written
that are incorporated into the latest ver-
sion of the instructions, and most have
to do with the speed and range of the
tuning circuit. My kit came with a small-
er version of the voltage regulator. The
holes for it are rather close together, so
I had to be very careful mounting it.
Later, I realized I could have spread the
leads out and used the larger set of
holes meant for the larger regulator.
There are no surface-mount parts, but
the toroid takes some time to wind and
must be done exactly as shown and
described in order for the regenerative
circuit to work. As mentioned in the
The three legs of the voltage regulator are very close togeth-
er on this PC board. Be sure to check for shorts between
close leads like these before powering a kit for the first time.
WHAT’S NEW
PreppComm Introduces New S2X Stand
PreppComm, a new U.S.-based manufacturer of the DMX-40,
a combination CW decoder and transceiver, has introduced a
stand that makes it easier to see and touch the LCD screen on
its flagship product.
The S2X Stand, which is composed of two separate legs,
each with two rubber feet, snaps onto your DMX-40 case bot-
tom, and holds the DMX-40 at a 45° angle. PreppComm said
that the new stand for the DMX-40 is available now and and
has a suggested retail price of $4.95.
PreppComm has also debuted its new online store <http:// A transistor is in place and ready to solder. The extra hole
preppcomm.com>, which has moved from a WordPress web- was incorporated into the PC board design in case a metal
site using Shopify for e-commerce entirely to Shopify, with a can type of the 2N3904 transistor was used instead of the
new look. PreppComm said the new website will help it add plastic case version.
more accessory products in the future.
i705
HF / 6M / 2M / 70CM
i7610
HF / 6M SDR Transceiver
ZZZLFRPDPHULFDFRPDPDWHXU
sales@icomamerica.com
©2021 Icom America Inc. The Icom logo is a registered trademark of Icom Inc.
All other trademark remain the property of their respective owners.
$OOVSHFLÀFDWLRQVDUHVXEMHFWWRFKDQJHZLWKRXWQRWLFHRUREOLJDWLRQ For the love
PERIODIC TABLE
OF SELECT
AMATEUR RADIO
CONTESTS
2022
All Your Contesting Needs
i9700
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of ham radio.
CQ WW
QRP: Low-Power Communications
BY R. SCOTT ROUGHT,* KA8SMA
QRP is Contagious!
I
am pleased to share with my fellow hams that the QRP
bug has struck again. Andy Ruggiero, WD8BWW, owner
of Mid-America Technology, Inc. (a radio design / repair
and electronics technology company), recently discovered
the power of QRP while troubleshooting transmitting issues
on my Yaesu FT-817 QRP transceiver. Regular readers of
this column know that I have a sweet spot for my FT-817. I
purchased this radio as soon as Yaesu introduced it over 20
years ago and until spring 2020, the FT-817 was my prima-
ry transceiver both in the shack and on the trail until I began
having intermittent issues with the transmitter. I concluded
that after many years of contacts, the finals (original MOS-
FET transistors) were going kaput. I had too many other radio
projects going at the time, so I shelved the radio until I had
time to make the needed repair.
Nearly a year and a half later, I decided to repair the FT-
817; however, rather than do the work myself, I sent it to
Andy who had done an excellent job making repairs to this
radio a few years ago and I knew that installing new finals
would be a simple task for him. Besides, I learned not too
long ago, after installing a bhi DSP noise cancelling module Photo A. My “suitcase-style” Bayou Jumper spy radio littered
(NEDSP1061-KBD) inside this radio, that fat fingers, poor with vintage travel stickers.
eyesight, and a small working area generate a lot of stress
for me, so I decided to send the FT-817 to a professional.
Andy contacted me the same day he received the trans- FT-817 at 5 watts output (rubbing a little salt into my wound
ceiver and — to my surprise — informed me he could not – HI). He was excited as could be and noted to the other ham
find anything wrong. He said the transmitter checked out at that this was his first QRP DX contact. I think everyone in the
5 watts on full power with no reduction in power after keying QRP community can remember the thrill of their first contact
down the transmitter for several seconds, the power ampli- with only a few watts, but I admit the thrill of watching some-
fier board appeared fine, and no issues were identified with one else making their first QRP DX contact is greater.
the components, solder joints, etc. In other words, the trans- Unbeknownst to Andy, this was also a first for my FT-817.
mitter was fine. Although I had made thousands of DX contacts with this radio
I was dumbfounded. over the years, this was the first time a DX contact (SSB or
I always practice short tune-ups when using an antenna CW) was made using its power set at 5 watts. I always run
tuner for non-resonant antennas and do the same when the radio at 2.5 watts. I contacted Andy after reviewing the
checking SWR on resonant antennas. While chatting, I men- video and congratulated him on the QRP contact and asked
tioned that the FT-817 had never been connected to a 13.8- him how much I owe him for the bench fee and further check-
volt power supply and that I have historically used a gel cell ing the radio. Andy told me “no charge for my time — the
battery (12-volt 7-amp hour) to power the radio. As soon as thrill of working Rome with 5 watts on an end-fed wire anten-
he heard me say I used an external battery to power the na was more than enough.” This was a double-win for me
radio, he zeroed in on whether my intermittent transmitting since I may have lured another ham into the world of QRP
issues could be related to the battery, not the radio. My jaw and as embarrassing as it is, I learned (the hard way) that
dropped when he asked about the battery as I had not test- my FT-817 never had an issue. I will call the latter a win since
ed it before shelving the radio. Unfortunately, this gel cell bat- it did not cost me anything – HI. Lesson learned — always
tery went to the recycling center after I upgraded to lithium- check your power supply before jumping to conclusions and
iron phosphate batteries last year, so I had no way to check troubleshooting radio gear.
if the issue stemmed from the battery. Since we were unsure
of the problem, I told Andy I’d pay for his time to further trou- Bayou Jumper – Finished!
bleshoot and play with the radio to determine if he could repli- In the October column, we heated up the soldering iron and
cate my findings. assembled the Four State QRP Group’s Bayou Jumper, a 40-
Later that evening, I received an email from Andy indicat- meter QRP CW transceiver kit that pays homage to World War
ing he could not identify any issues with the transceiver and II-era Paraset spy radios. As promised in the last column, I
that the problem was likely related to my battery. He also have included two photos of the finished product. I stained the
asked me to watch a video he had attached to the email. case light maple and purchased stickers from an online store
When I opened the video I saw that Andy had filmed himself to decorate (with a little help from my XYL) the exterior of the
making a SSB contact with a ham in Rome, Italy using my case (Photo A). Photo B shows the interior of the case with a
military intelligence logo on the inside cover. I laser printed the
*<ka8sma@cq-amateur-radio.com> logo onto water-transfer decal paper (available online and in
L
ast month, we looked at capacitors
and capacitance as part of my
“junk box” article series (Photo A).
This month, let’s look at inductors and
inductance. According to the website
Electronics Tutorials <https://tinyurl.
com/2sra88us>, “an Inductor is a pas-
sive electrical component consisting of a
coil of wire which is designed to take
advantage of the relationship between
magnetism and electricity as a result of
an electric current passing through the
coil.”
Readers may recall that whenever
electrical current flows along a conduc-
tor, a magnetic field is generated. This
is a very useful electrical phenomenon
because this physical property is a pri-
mary reason electronics exists. Res-
onant circuits, power supplies, tuned cir-
cuits, transmitters, receivers, antennas,
Photo A. A varied assortment of inductors found in a junk box. (Illustrations cour-
phones, televisions, just about anything
tesy of Wikimedia Commons, except as noted)
electronic depends on inductors.
Steve Werner, AG4W (“A Journey to the Moon and Back,” p. 11) of Huntsville,
Alabama, is a DXer and contester who was looking for new challenges after he pret-
ty much “worked them all,” so he set his sights on the ultimate DX — Earth-Moon-
Earth, or EME DXing, in which every contact covers a distance of roughly half a mil-
lion miles. He tells us how he tried to start small.
Alan Davidson is President Biden’s Charles E. Scharlau, NZØI (co-author “Arducon,” p. 22), was first licensed in 1974
nominee to head up the FCC-equiva- as WN5MIY, and currently serves as USA ARDF Co-coordinator. He has been active
lent for federal government spectrum in Amateur Radio Direction Finding since 2000. He represented the USA at the ARDF
users, the NTIA. (U.S. Commerce World Championships in 2004, 2006, 2008, and 2010. Professionally, Charles spent
Department photo) 26 years working in both hardware and software positions in aviation, maritime, and
cellular communications industries. He holds a BS Physics degree from the University
of Arkansas at Fayetteville, and an MSEE degree from the University of Colorado at
The President also nominated attor- Boulder. Charles can be reached at <nz0i@openardf.org>.
ney Gigi Sohn to fill a vacant seat on the Co-author Gerald Boyd, WB8WFK, was first licensed in 1975, and currently serves
FCC. She is currently a Distinguished as USA ARDF Co-coordinator. Jerry has been active in the development of Radio
Fellow at the Georgetown Law Institute Direction Finding (RDF) equipment and techniques since the early 1990s. Jerry rep-
for Technology Law and Policy and pre- resented the USA at the 2004, 2006, and 2010 ARDF World Championships. He has
viously served as a counselor to former designed custom RDF receivers, directional antennas, and transmitters for use in
FCC Chair Tom Wheeler. Much of her ARDF competitions and receivers for search-and-rescue for locating downed aircraft
work has been in advocacy for Emergency Locator Transmitters (ELTs). Jerry currently holds an Extra Class license
widescale broadband access. The and has worked professionally in the aerospace industry for over 41 years. Jerry can
White House notes that, if confirmed, be reached at <wb8wfk@icloud.com>.
Sohn would be the FCC’s first-ever
Martin Butera, PT2ZDX/LU9EFO (“PY2GN: Brazil’s First Public WebSDR Station,”
openly LGBTQ+ commissioner.
p. 26), is from Argentina but currently living in Brazil, where he has been visiting and
Mr. Biden also nominated Alan David- writing about some of the country’s premier ham radio installations. This is his sec-
son to head up the Communications and ond article for CQ.
Information division of the National
Telecommunications and Information
Administration. NTIA is the FCC’s coun-
terpart in terms of spectrum manage- The Shortwave
ment for federal agencies, including the
military. This is significant to hams
because many of our bands are shared
Propagation Handbook
with federal government users. Davidson 4th Edition
was the first Director of Digital Economy
at the Commerce Department, which is 208-page Paperback—Only $42.95
NTIA’s parent agency. He is currently Book on CD—$32.95
Senior Advisor to the Mozilla Foundation,
Buy Both the Paperback and CD—
and previously served as the open-
access software group’s Vice President Only $61.95
of Global Policy, Trust and Security. Plus applicable shipping!
Before that, he worked for Google, where
he was the company’s chief lobbyist in CQ Communications, Inc.
Washington between 2005 and 2012. All Phone: 516-681-2922
three nominations are subject to Senate http://store.cq-amateur-radio.com
confirmation.
Haywire State
A
nyone who’s been around the analog business more
than a few weeks is (hopefully) familiar with the late,
legendary Bob Pease <https://tinyurl.com/fcvzt8x4>.
Bob was one of my mentors from afar, and just about every-
thing I know about solid-state anything, I learned from read-
ing his countless Pease Porridge columns in Electronic
Design magazine. The fact that he looked like Moses only
enhanced his authoritativeness.
Perhaps one of the most famous photos from Bob’s
archives was on the cover of his book, Troubleshooting
Analog Circuits1 (Photo A). That’s an actual functioning cir-
cuit in front of him (an operational amplifier, I believe).
Although I have not achieved this level of … whatever it is
… I am well on my way. Photo B shows my workbench in its
current state. At least I think this puts me in good company
with Mr. Pease. I am also reminded of that most informative
passage from the ancient book of Proverbs: “Where no oxen
are, the crib is clean: But much increase is by the strength
of the ox.” (Proverbs 14:4).
If the state of one’s crib is any indicator, as suggested
above, my bench should be a powerhouse of productivity.
Oh, to be sure, I occasionally neaten things up between
active projects, (though my attempts at inventing a self-
cleaning bench have all failed miserably), but I find much
more inspiration from such works in progress than from a
sterile, organized workbench, as do many others of my ilk.
Speaking of ilks, I’ve discovered that non-creative, non-
inventive types just don’t understand unfinished products.
Whether you’re a painter, a potter, or a programmer, there’s
going to be a stage (or even an era), where the thing you’re
working on is going to be in a haywire state, not even rec-
ognizable for what it is … or likely to become.
Wilbur and Orville Wright were not in the least encumbered
by any pre-conceived notions of what an airplane should look
like. They did everything backwards. The elevator was in the
front, and the props were in the back. Though they did every- Photo A. The cover of the late Bob Pease’s book, Trouble-
thing “wrong,” the thing flew. shooting Analog Circuits, published by Elsevier, shows him
Actually, they didn’t get everything wrong. The super high- checking out a “haywire” circuit on his bench. (Photo of auto-
tech military Gray Eagle drone has a pusher prop … it keeps graphed cover courtesy of Kirt Blattenberger, KB3UON, of
the prop wash away from the flying surfaces, giving it a much RF Café <www.rfcafe.com>)
better aerodynamic efficiency and longer range. Maybe the
Wright Brothers knew about this … or maybe they didn’t. No
matter; they forged ahead the best they could, and the rest
is history. Now, while every great creative enterprise has to pass
One of Bob Pease’s great quotes is, “My favorite pro- through the haywire state, it doesn’t have to stay there.
gramming language is solder.” There is so much truth in this Mr. Pease’s famous breadboard eventually ended up in
statement. You can do all the circuit modelling you like, but the form of a commercial op-amp chip (I forgot which one).
sometimes the only viable solution is to solder it together and One of my great joys is to see one of my creations even-
see what smokes. This is especially apropos when working tually packaged in a non-Frankensteinian form that won’t
with analog circuitry, particularly at higher frequencies. scare visitors right out of the shack. I always appreciated
Digital circuits, as a general rule, either work or they don’t. Heathkit’s “fit and finish” and use it as sort of a benchmark
Analog circuits can have continuous states of performance for my projects’ final forms. Their cabinets were works of
ranging from “sort of works” all the way up to “exceeds all art, and immediately recognizable three-quarters of a cen-
performance specifications.” tury after the fact. But even better, the builder of a Heathkit
got to see the product in a haywire state, up to the time it
*3763 Lyle Avenue was lovingly inserted into its final Heath green cabinet.
North Pole, AK 99705 (Johnson also offered many of their transmitters in kit form,
email: <kl7aj@cq-amateur-radio.com> a slightly less known fact; I have a kit-built Johnson Ranger
WA5VJB was unable to complete his column for this issue, so we once again asked W1IS and
KC1DSQ to fill in. This time, Bob and Bob were trying to optimize an end-fed half-wave antenna
for multiband use when they realized that the antenna's basic design assumptions had not
been closely examined in decades. Here are the results of their research. - W2VU
V
irtually all hams know dipole
antennas for their simplicity and
the fact that the impedance of a
dipole, about 70 ohms, is a good match
to our commonly used 50-ohm feed-
lines. A dipole is most likely the first HF
antenna that most of us still use. Over
time, we learn about other configura-
tions like the Off-Center-Fed, or OCF1,
multiband dipole whose impedance of
around 200 ohms doesn’t match our
coax and needs a balun to provide a
match. If you can feed a dipole from a
point off-center, why can’t you feed the Figure 1. Single-band end-fed antenna.
antenna from the end?
You can, of course, but we need to
start with some basics about antennas.
10' 8''
1:1
Coax
Wire Counterpoise
The antenna with wire counterpoise is shown in Figure 3. Photo B. (1) PC board with load; (2) Silicone-potted load;
The lengths shown are for #14 Flexweave from RF Davis or (3) Load mounted on an insulator.
#14 THHN wire from the local home improvement store. The
total length of the radiator is 136 feet 6 inches. The distance
from the feedpoiint to the load capacitor is 43 feet 8 inches.
The load capacitor is 150 pf. Its voltage and current require- Photo D. Isolation of the transformer from the 1:1 balun in
ments depend on the design power as shown in Table 2. separate boxes coupled together with a dual PL-259 con-
Because the capacitor is out in the elements and is likely nector to avoid unwanted coupling to the feedline.
to experience high-voltage static build up, we protect it by
placing a resistor across it to drain built-up static charge while C or use two separate boxes coupled with a dual PL-259 cou-
handling the voltage and power it experiences in operation. pler, Photo D.
For less than 500 watts, a 1-megohm, 1-watt, non-inductive
resistor works well. For higher power levels, a 2-watt, 2.7- Coax Counterpoise
megohm non-inductive resistor is needed.
Mounting the capacitor and resistor on a 1- x 1-inch PC The coax counterpoise is shown in Figure 4. This is basical-
board makes assembly and potting easier, especially for the ly the same antenna as the wire counterpoise version with
high-power surface-mount parts. These are large surface- the wire removed and the 1:1 balun in a separate box placed
mount parts that are easily soldered to a 1x1 PC board with 13 feet, 2 inches down the feedline. The outer surface of the
a slot cut out of the middle with a Dremel tool, as shown in coax shield serves the counterpoise and the 1:1 balun / choke
Photo B(1). Further, though not absolutely necessary, we like constrains RF from flowing on the rest of the feed line. Thus,
to protect our capacitor and resistor with a layer of modeling the 1:1 position defines the length of the counterpoise and
silicone or a non-conductive epoxy coating, as shown in prevents feedline radiation below it. We were able to achieve
Photos B(2) and B(3). comparable performance with both counterpoises.
The wire counterpoise is 13 feet 2 inches long and will inter-
act with the feedline if it gets too close, so we ran it horizon- The Matching Transformer
tally for 30 inches before allowing it to droop towards the The matching transformer is fundamental to building a truly
ground. The wire should be stabilized to maintain a constant multi-band end-fed antenna. It determines the match on all
distance between it and the feedline and other objects, mak- bands and limits the amount of power the antenna can safe-
ing isolated coax a more desirable configuration. The match- ly handle. The design of the matching transformer starts with
ing network is a 36:1 transformer followed by a 1:1 balun4 the parameters of the core material to determine:
with at least 30-dB isolation to suppress common mode cur-
rents. In order to reduce the interaction between the match- 1. Impedance of the primary at the lowest frequency. Too
ing transformer, the two coils should be separated as in Photo low and there will be a mismatch and high SWR. The imped-
BUDDIPOLE
POWERMINI 2
Compact Portable DC Power Management
System with built-in Solar Controller.
13' 2''
Coax
1:1
Coax
ance is determined by the type of core material, number of ty. An 80-meter test antenna was launched to validate our
cores, and the number of turns. modeling and learn the peccadillos of the high-impedance
2. Losses are determined by the resistance of the wire feed. We placed temperature-sensitive strips on the cores to
and core losses. Core losses are a function of the materi- measure the highest temperature reached under continuous
al and the flux density. Flux density is proportional to the power for 1 minute at powers proportional to the power-han-
number of turns and the current in the wires, making fewer dling capability of each of the transformers, calculated from
turns desirable. the loss tests. We also used each of the transformers on-
3. Heat. Losses show up as heat in the core/s, limiting the
power that the transformer can handle. Also, if you overheat
the core beyond its Curie Point (a temperature at which a Low Medium High
material’s magnetic properties change sharply), it will fail and
Digital 50 250 400
recover as the temperature decreases.
CW 100 500 800
We built and tested several transformers to find the most
effective match with the widest bandwidth by testing them SSB 150 750 1,200
with resistive loads. We then measured the losses in each
of the transformers to determine their power-handling abili- Table 3. Power ratings for three transformer configurations.
Parts List Photo F. Transformer for medium power (750 watts): Two
240-43 cores, wire counterpoise.
175 ft, #14 stranded wire, Davis RF or THHN from home
improvement store
1 – End insulator for coax counterpoise
2 – End insulators for wire counterpoise
1 – Insulator to hold the R-C load PC board
1 – 1- x1-inch PC board
1 – 1-watt, 2.7-megohm non-inductive resistor (high power);
1-watt, 1-megohm non-inductive resistor (low power)
1 – (<750 watts) mica capacitor, 150 pF, CDV16FF151J03F,
Mouser 598-CDV16FF151JO3F
1 – (1.2-kilowatt) ceramic capacitor, 150 pf, 3 kilovolt,
Knowles-Syfer 222523K00151GQTAF9LM, Digi-key 1608-
1588-1-ND
1 – 56 pF 3 kilovolt capacitor, CC45SL3FD560JYNNA, Digi-
Key 445-15996-ND
Cores:
1 – (<150 watts) 140-43 core, FairRite, 5943002701, Mouser
623-5943002701
2 – (<750 watts) 240-43 cores, FairRite, 5943003801,
Mouser 623-5943003801
3 – (<1200 watts) 236-52 cores, FairRite, 5952003801,
Photo G. Transformer for high power (1,200 watts): Three
Mouser 623-5952003801
236-52 cores, coax counterpoise.
1:1 Balun choke (see Balun Basics3):
#18 Polyamideimid solid copper wire, Remington Industries, the-air for ragchews, DX chasing, and CQ contests in both
18H200P.12, <remingtonindustries.com> CW and SSB.
Potting - Silicone – see text, or MG Chemicals, 834FX, black, The 1-minute test is a good proxy for digital operation. The
flexible, thermally-conductive potting compound, Amazon.com losses show up as heat that can make the box housing the
Box vent, Amphenol, VENT-PS1YBK-N8001, Mouser 523- transformer get quite hot5. For example, a transformer with
VENT-PS1YBKN8001 a loss of 0.5 dB with 100 watts applied dissipates 12 watts,
Transformer box, Thomas & Betts E989NNJ PVC molded and driven with 1 kilowatt dissipates 120 watts, a lot of power
screw cover junction box, 4-inch x 4-inch x 2-inch, Carlon or to get out of a small box. So we use Amphenol Vents to
Awclub 4.52-inch x 3.54-inch x 2.16-inch both on Amazon improve the heat dissipation from the boxes (see parts list).
8 – 10-24 stainless steel hex nuts (local HW store) Recognizing that the goal of the transformer is to provide
8 – #10 stainless steel flat washers (local HW store)
a high voltage to match the high impedance at the end of the
8 – #10 stainless steel lock washers (local HW store)
2 – #10 ring terminals (local HW store)
antenna, it seemed odd that most transformers were wound
Scotch® outdoor double-sided mounting tape, (local HW with the low impedance primary wires wrapped tightly around
store) a high impedance side of the secondary. Winding wires tight-
ly around each other capacitively couples them, much like a
Kits with pre-mounted and potted capacitors and resistors “gimmick capacitor,” putting an unneeded load on the sec-
are available on the authors’ website, <www.ocfmasters.com> ondary and likely limiting the high frequency response of the
transformer. That is exactly what it does because winding the
Figure 5. A typical set of SWR curves measured with 100 feet of RG-8x on each HF band between 80 and 10 meters (except
60 meters).
7' RG8X
1:1
Figure 6. Dimensions of 40-meter end-fed antenna with coax counterpoise, tunable for higher-frequency bands as well.
SWR on 15 is less than 2:1 across the band. Tuning a wire RF feedback. It is our practice to use another 1:1 balun at
counterpoise is similar, but if the SWR on 10 meters is not the entrance to the shack to suppress any RF picked up by
below 2.5:1 between 28 and 28.5 MHz, adjust the length of the feedline.
the counterpoise. The high impedance affects the tuning We found that we could achieve good positioning of the
because the frequency is more susceptible to surroundings resonances by cutting the length for the high bands and rais-
and environmental conditions such as moisture. The com- ing the lower bands’ resonant frequencies with a capacitive
bined effect means resonances may not be exactly where load of 150 pf at 32% of the length. This worked better than
they are expected, but the bandwidth is wide enough to cover the common practice of cutting the length for the low bands
the variation. A typical set of SWR curves measured with 100 and using a small coil near the end of the antenna to lower
feet of RG-8x is in Figure 5. Note that the low-power version the resonant frequency for the high bands.
works well at two-thirds power on 6 meters while the core We achieved the lowest SWRs by using a 36:1 transformer
loss of the higher-power versions precludes 6-meter opera- and a counterpoise length of 5% of the wavelength at the
tion. Also, any end-fed antenna with a native SWR above lowest frequency. The transformer is the most crucial aspect
2.5:1 should be run at two-thirds power. of the design. The common practice of building the trans-
former with the primary twisted with the first few secondary
How About 40-Meter Multiband or a 60-Meter windings is not the best design. Instead, a transformer with
Single-Band Antennas? the primary centered on the secondary has better high fre-
quency performance. We found that one or two type-43 cores
A broadband matching transformer makes these antennas
worked well for low- and medium-power designs, and that
possible. A 40-meter end-fed (Figure 6) is a simple modifi-
three type-52 cores worked well for high power designs.
cation of the 80-meter antenna made by changing the lengths
The flexibility of using a broadband transformer was
of the wires. The resulting configuration is:
demonstrated by the simplicity of making a 40-meter multi-
band version or a 60-meter single-band version with the
• Total Length: 67 feet
same transformer.
• Distance to 150-pF load: 21.6 feet
All these antennas performed well on the air with no
• Counterpoise Length: 6.6 feet
detectable RF in the shack. We consider the results and per-
• Tuning is similar to the 80-meter version as verified in
formance to be similar to our OCF designs1 with more flexi-
our tests.
bility in deployment while sacrificing only the 60-meter band.
For 60 meters or any single band end-fed half-wave anten-
na, you don’t need a capacitor. Acknowledgements
1. Calculate the length of the counterpoise, wire or coax / We thank our spouses Dee Glorioso, W1MGA, and Barbara
balun, as 0.05% of the wavelength. For 60 meters, it is 3 Rose for their support throughout this long project, along with
meters or 9.84 feet. Colin Brench, W1DJR, and Allison Parent, KB1GMX, for
2. Calculate the length of a half-wave wire, L=468/F; for 60 sharing their experiences with end-feds.
meters, 5.36 MHz, the length is 87.5 feet, but with a 36:1
transformer, the length will be slightly shorter so 87.5 feet is
a good place to start. Adjust the length for minimum SWR at References
5.36 MHz to cover the 60-meter band. 1. “Multiband Off-Center-Fed Dipoles for 160 & 80 Meters,”
Bob Rose, KC1DSQ and Bob Glorioso, W1IS, CQ magazine,
June 2020
Summary 2. “The End-Fed Half Wave Antenna,” Steve Yates, AA5TB,
We found that the wire counterpoise and the coax coun- <www.aa5tb.com/efha.html>
terpoise have essentially the same performance. We pre- 3. Understanding, Building & Using Baluns, Jerry Sevick,
fer the coax counterpoise because it is less fussy mechan- W2FMI, CQ Communications, <https://tinyurl.com/ubw5e9p>
ically and less likely to get tangled in tree branches. For the 4. “Balun Basics: What’s a Balun? Why a Balun? How Do I
wire counterpoise, a 1:1 balun should be used following the Make a Balun?” By Bob Glorioso, W1IS and Bob Rose,
transformer. For the coax counterpoise, the 1:1 balun is put KC1DSQ, CQ magazine, January 2021
in a separate box and positioned on the feedline to define 5. “The End-Fed Half Wave Antenna,” Steve Dick, K1RF,
the length of the counterpoise. This effectively eliminates <https://tinyurl.com/3cdm9jr2>
Editor’s note: We are rearranging our column schedule a K3RWR; James Davey, K8RZ; Bob Johnson, K9KFR;
bit to accommodate a few changes in the lineup. As a result, Steven Franke, K9AN; Andy Bell, KU4XR; Eric Tichansky,
the MF/LF column will now run in March, June, September, NO3M; Paul Kelly, N1BUG; Bill De Carle, VE3IQB; Jay
and December. To give KB5NJD a little breathing room, we Rusgrove, W1VD; and Mike Sapp, WA3TTS.
are pleased to have VK4YB as a guest columnist in this Only on the occasional day were reports missing and that
issue. John will be back in March. – W2VU was probably due to lightning activity in the receiving zone.
Note that all the reports were on the eastern end of the paths.
Repeated efforts to get reports in the opposite direction failed.
F
rom the earliest experiments on 2200 meters, it has Is this a case of one-way propagation? I do not think so.
been known that extremely long-haul DX signals have There is a much simpler explanation. The successful receiv-
been detected from radio amateur stations by other ing stations are operating in the few hours before dawn. This
amateurs. is the quietest time. VK signals making the return trip are
On April 11, 2005, Mike McAlevey, ZL4OL, was able to arriving in the early to mid-evening when conditions in Europe
detect on charts sufficient dots and dashes in the correct are very noisy. This is the same situation with the VK to east-
places to positively identify the source as signals from Laurie ern U.S. path.
Mayhead, G3AQC (SK 2009), at a distance of 19,187.2 kilo-
meters (11,922 miles), a remarkable achievement, which is Can Conventional Multi-Hop Propagation
still the world one-way distance record today. The mode used Explain These Signals?
was DFCW180, which is dual-frequency very slow speed
I do not believe it can. Low-band propagation guru Jim
CW. It takes 3 minutes to send one dot. Nowadays, we let
Hollander, W5EST, has studied these long paths and, even
computers do all the hard work and send signals that are
invoking equatorial anomalies and the like, cannot get the
best decoded by other computers. The best known of these
losses low enough to explain the long-haul signals.
are WSPR (Weak Signal Propagation Reporter) signals. This
Independently, Carl Luetzelscwab, K9LA, has studied these
is a system designed by Joe Taylor, K1JT, and first released
paths and came to a similar conclusion. The signals should
in 2008. In 2021, a new version of the system was released
peter out well before 16,000 kilometers.
by Joe and teammates Bill Somerville, G4WJS, and Steven
Let’s have a look at the actual paths involved. Figure 1
Franke, K9AN, which included FST4 variations which were
shows the great circle route from DL7NN to VK4YB, and
designed with 2200 meters in mind. Whereas WSPR typi-
Figure 2 shows the path from VK4YB to N1BUG.
cally decoded signals down to 33 dB below the noise in a
The paths are very similar as you would expect, given the
2500-Hz SSB channel, the longest version of FST4 could
similar latitudes of the Northern Hemisphere stations, but one
extend the threshold as low as -45 dB.
is the mirror image of the other. The takeoff angle from
Germany is slightly to the north of east and the receive sig-
New Discoveries nal in Maine appears to come from the west-northwest. There
This turned out to be a game changer. European stations is, however, one big difference in the paths. Can you see
sending FST4W-1800 (aka FW30) started to be detected in what it is?
Australia, and Australian stations were detected on the East The big difference is the EU-to-VK path is largely across
Coast of the United States, both over distances of 16,000 land, while the VK-eastern U.S. path is largely across sea.
kilometers (10,000 miles). By December 2020, these reports It is well-known that sea paths have less attenuation than
were becoming a daily feature. Groups of stations were land paths. The sea reflections are relatively low loss com-
involved. Here are some of the participants: pared to the land reflections. Yet the signal strengths as
Europe: Club Station DLØHOT; Al Mugler, DL7NN; Victor observed by multiple stations are nearly identical on both
Sadchikov, UA4AAV; Alex Lesnichy, R7NT. paths. My startling conclusion is that this mode of propaga-
Australia: Edgar Twinning, EJTSWL (an unofficial short- tion does not include any ground reflections.
wave listener ID); Peter Elekessy, VK2AN; Roger Crofts, Is this possible? Well, it is possible if either ducting or
VK4YB; Steph Spirat, VK5FQ; Brian Barrow, VK5ALZ. chordal hop propagation is involved. These have both been
North America: Wayde Bartholomew, K3MF; Rob Renoud, suggested on multiple occasions before, but maybe it is time
to look at them again.
*827 Middle Run Ct.
Duncanville, TX 75137 Ducting
<kb5njd@cq-amateur-radio.com> In order for ducting to occur, there needs to be a kink in the
electron density below the E-layer which would send the
# Email: <roger@monitorsensors.com> 2200-meter signal back upward and prevent the signal from
Figure 2. Likely propagation path between VK4YB and N1BUG. Can you see the main difference between this path and
the one to DL7NN?
reaching the ground. These kinks do Have we now come to the end of the
indeed exist but the problem is they road? Not quite, there is still another
would need to exist almost every night possibility.
of the northern winter and stretch In Figure 3, the vertical distances are,
almost halfway around the world. I just of course, exaggerated for clarity. We
cannot see that happening. tend to think of the world as an orange
with the peel representing the area
Chordal Hop between layers within which the signal
Is chordal hop a possibility? Let’s take can move. To be more realistic on 2200
a look at conventional HF chordal hop, meters, we need to think of the world as
shown in Figure 3. In this scenario, both an apple with the skin being the only
stations are near the terminator. The place the signal can go. The height of
terminator causes a tilt in the reflecting the R-layer at night is only 60 to 80 kilo-
layer which enables the signal to enter meters, compared with the world cir-
the chordal hop mode. A similar tilt at cumference of 40,000 kilometers.
the other station enables the signal to There is not much room to work with.
return to ground. Is something like this Let’s take a look in Figure 4 at what a
happening at 2200 meters? The answer single chordal hop might look like.
is no. When European stations are
heard in Australia, the terminator is A Typical Grazing Chordal Hop ANTENNAS: Delta Loop HF,
already some thousands of kilometers The horizon distance from a height of HGSW Beam, Multiband
Antennas, Cage Dipole,
to the west of the transmitting site. 80 kilometers is near enough to 1,000 Emergency Communications
There is no tilting occurring at that time kilometers. The distance from the trans- Stealth Antennas, Single
at the transmit end. The terminator does mitter on the left to the receiver on the Band Half-Wave HF Dipoles
get near the receiving stations in the late right is 4,000 kilometers. From the
BALUNS & A NTENNA ACCESSORIES:
session and, in fact, it is not uncommon refraction point on the E-layer to the Antenna Accessories, Rope, Ends, EZ Hang;
to see a small lift in receive signal next refraction point is 2,000 kilometers. Baluns & Line Isolators: Tower Accessories
strength of 2 or 3 dB at this time. The signal comes very close to the ACCESSORIES: Radios, Capacitors, Solar
However, we can rule out tilting as a Earth’s surface in the center of the path
major factor. but does not touch or reflect from the 3861 Mount Olive Church Road
Moravian Falls, NC 28654
(828) 738-6445 website: www.ni4l.com
Figure 5. A more realistic illustration of a grazing chordal hop. See text for details.
surface, which is why I call it “grazing chordal hop” or GCH FST4 software provides data on the Doppler shift of the
from now on. So, is the above scenario possible? The answer arriving signal. The Doppler shifts are much lower than
is no, for two good reasons. would be expected for such a long path. This indicates a
No earth-bound transmitting antenna can ever produce any stable path and is consistent with GCH. In the case of the
radiation at 0°. Nor can an earth-bound receiving antenna EU-to-VK path, there are, unfortunately, no intermediate
receive a signal at 0° as required by the above diagram. We receiving stations whose reports could provide additional
still have the problem of how to get a signal into and out of information. The many Japanese stations are far to the north
the GCH mode. of the Great Circle path and rarely decode the EU stations.
Now consider the modified diagram in Figure 5. There is There are active receiving stations in central and western
nothing clever about this. The transmitter illuminates the sky U.S. Ray, SWLEM3 and Paul Johnson, KILOMETERS5SW
above the transmitting site and hopefully for some distance come to mind (These are both unofficial SWL identifiers for
in the direction of the receiver. It is a brute force method. A use on internet reporting. – ed.). These stations only occa-
very small part of the signal will be propagated at the correct sionally decode the VK FW30 signals and when they do,
angle to enter the GCH, but a heavy price in dB has to be the reports are at about the same levels as the East Coast
paid to get a signal there; likewise at the receiving site. We stations. The situation in North America is more complex.
now have to do a little bit of math to see if a 16,000-kilome- Because of the Pacific Ocean pipeline, conventional multi-
ter path is feasible. hop signals are also present and will give rise to reports on
the West Coast and the Midwest.
Total loss = 2x + ny dB At the time of writing this article, September 2021, the new
season is just starting. Already European signals are being
Where x = loss to get into or out of GCH decoded in Australia and VK signals are being decoded at
n = number of GCHs the super receiving station, operated by Eric Tichansky,
y = average loss per GCH NO3M, in Pennsylvania. From last year’s experience, we
know that even modest receiving stations using just short
We know the number of hops, so “n” is 8. We know the whip antennas can decode long haul DX. Most of the trans-
transmitted power is +30 dBm. From measurement, using a mitting stations are using 20- to 30-meter verticals with base
Siemens D2008 selective level meter, we know the typical or top loading. These are big antennas by amateur standards
band noise at the VK4YB receiving site is -95 dBm, correct- but tiny in terms of wavelength. Just to get 1-watt EIRP, sev-
ed for a 2.5-kHz bandwidth. The decoder tells us the signal eral hundred watts of RF power is usually needed. The
is 43 dB below this noise level. Our total budget for the path ground systems are important.
is thus 168 dB. This is the actual measured path loss. We do We need more stations to participate to provide more data.
not know the exact values of x or y, but for every estimate of The GCH mode is pure speculation at this point. Perhaps you
x, there is a corresponding value of y. Here are some possi- can think of a better explanation. The FST4 modes have both
ble contenders: x=36, y=12; x=40, y=11; x=44, y=10. beacon modes, indicated by the letter W, and QSO modes.
The rays diverge on leaving the transmitter but start to So a QSO is a real possibility at these distances. The paths
reconverge when approaching the antipodal point. The are stable enough, for long enough, to allow a QSO, proba-
combined signal can be enhanced if the rays are in phase bly using F15, rather than F30. Exciting times are ahead. Will
and they will be in phase if the path lengths are the same. you join us on 2200 meters?
This is aided by the long wavelength of 2.2 kilometers. The – 73 and good luck from Roger, VK4YB
Simply Simplex
*Email: <k8zt@arrl.net>, Table 1. FM simplex frequencies band plan for VHF and UHF amateur bands in
website <www.k8zt.com> the United States. (Figures by the author)
Photo B. Base antennas for VHF/UHF FM are available as single-, dual-, tri-, and multi-band verticals. Some examples,
from left to right, are Comet GP-15 (52/146/446MHz), Comet GP-98 (146/446/1200 MHz), Diamond V2000A (52/146/446
MHz), Diamond D3000N Super Discone Antenna(50-1200 MHz transmit), and MFJ’s MFJ-1536 (6M/2M/440MHz). (Photos
from manufacturers’ websites <https://cometantenna.com>, <www.diamondantenna.net> and <www.mfjenterprises.com>)
Antennas
Better antennas are a great way to increase both your trans-
mitted signal strength and your ability to receive other sta-
tions. Better antennas can be very useful for simplex opera-
tion but can also increase both the number of available
repeaters and the quality of your signal into repeaters.
Antenna options to enhance your VHF/UHF radio’s signal
can be broken down into seven categories:
• Extended length, flexible rubber duck type for HTs
• Retractable whip antennas that can extend for HTs
• Improved ground plane for your HT with use a “tiger-tail”
<w3atb.com/tiger-tail-antenna>
• Mobile-style vertical antennas
• Fixed, base, vertical antennas
• Portable flexible antennas (twin-lead J-poles)
• Beam antennas
I have put together a short guide for portable and tempo- Table 2. 2-meter simplex frequencies with 15- or 20-kHz
rary antennas that includes VHF/UHF antennas at spacing
<tiny.cc/portant>.
Extended length, flexible and retractable whip antennas Vertical single or dual-band mobile antennas can be used
attach directly to the HT in place of the rubber duck. Their on your automobile or with a suitable metal ground plane and
longer length usually results in increased gain over the orig- mount at home, either indoors or outdoors. You will need a
inal equipment antennas. length of coax to connect these antennas to your HT or mobile
T
his month I want to focus on FM simplex activity. This
is not complicated ... but it is different from using
repeaters. Simplex requires line of sight (unless, of
course, you get some enhanced propagation — more on that
later) and thus will challenge you to implement the best setup
you can from home, car, or portable locations.
Repeaters have their place, but all require power supplies
and most digital activity will require internet access as well.
Depending on the situation, repeaters may or may not be a
suitable platform for communications in an emergency. Many
nets that are regularly held on repeaters feature a “simplex
night” once a month or so, to help their members assess their
readiness for point-to-point communications on the band in
question. While most nets are on the higher VHF and above
frequencies, you will also find local nets on 6 meters and 10
meters. Our focus is on the use of FM on bands including 2
meters, 70 centimeters, and 1.25 meters. Table 1 shows the
simplex allocation suggestions from ARRL.
Note: that virtually all FM activity uses vertically-polarized
antennas. This is important when communicating point to
point, as cross-polarization losses are significant.
Here are two simplex nets seeking to promote this
activity:
Photo B. The promotional page from the Central Alabama Simplex Net website.
DX Opportunities
(Courtesy of the Central Alabama Simplex Net) DX on FM simplex ... as I alluded to early
on, propagation is still an opportunity on
FM simplex. Most of the time, simplex
umn, starting a new endeavor is much find stations with beams, but these will frequencies are higher in the band than
easier with one or more like-minded of course need to be vertically polarized so-called weak-signal frequencies, so
folks. Find some friends and begin as well. Because much of your work the MUF (maximum usable frequency)
assembling your stations to try simplex will actually be point-to-point, this is a sometimes doesn’t reach them. But on
work. By trial and error, you will learn a case in which polarization is important. certain days, you will find amazing prop-
lot, and improve your station and your
skills. If you can make the commitment
to meet regularly, you will find that your
Low Power and Remote Stations
I include this as a sidebar because one goal of every ham activity should be
little group will grow, and perhaps you
to increase participation and thus introduce more folks to that particular side of
end up leading your club or organiza-
the hobby. When building an FM simplex net, remember that there will be those
tion to a monthly simplex practice net.
who hear you but can’t be heard. Perhaps they are too far and don’t have good
Either way, you will have an improved
propagation, or simply don’t have the antenna system or power out to make
FM setup, and will have explored one
contact. Unless you provide for, and acknowledge those stations, they may give
more facet of our hobby.
up out of frustration. Your net control methods should include a time for listen-
ing for “low power” and “DX” stations, as well as periodically giving out contact
Working Conditions – Station information (phone, email, social media account) for someone on the net who
Requirements for Effective will attempt to “elmer” (hamspeak for mentor) newcomers. In this way, you are
Simplex advancing the cause of amateur radio, and the spirit of helpfulness and coop-
One of the beneficial things about work- eration that marks our ranks.
ing simplex is that it forces you to ensure
Band Recommended Frequencies Calling Frequencies
your station is as finely tuned as possi-
ble. While RF power is important, you 10 meters 29.600 MHz -
will find that your antenna system real- 6 meters 51.5 – 51.6 MHz 52.525
ly makes the most impact. Most simplex 2 meters 146.40 – 146.58 MHz 146.520
work is done with vertical antennas, and 1.25 meters 223.40 – 223.52 MHz 223.500
there are many such antennas available
that offer excellent gain (increased sig- 70 centimeters 445 – 447 MHz (shared) 446.000
nal strength). You will also benefit from 33 centimeters 927.075 – 927.125 MHz 927.500
upgraded feed line (coax); strive for 23 centimeters 1294 – 1295 MHz 1294.500
LMR 400 or better to reduce signal loss
at VHF and higher frequencies. You will Table 1. Simplex frequencies for VHF and above
YL Awards
CQ USA-CA Award Update
500 County Level
JA3UCO – Award number 3812 dated July 17, 2021
K9EGS – Award number 3813 dated August 10, 2021
IK6OIN – Award number 3814 dated August 21, 2021
N7WFK – Award number 3815 dated September 24, 2021
SV1AER – Award number 3816 dated September 30, 2021
IT9ODQ – Award number 3817 dated October 10, 2021
U
pon looking for awards offered for YLs (“young ladies,”
a term used for any female ham) or for contacts with
YLs, I was initially working with a couple of ladies in Worked All Zones – DX YL (WAZ-YL)
the Huntsville area and discussed the matter at the W4DXCC 1. Available to any licensed amateur in the world.
convention this past September. I discovered that the Young 2. Work YLs in 10 different CQ Zones to qualify for certifi-
Ladies Radio League (YLRL) has an active award program, cate with 10-Zone sticker.
so we will feature those awards this time around. 3. Any and all authorized amateur radio bands may be used.
The YLRL was founded more than 80 years ago as an orga- 4. Cross-band contacts are permitted.
nization made up of, run by and promoting women in ama- 5. Contacts may have been made over any period of time.
teur radio. Its founders included some of the most prominent 6. Submit a list of claimed contacts alphabetically arranged
women in amateur radio at the time. The following is from by continent.
the group’s website at <ylrl.org/wp>: 7. For each additional 10 Zones a sticker can be added.
YLRL was founded by Ethel Smith, W7FWB/K4LMB; Lida 8. A plaque is available when all 40 CQ Zones are confirmed.
King, W1GQT; Jean Doss, W5HYF; Genevieve Capstaff,
W6RGX; Marjorie Frazier, W7GXI; Mary Bamberg, W8SBB; Worked All States YL (WAS-YL)
Anita Bien, W8TAY/W4JCR; Lenore Kingston Jensen, 1. Available to any licensed amateur in the world.
W9CHD/W6NAZ; Enid Carter Aldwell, W9NXB / W6UXF / 2. Contact must be made with a duly-licensed YL in each
KH6IHW; Jean Burkhead, W9NLW; Loretta Ensor, of the 50 states in the U.S.
W9UA/WØUA; Carol Keating, W9WWP/W6WSV; and Ethel 3. The District of Columbia may be counted for Maryland.
Pick, VE2HI, in 1939. It is the longest and oldest YL organi- 4. There are no time or band limitations.
zation. These ladies made it possible for us to continue to 5. In qualifying for this certificate, it is possible to work the
make amateur radio a way of communicating with other YLs. SAME YL in each of the 50 states.
Don’t think even these ladies ever thought that 80 years later 6. The list of contacts must be arranged alphabetically by
we would be a worldwide organization. state.
2019 was the 80th year of the YLRL organization, the
longest running YL club in the world. Five hundred (500+)
YLs cannot be wrong.
YLRL is an organization for women with amateur radio
licenses and like radio itself, extends to women all over the
world. On this website you can learn about the organization,
acknowledge our fore-mothers, purchase items to show your
pride and connection, find out the latest information about
contests and special events, and stay updated on happen-
ings with our members.
The YLRL offers a variety of award certificates, a few for
YLs only but most for anyone working a specified number of
YL hams in the locations / modes / bands specified for each
award. The most popular are described below, again taken
from the YLRL website.
*Email: <KI4KWR@cq-amateur-radio.com>
DX YL
1. Available to licensed YL operators only, for working 10
different licensed women operators outside your own coun-
try, on or after April 1, 1958.
2. USA and possessions are counted as separate coun-
tries, as well as Alaska and Hawaii.
3. Any and all amateur bands may be used.
4. Contacts do not have to be with 10 different countries,
just 10 different DX YLs.
5. Use approved DX country list. Worked All Continents YL (WAC-YL)
6. The log must be arranged alphabetically by callsign. 1. Available to any licensed amateur in the world.
7. Endorsements: Stickers will be awarded for each 10 addi- 2. Two-way communications must be established on the
tional DX YLs, subject to the same confirmation as above. amateur radio bands with YLs on the six continents: North
When 100 DX YL contacts have been confirmed, you may apply America, South America, Europe, Africa, Asia, and Oceania
for either a special paper certificate or an engraved plaque. (which includes Australia and New Zealand).
3. Any and all authorized amateur radio bands may be used.
4. Cross-band contacts are permitted.
5. Contacts may have been made over any period of time.
6. Contacts with all six continents must be made with duly
licensed women operators.
7. It is not necessary for each contact to be a different YL.
8. Submit a list of claimed contacts alphabetically arranged
by continent.
YL-DXCCL
1. Available to any licensed amateur in the world.
2. Two-way communications must be established on autho-
rized amateur bands with stations (fixed or mobile), operat-
ed by licensed YLs from 100 countries on the current ARRL
list of countries.
W
e all get wrapped up in chasing the usual awards, Here are the challenges we had in the ensuing months.
but for many of us that can become hit or miss as APRIL: 15-DAY PHONE CHALLENGE: Same rules as
you climb the award ladders to WAS, WAC, DXCC, March except all QSOs had to be made on phone.
WAZ, and so on. Personally, having worked them all, I have (Interesting side note, the phone challenge was the least pop-
found it fun to fill in holes with band and mode QSOs. But I ular, who would have thought that?)
can remember occasional past “club activity awards” that May: 15-DAY DIGITAL CHALLENGE: Same rules as
really caught my attention. DXing in the pandemic present- March except all QSOs had to be made on a digital mode.
ed us all with a high and low of activity. The high represent- FT8 was the most popular by far.
ed the extra time many of us had staying at home, turning
on the radio and making QSOs. The low was having all of
that extra time, but with the pandemic, DXpeditions were
pretty much on hold. So, we were all left with working other
people who were staying home all over the world, but usu-
ally in the less rare DXCC entities, and virtually none to unin-
habited ones. Overall, this was a blessing in disguise for
general ham radio activity. There were many non-hams out
there resorting to watching the news on TV far more than
was healthy (IMHO), or focusing all of their attention to
“online social media.” Meanwhile, many ham radio opera-
tors who had access to a radio were getting on the air a lot
more frequently than before. A sidebar to all this was also
increased activity on FT8, which was something new for
many hams to experience. After sitting around for 2020 with
little coordinated activity, with most Field Days cancelled
and moved to home stations to be safe, and nearly all
meetings moved to Zoom, all that was left were the regular
contests. But even those, without the normally abundant
contest DXpedition stations to add to the excitement, just
weren’t quite the same. It was time to come up with a club Photo A. Sample certificate for South Jersey DX Asso-
membership challenge! ciation’s 15-DX-Challenge last February. Members could
So, in January 2021, I decided to try something locally by earn it by working at least one DX station a day on at least
having “pandemic challenges” for our South Jersey DX 15 days of the month.
Association (SJDXA) membership. Certificates were issued
to everyone who accomplished a challenge. At first, these
were monthly challenges. But we switched over to a couple
of seasonal challenges more recently.
The first challenge would be a “15 DAY DX CHALLENGE”
for the month of February (Photo A). The rules were pretty
simple. You had to work at least ONE DX station per day for
15 days in February. This sounded pretty simple, but my
intention was to encourage members to turn on their radios.
Giving them a reason to get on the air and make at least ONE
QSO outside the U.S. each day! I had no idea how much
interest there would be in this challenge. But to my surprise
we had 14 members meet the challenge. Keep in mind that
we have 39 members with a fair number not that active on
the air. I would take a guess at perhaps 25 actively “on the
air,” which is probably fairly normal for a club our size. So,
getting 14 members to actually track and submit for the chal-
lenge was pretty awesome.
Along came March … what to do next and step things up
a bit? This time we went for a 15-DAY WARC/60 CHAL-
LENGE. Same rules as the February challenge except all
QSOs had to be made on the WARC bands (30, 17, and 12
meters) or 60 meters. Ten members accomplished this one. Photo B. SJDXA’s June challenge was to work DX stations
on two different modes. The goal of the challenge program
was to encourage club members to get and stay active on
*email: <n2oo@comcast.net> the air during the Covid pandemic.
5 Band WAZ
As of October 15, 2021 Callsign Zones Zones Callsign Zones Zones
2327 stations have attained at least the 150 Zone level, and Needed Needed
1086 stations have attained the 200 Zone level. RZ3EC 199 1 on 40M W6RW 198 2 & 22 on 10M
S58Q 199 31 W9RN 198 26, 19 on 40M
As of October 15, 2021 SM7BIP 199 31 WC5N 198 22, 26
The top contenders for 5 Band WAZ (Zones needed on 80 USØSY 199 1 on 15M WL7E 198 34, 37
or other if indicated): VO1FB 199 19 Z31RQ 198 1, & 2 on 10M
CHANGES shown in BOLD W1FJ 199 24 ZL2AL 198 36, 37
W1FZ 199 26
W3LL 199 18 on 10M The following have qualified for the basic 5 Band WAZ
Callsign Zones Zones
W3NO 199 26 Award:
Needed
AK8A 199 17 W4LI 199 26
W6DN 199 17 Callsign 5BWAZ # Date # Zones
DM5EE 199 1 NT9F 2320 2021-09-16 151
EA5RM 199 1 W6RKC 199 21
W6TMD 199 34 DL6JZ 2321 2021-09-23 193
EA7GF 199 1 OH2BEN 2322 2021-10-03 199
H44MS 199 34 W9OO 199 18 on 10M
W9XY 199 22 DK1WU 2323 2021-10-03 182
HAØHW 199 1 USØSY 2324 2021-10-03 199
HA5AGS 199 1 9A5I 198 1, 16
EA5BCX 198 27, 39 OH1JP 2325 2021-10-04 162
I5REA 199 31
F5NBU 198 19, 31 K3FRK 2326 2021-10-05 172
IKØXBX 199 19 on 10M
F6DAY 198 2 on 10M & 15M JH9AUB 2327 2021-01-07 187
IK1AOD 199 1
IK8BQE 199 31 G3KDG 198 1, 12
G3KMQ 198 1, 27 Updates to the 5BWAZ list of stations:
IZ3ZNR 199 1
HB9FMN 198 1 on 80M & 10M
JA1CMD 199 2 Callsign 5BWAZ # Date # Zones
I1EIS 198 1 & 19 on 10M
JA5IU 199 2 RC2A 2217 2021-09-15 180
JA1DM 198 2, 40
JA7XBG 199 2
JA3GN 198 2 on 80M & 40M
JH7CFX 199 2
JA7MSQ 198 2 on 80M & 10M New recipients of 5 Band WAZ with all 200 Zones con-
JI4POR 199 2 JH1EEB 198 2, 33 firmed:
JK1AJX 199 2 on 10M KØDEQ 198 22, 26
JK1BSM 199 2 K1BD 198 23, 26 5BWAZ # Callsign Date All 200 #
JK1EXO 199 2 K2EP 198 23, 24 NONE
K1LI 199 24 K2TK 198 23, 24
K4HB 199 26 K3JGJ 198 24, 26 Rules and applications for the WAZ program may be obtained
K5TR 199 22 K3LR 198 22, 23 by sending a large SAE with two units of postage or an address
K7UR 199 34 K3WA 198 23,26
K9KU 199 22 on 15M label and $1.00 to: WAZ Award Manager, John Bergman,
K4JLD 198 18, 24 KC5LK, 125 Deer Trail, Brandon, MS 39042-9409. The pro-
KZ4V 199 26 K9MM 198 22, 26
N3UN 199 18 cessing fee for the 5BWAZ award is $10.00 for subscribers
KI1G 198 24, 23 on 10M (please include your most recent CQ mailing label or a copy)
N4NX 199 26 KZ2I 198 24, 26
N4WW 199 26 and $15.00 for nonsubscribers. An endorsement fee of $2.00
N4GG 198 18, 24
N4XR 199 27 N6PF 198 18, & 23 on 10M for subscribers and $5.00 for nonsubscribers is charged for
N8AA 199 23 NXØI 198 18, 23 each additional 10 zones confirmed. Please make all checks
N8DX 199 23 ON4CAS 198 1,19 payable to John Bergman. Applicants sending QSL cards to a
N8TR 199 23 on 10M OZ4VW 198 1, 2 CQ checkpoint or the Award Manager must include return
OH2BEN 199 1 on 10M UA4LY 198 6 & 2 on 10M postage. KC5LK may also be reaced via email: <kc5lk@cq-
RA6AX 199 6 on 10M UN5J 198 2, 7 amateur-radio.com>.
RU3DX 199 6 US7MM 198 2, 6
RWØLT 199 2 on 40M VK3GA 198 12 & 13 on 10M *Please note: Cost of the 5 Band WAZ Plaque is $100 shipped
RX4HZ 199 13 W5CWQ 198 17, 18 within the U.S.; $120 all foreign (sent airmail).
SSB: 350: YO3HJV, KB2QQZ. 400: W4SSF. 450: N8IK. 500: SV1AER. 650: JH7CUO. 900: SINGLE BAND WAZ 293.................................................OH1JP
JK7QJK. 294..................................................JA4IXI
6 Meter 295..............................................IKØWRB
Mixed: 450: YO3HJV, KB2QQZ. 500: KG5ZNJ, JJ2NWI, WA3EEC. 550: JS2IYY, HB9FNO. 181..............................KØWYN, 26 Zones 296 ...............................................JH7IQQ
600: JP7WJA, WA1DD. 650: NØNV. 700: WF8R, N7TBR. 750: N2TC. 800: N2YU, N1AH, 182 .............................JA9KRO, 25 Zones 297...............................................JH9AUB
KE5WCT. 850: IN3FCK, N6VF, K3FRK. 950: K2KJ. 1000: N8IK, KO8V. 1050: KA5WSS, 298 ...............................................JG3IWL
W4SSF. 1100: OH1JP. 1350: WR7X. 1400: IK6OIN. 1450: SV1AER, LA7EIA, JH7CUO. 6 Meter Updates
1550: HB9VAB. 1800: JA7VFA. 2200: JR3UIC. Mixed
141...............................DK1FW, 30 Zones
146.............................HB9BGV, 30 Zones 10096 ...........................................JH9VLZ
Digital: 350: WR7FT, DH3PL, N7RGF, N6YIH. 400: IN3FCK, N3AML. 450: VK2EY,
10097 ............................................KD3HN
HB9FNO. 500: KG5ZNJ, WA3EEC. 550: WA1DD, JS2IYY. 600: JHØEYA. 650: N2YU. 700:
40 Meter Digital 10098 ...............................................NT9F
W4SSF, WF8R, N7TBR. 750: K2KJ, KA5WSS, N6VF. 800: IU1HGN, N1AH, KE5WCT.
850: OH1JP. 900: AB1NS. 1000: KO8V. 1050: SV1AER. 1200: LA7EIA. 1250: WR7X. 1450: 18.....................................................N1NK 10099 ...........................................DJ2WW
HB9VAB. 1500: JA7FVA. 1850: JR3UIC. 19 .................................................JA7CVL 10100..............................................ES1LL
10101 ............................................RN3BC
160 Meters: HB9VAB 80 Meter CW 10102 ...............................................N7NT
80 Meters: HB9VAB, KO8V 111..............................................OH2BEN 10103...............................................K7GA
60 Meters: AB1NS, HB9VAB 10104.............................................IK6OIN
40 Meters: JH7CUO, W4SSF, HB9VAB, N6VF, N8IK 160 Meter 10105 ............................................N6DNU
30 Meters: K2KJ, HB9VAB, WF8R 10106 ...............................................N3PS
681.............................OH2BEN, 40 Zones
20 Meters: JP7WJA, IK6OIN, WA1DD, KA5WSS, KG5ZNJ, JH7CUO, W4SSF, VK2EY, 10107 ............................................KØSRL
682............................RAØSMA, 30 Zones
WR7FT, JS2IYY, N6VF, JJ2NWI, WF8R 10108...............................................WF7T
17 Meters: SV1AER, KA5WSS, HB9VAB
10109................................................W7IY
15 Meters: JH7CUO, HB9VAB
12 Meters: K7PT ALL BAND WAZ 10110 ............................................W5AAJ
10 Meters: NA5WH 10111 ...............................................NF7D
6 Meters: VE6MB CW
1162...............................................BA5AD SSB
Africa: IN3FCK 1163.................................................WF7T 5519.............................................GM7NZI
Asia: JP7WJA, VK3SN, IN3FCK, OH1JP, JH7CUO, JP2XSP, JS2IYY, WF8R 5520 ...........................................DL2AWG
Europe: JP7WJA, WA1DD, HF1RF, VK3SN, OH1JP, JH7CUO, W4SSF, DH3PL, HB9VAB, 5521 .............................................YO3IPR
JJ2NWI, YO3HJV, HB9FNO, WF8R, IW7DVM. KB2QQZ. Digital
Oceania: VK3SN, LA7EIA, JH7CUO, VK2EY, JS2IYY, HB9VAB, WF8R RTTY
288................................................JH7IMX
North America: WA1DD, KG5ZNJ, KO4HXC, OH1JP, WP4JLZ, JH7CUO, W4SSF, 309 ................................................KSØAA
289...................................................K7GA
WR7FT, N3AML, VE6MB, N6VF, N7RGF, N6YIH, N8IK, W4TYD, WA3EEC, WF8R
South America: HB9VAB 290...............................................JH1GZE
291...............................................JA5GOJ Satellite
6M Bar: LU9DO 292 ................................................W5AAJ 33...............................DL6GBM, 25 Zones
Rules and applications for the WAZ program may be obtained by sending a large SAE with
Complete rules and application forms may be obtained by sending a business-size, self- two units of postage or an address label and $1.00 to: WAZ Award Manager, John Bergman,
addressed, stamped envelope (foreign stations send extra postage for airmail) to "CQ WPX KC5LK, 125 Deer Trail, Brandon, MS 39042-9409. The processing fee for all CQ awards
Awards," P.O. Box 355, New Carlisle, OH 45344 USA. Note: WPX will now accept prefix- is $6.00 for subscribers (please include your most recent CQ mailing label or a copy) and
es/calls which have been confirmed by eQSL.cc. and the ARRL Logbook of The World (LoTW). $12.00 for nonsubscribers. Please make all checks payable to John Bergman. Applicants
sending QSL cards to a CQ checkpoint or the Award Manager must include return postage.
*Please Note: The price of the 160, 30, 17, 12, 6, and Digital bars for the Award of Excellence KC5LK may also be reached via e-mail: <kc5lk@cq-amateur-radio.com>.
are $6.50 each.
CQ DX Honor Roll
The CQ DX Honor Roll recognizes those DXers who have submitted proof of confirmation with 275 or more ACTIVE countries. With few exceptions, the
ARRL DXCC Countries List is used as the country standard. The CQ DX Award currently recognizes 340 countries. Honor Roll listing is automatic when
an application is received and approved for 275 or more active countries. Deleted countries do not count and all totals are adjusted as deletions occur. To
remain on the CQ DX Honor Roll, annual updates are required. All updates must be accompanied by an SASE if confirmation of total is required. The fee
for endorsement stickers is $1.00 each plus SASE. (Stickers for the 340 level and Honor Roll are available.) Please make checks payable to the Award
Manager, Keith Gilbertson. Mail all updates to Keith Gilbertson, KØKG, 21688 Sandy Beach Lane, Rochert, MN 56578-9604 USA.
CW
DL3DXX ....339 K4CN ........339 N7RO ........339 K8SIX........338 K9OW ......334 K6YK.........329 YT1VM ......322 WA4DOU ..312 4XIVF ........286
HB9DDZ....339 K4JLD .......339 NØFW ......339 KA7T .........338 PY2YP ......334 W9IL..........329 4Z5SG.......321 YO9HP......312 K6YR.........284
K4IQJ ........339 K4MQG .....339 OK1MP .....339 WA5VGI ....338 WG5G/ IKØADY ....328 N2LM ........321 W6WF .......309 PP7LL ......282
K9MM........339 K5RT.........339 W3GH .......339 W9RPM.....338 QRPp ....334 OZ5UR......328 ON4CAS ...321 KT2C........ 307 WR7Q .......282
N4MM .......339 K7LAY.......339 W4OEL .....339 G3KMQ .....337 WD9DZV...334 AB4IQ ......327 W2OR .......320 K4DGJ ......307 N2VW........280
WB4UBD...339 K7VV.........339 W5BOS .....339 KØKG........337 K2OWE .....333 K6CU ........326 HB9DAX/ W4ABW ....306 K4EQ ........280
WS9V........339 K8LJG .......339 W7CNL .....339 W7IIT ........337 K5UO ........333 KE3A.........326 QRPp .....319 K7ZM ........305 W8BLA......280
EA2IA........339 N4AH ........339 W7OM.......339 K8ME ........336 N6AW........333 EA5BY ......325 W6YQ ......319 HA5LQ ......301 WB5STV ...277
F3TH .........339 N4CH ........339 W8XD........339 W1DF........336 W4MPY.....333 KA3S.........325 HA1ZH ......318 RN3AKK....300 YO6HSU ...275
K2FL ........ 339 N4JF .........339 WK3N........339 W6OUL .....336 K6LEB.......331 K7CU ........324 N6PEQ......318 WA9PIE ....298
K2TQC ......339 N4NX ........339 WØJLC .....339 JA7XBG ....335 K9VKY ......331 N3RC ........324 CT1YH ......316 K4IE ..........295
K3JGJ .......339 N5ZM ........339 WØVTT .....339 F6HMJ ......334 N7WO .......331 N7WO .......324 EA3ALV ....315 YU1YO......295
K3UA.........339 N7FU.........339 YU1AB ......339 K1FK .........334 OK1DWC ..331 KEØA ........322 RA1AOB ...313 WA2VQV...292
SSB
AB4IQ .......340 K6YRA ......340 VE3MRS ...340 W4UNP .....339 F6HMJ ......335 AA1VX ......332 N2LM ........328 N7YB.........315 4X6DK.......298
DJ9ZB .......340 K7VV.........340 VE3XN ......340 W9RPM.....339 HB9DQD ...335 KE3A.........332 AE9DX ......327 IV3GOW....312 K2HJB.......295
DL3DXX ....340 K8LJG .......340 VK2HV ......340 EA3EQT....338 IKØAZG ....335 N2VW........332 K7HG ........327 N8SHZ ......312 F5MSB ......293
DU9RG .....340 K8SIX........340 W3AZD .....340 K3UA.........338 IW3YGW ...335 N5YY.........332 K6GFJ.......326 K7CU ........311 W9ACE .....291
EA2IA .......340 K9MM........340 W3GH .......340 K7LAY.......338 OE2EGL....335 K5UO ........331 KE4SCY....326 OK1DWC ..311 N3KV.........289
EA4DO......340 KE5K.........340 W4ABW ....340 K9HQM .....338 VK2HV ......335 KC2Q ........331 KF4NEF ....325 KU4BP ......310 W6MAC.....289
HB9DDZ....340 KZ2P .........340 W5BOS .....340 KM2P ........338 W4WX.......335 SV3AQR ...331 W6WF .......325 W6NW.......310 N5KAE ......283
I8KCI .........340 N4CH ........340 W6BCQ.....340 N4NX ........338 WB3D........335 WØROB ....331 W9GD .......325 I3ZSX ........309 IZ1JLG ......282
IK1GPG.....340 N4JF .........340 W6DPD .....340 YU1AB ......338 AA4S.........334 W6OUL .....331 VE7EDZ ....324 G3KMQ .....308 WA9PIE ....282
IN3DEI ......340 N4MM .......340 W7BJN......340 4Z4DX.......338 EA5BY ......334 XE1MEX ...331 WA5UA .....324 KA1LMR....308 WD8EOL...281
K2FL .........340 N5ZM ........340 W7OM.......340 K1UO ........338 K9OW .......334 KD5ZD ......330 F6BFI ........323 RA1AOB ...308 IWØHOU...277
K2TQC ......340 N7BK.........340 W8ILC .......340 N7WR .......338 PY2YP ......334 WA4WTG..330 ON4CAS ...323 XE1MEX ...308 AKØMR.....276
K3JGJ .......340 N7RO .......340 W9SS........340 WA5VGI ....338 VK4LC.......334 W1DF........330 VE6MRT ...323 IK5ZUK .....307 NØAZZ......275
K4CN ........340 NØFW .......340 WB4UBD...340 W2CC .......338 W8AXI.......334 WØYDB ....330 W5GT........323 IØYKN.......306 SQ7B ........275
K4IQJ ........340 OK1MP .....340 WK3N........340 W7FP ........338 XE1J .........334 ZL1BOQ....330 N6PEQ......322 XE1MW.....305
K4JLD .......340 OZ3SK ......340 WS9V........340 W9IL..........338 CT3BM......333 AD7J .........329 W4MPY.....322 K4IE ..........304
K4MQG .....340 OZ5EV ......340 XE1AE ......340 N4FN.........337 IK8CNT .....333 N3RC .......329 K8IHQ .......321 K4ZZR.......304
K4MZU......340 VE1YX ......340 YU3AA ......340 IØZV..........336 K8LJG .....333 VE7SMP ...329 KW3W.......320 K7ZM .......303
K5OVC......340 VE2GHZ....340 JA7XBG ....339 K3LC .........336 N6AW........333 WØULU.....329 TI8II...........320 4Z5FL/M....302
K5RT.........340 VE2PJ .......340 KØKG........339 K8ME ........336 OE3WWB..333 CT1AHU....328 YO9HP......320 K7SAM......301
K5TVC ......340 VE3MR......340 W2FKF......339 EA3BMT....335 WD9DZV...333 N1ALR ......328 XE1RBV....317 KA8YYZ ....301
RTTY
NI4H . . . . . 338 WK3N . . . . 338 OK1MP . . . 337 K8SIX . . . . 334 W3GH . . . . 333 AB4IQ . . . . 323 N4MM . . . . 302 K8ME . . . . 278
WB4UBD . 338 N5ZM . . . . 338 K4CN . . . . 334 W9RPM . . 334 K3UA . . . . 332 K4WW . . . 323 K4IQJ . . . . 300 IN3YGW . . 275
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CONTESTING
BY TIM SHOPPA,* N3QE
Getting an Assist
S
ingle-op entrants in the six 2022 gory? Part of it reflects the “boy and his Assisted
North American QSO Parties radio” mindset of old-school contesters Contest CW SSB
have, for the first time, the choice who aren’t fans of assisted contesting.
of entering the Assisted category. In I also note that both the NAQP and CQ WW 2020 51% 37%
previous years, assisted NAQP single ARRL RTTY contests have large ARRL DX 2021 48% 40%
ops had their scores listed with the domestic components, and domestic ARRL Sweepstakes 2020 36% 29%
multi-operator M/2 entrants. The 100- contests have been slow to adopt a sep-
watt power limit and friendly exchange arate category for assisted single-ops.
of name and state make the NAQPs Contrast this with the large DX contests Table 1. Percentage of operators
popular with beginning contesters. which emphasize working other coun- choosing the assisted category in six
Advanced contesters looking for high tries for points and multipliers, and large contests.
rates and an opportunity to exercise which were the early adopters of assist-
their SO2R skills compete hard in the ed categories. Let’s look at the enthu- tor arrangements involving assistance
NAQPs as well. With the addition of a siastic early adoption of assisted cate- through DX-alerting nets, etc.) is not
separate assisted category, the NAQP gories in the biggest DX contests. permitted.”
now becomes a prime training ground DX spotting networks — in the form By the late 1980s, Dick Newell, AK1A,
for learning how to use spots to chase of landline phone calls between hams had combined the nascent technolo-
both multipliers and QSOs. interested in DXing or local VHF an= gies of amateur VHF packet data with
In every respect, the NAQP contests nouncements — have existed since the the traditions of HF DXing and contest-
were late in adding an official assisted 1950s. Especially in DX contests, ing. No longer were phone trees or
category. In the January 2021 NAQP enthusiastic contesters had been using voice VHF nets the only way to distrib-
CW results, 168 stations are listed in the DXers phone and VHF networks to ute spots — contesters and DXers
the M/2 scores. Only 18 of them are true help them work new multipliers, and for could post the stations they heard and
multi-ops, the other 150 are assisted decades this assistance, in the form of worked to a digital VHF network for dis-
single operators. The ARRL RTTY knowing the frequency and callsign of tribution throughout a region or across
Roundup was also late in adding the rare DX, wasn’t explicitly mentioned in the country. Dick was inducted into the
assisted category, back in 2014. In any contesting rules. The first contest CQ Amateur Radio Hall of Fame in 2002
2013, the last year when single-op rules related to “assistance” appear in for his contributions to both DXing and
assisted entrants were listed under the the 1977 CQ World Wide DX Contests. contesting. A contest station with a VHF
multi-operator scores in the ARRL There, the definition of the Single packet node nearby, a TNC to interface
RTTY Roundup, 373 of the 460 multi- Operator category notes that “The use the radio to the computer, and AK1A’s
op scores were assisted single-ops. of DX spotting nets or any other form of PacketCluster software would scroll the
Why were these two contests so slow DX alerting assistance places the sta- spots past on the PC’s screen running
in adopting an assisted single-op cate- tion in the Multi-Operator category.” In the DOS-based software. A few years
1980, the ARRL DX Contest included a later, assisted contesters on the lead-
similar rule in the definition of Single ing edge of technology began incorpo-
email: <n3qe@cq-amateur-radio.com> Operator: “Use of spotting nets (opera- rating computer-distributed spots into
Sunspots: Sunspots:
Observed Monthly, September 2021: 52 Observed Monthly, September 2020: 1
12-month smoothed, March 2021: 21 12-month smoothed, March 2020: 3
10.7-cm Flux: 10.7 cm Flux:
Observed Monthly, September 2021: 87 Observed Monthly, September 2020: 71
12-month smoothed, March 2021: 79 12-month smoothed, March 2020: 70
A
s this column goes to press, it is safe to say that the regular record keeping of sunspot counts began. Cycle 24
Sun’s sunspot activity is increasing. Space weather was also the weakest in 100 years. Solar maximum occurred
scientists are making an assessment of Sunspot Cycle in April 2014 with sunspots peaking at 114 for the solar cycle,
25 and they say it appears to be moving more quickly toward well below average, which is 179.
a solar cycle maximum, as the numbers reveal that the activ- While Solar Cycle 24 was average in length, the progres-
ity level is moving higher than the current forecast. sion of activity was unusual. The Sun’s Northern Hemi-
The current solar prediction is now updated each month sphere led the sunspot cycle, peaking over two years ahead
using historical data as well as the latest month’s observed of the Southern Hemisphere. This resulted in solar maximum
solar indices to provide estimates for the rest of the current having fewer sunspots than if the two hemispheres were in
solar cycle and the next. These predictions are made by the phase.
Space Environments Team in the Natural Environments
Branch of the Engineering Directorate at Marshall Space Solar Cycle 25
Flight Center (MSFC). Their forecast provides solar cycle For the past year, sunspot activity on our local star has steadi-
predictions for NASA engineering programs and the aero- ly increased, indicating that the Sun transitioned to Cycle 25.
space community. This current cycle is forecast to be weak, the same strength
The updated forecast provides future statistical estimates
of sunspot number, solar radio 10.7-cm flux (F10.7), and the
geomagnetic planetary index, Ap, for many groups that have LAST-MINUTE FORECAST
use of this space weather data. Some use these numbers Day-to-Day Conditions Expected for December 2021
for input to various space environment models. HF radio com- Expected Signal Quality
municators — including the amateur radio community — use Propagation Index (4) (3) (2) (1)
the sunspot count, the F10.7, and the Ap as inputs to VOA- Above Normal:
1-3, 16-23, 26, 28-30
A A B C
CAP computer models used for planning and analyzing the High Normal: A B C C-D
radio propagation paths that use the ionosphere for DXing. 4, 7-10, 14-15, 25,
27, 31
The forecasted solar indices represent the 13-month Low Normal: B C-B C-D D-E
smoothed values consisting of a best estimate value stated 5, 11-13, 24
Below Normal: C C-D D-E E
as a 50-percentile value along with the 95- and 5-percentile 6
statistical values. The F10.7 prediction also includes a 75- Disturbed:
n/a
C-D D E E
Table 1. Solar flares are classified by intensity. Each class represents a ten-fold increase in intensity.
event was captured in real-time by the space agency’s Solar Solar cycle prediction gives a rough idea of the frequency
Dynamics Observatory (SDO). of space weather storms of all types, from radio blackouts to
It is hard to tell to where the exact trajectory of the CME geomagnetic storms and solar radiation storms. Such pre-
passes. Solar event observers speculated that the CME from dictions and observations are used by amateur radio com-
this flare — a huge eruption of charged particles — would municators who employ modeling tools like VOACAP.
reach Earth by October 30th or 31st. If the CME directly
impacted Earth, it might have triggered Earth’s Northern and New Satellites Will Provide Enhanced
Southern lights and potentially interfered with satellite-based Observations of the Sun
communications (not to mention HF propagation). The CME In 2024, NOAA is expected to launch a new spacecraft ded-
missed Earth, and we just observed a slight glancing blow, icated to operational space weather forecasting. NOAA’s
that resulted in a Planetary-K Geomagnetic rise to a minor Space Weather Follow-On L-1 Observatory will be equipped
geomagnetic storm level. with instruments that sample the solar wind, provide imagery
Figure 3. Ten years ago, in November 2011, there was a Figure 4. Solar flares are massive eruptions of radiation from
period with a number of sunspot regions rotating across the the Sun that send charged particles streaming outward from
visible solar disc. A lot of sunspots peppered the Sun over the star (see text for more details). They can also be accom-
a magnetically active 23-day period (November 4-30), which panied by massive eruptions of solar particles, called coro-
is one complete solar rotation. During this month, most of nal mass ejections (CMEs). Such eruptions send charged
the sunspots appeared in the Sun’s northern hemisphere. particles out from the Sun at about one million miles per hour
This was the peak month thus far into that solar cycle (Cycle (1.6 million kph) or more, and typically take a few days to
24). The images were taken by SDO’s HMI instrument in reach Earth. On October 28, 2021, a flare caused a coro-
what we call intensitygrams, which is how the Sun appears nal mass ejection that appeared to be Earth-directed, but
in filtered light. The video shows how spots can change over later resulted in only a minor brush with our geomagnetic
hours and days. The movie consists of over 1,000 frames field. This X-class flare, measuring X1.0, originated from a
— Watch the video at <https://youtu.be/JfmezCNYtIo>. sunspot called AR2887 (Active Region 12887). (Courtesy
(Courtesy of The Solar Dynamics Observatory [SDO]) of SDO)
of CMEs, and monitor other extreme Stay tuned to this column for a play- pheric noise levels will be at seasonally
activity from the Sun in finer detail than by-play of the action. low values during the month. Reason-
before. NOAA’s next Geostationary ably strong signal levels are expected on
Operational Environmental Satellite December Propagation most of the open bands. The higher
(GOES-U) is also scheduled to launch in During December, expect a moderate to bands will carry world-wide DX propa-
2024. GOES-U will carry three solar low level of solar activity, with 10.7-cm gation more often, as we are seeing a
monitoring instruments, including the first flux levels peaking in the low 100s. In the steady rise in sunspot activity.
compact coronagraph, which will help Northern Hemisphere, expect the sea- For this month, 10- and 12-meter DX
detect CMEs. Enhanced observations of sonal increase of ionospheric density to openings will be sporadic and only dur-
the Sun from these satellites will help build more rapidly after sunrise than dur- ing daylight hours if existent, especially
improve space weather forecasting. ing other seasons. Static and atmos- where the propagation paths cross the
sunlit regions. If they develop, they will
be rather short but strong, with a lot of
fading.
Real Hams Do Code Expect fair daytime openings on the
Learn code with
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15-, 17-, and 20-meter bands, primari-
ly on north-south paths, with strong
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evening.
The 30-meter band will be a strong
player for DXing, as well, following the
pattern of 20 meters. Expect this band
to remain open toward the south and
west from early evening until about
midnight, mostly for DXers in the lower
latitudes.
On 40 meters, regional daytime open-
ings will remain strong for most of the
day, while great DX will open early in
the afternoon. From midnight to sunrise,
40 meters promises some of the hottest
nighttime DX during December. The
first DX openings should be toward
Europe and the east during the late
afternoon, then move across the south
through the hours of darkness, while
remaining open into most parts of the
world. Just after sunrise, openings will
be more in a westerly direction. Low
EVEN MORE!
meters again for about an hour or so
after sunrise. For openings between
1,300 and 2,300 miles, openings will
occur on 20, 17, and 15 meters, with
fewer on 12 and 10 meters, during the
daylight hours. From sundown to mid- WHY?
night, check 20, 30, and 40 meters for
these long-distance openings, and Because they are giving back to their communities! They are
then check 40 and 80 meters after mid-
night until sunrise. Try 40 meters again helping with civic events, motorist assistance AND MORE,
for an hour or so after sunrise. yes even emergencies and disasters, if needed!
VHF Conditions
Aurora is not expected to occur this CONTACT
month, with perhaps one or two excep-
tions. If there were any chance at all,
REACT INTERNATIONAL
you’ll want to look for days with condi- 301-316-2900
tions at Disturbed or Below Normal, when
there is a possibility for Field Aligned Or write to
Irregularities (FAI) and Auroral-E propa- REACT INTERNATIONAL
gation. Check the last-minute forecast for P.O. Box 21064, Dept CQ100
those days during December that are Glendale, CA 91221
expected to be in these categories.
Look for some decent meteor show- RI.HQ@REACT Intl.org
er activity this month, providing condi-
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Advertising Rates: Non-commercial ads are 20 cents per word including abbreviations and addresses. Commercial and organization ads are $1.00 per word. Boldface
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