Last night I copied SW Radiogram out of Pennsylvania on 9625kc and it was marginal to say the least. That station is always difficult to copy here in RI because it can sit just inside of normal HF single-hop distance. 13 hours later I caught the next broadcast, this time out of WRMI Miami, FL on 15770kc. That was a totally different story. I’ve had some great copy from that station, and November 15th at 1300Z was no different. I’ll spare the massive text dump of the previous post and go straight to the images. Clean, Clear and Vibrant.
Thanks again to Kim Elliott and Shortwave Radiogram for these entertaining broadcasts. Shortwave listening doesn’t have to be all AM voice and music. There is room for more modes and more voices. 73, N1QDQ
Posted onNovember 4, 2021|Comments Off on SW Radiogram under Very Poor Conditions
The earth’s atmosphere was impacted by a Coronal Mass Ejection (CME) early on November 2, 2021. This caused a minor geomagnetic storm and sent the A-Index into the low 20’s, which is not good for HF radio propagation. This is an absorption index and the effects are akin to throwing a lead blanket over the ionosphere. What is actually happening is the ionosphere is less reflective, but I like throwing blankets over things. In practice there is a reduced chance of multi-hop propagation. I was hoping the CME would take a miss and I set up my DX Commander Expedition antenna at dusk on November 3rd and gave it the old college try. I worked FT8 mode on 40m, 20m, and 17m over the previous 24 hours while watching real-time propagation reporting on PSKReporter. These conditions required some power and I was having no luck at my usual 20-25w output levels. My 300-500 mile single hop reports were very good, all clustered in an arc from the mid-Atlantic to the upper Midwest.
Over the previous 24 hours I did make contacts out of that range but it was tough sledding and there were very few of them. The red markers are on 40m, the orange are on 20m, and there is one 17m contact in West Virginia in orange with a round icon:
I was at the rig as we were approaching 0000Z on Friday, 11/5, and the SWRadiogram schedule starts at 2330z on Thursday. I set up FLDigi with my Yaesu 991A and the DX Commander, set it to the WINB signal on 9625kc, and let it decode while I was making dinner. Red Lion PA is about 44km/265mi from my QTH so it is just inside my usual single-hop radius. I did listen to the signal as the broadcast started. signal was washed out and fading, and nothing like “armchair copy”. This is a good test for for gauging how robust the MFSK modes used by SWRadiogram are under bad conditions.
Surprisingly the test copy was not bad at all. I copied all images except for the third and seventh. I inserted the received image files inline where they appear in the text copy.
Here Goes, Warts and All:
Welcome to program 229 of Shortwave Radiogram.
I’m Kim Andrew Elliott in Arlington, Virginia USA.
Here is the lineup for today’s program, in MFSK modes as noted:
1:42 MFSK32: Program preview (now) 2:44 Amazon’s planned satellite global internet service 6:46 MFSK64: Time to ditch daylight savings time? 10:00 This week’s images 28:14 MFSK32: Closing announcements
Please send reception reports to email@example.com
Amazon to launch prototype satellites for global internet service
By David Szondy November 02, 2021
Amazon announced today that it is going ahead with Project Kuiper, its rival to SpaceX’s Starlink orbital global internet service, by launching a pair of prototype satellites into low-Earth orbit next year. Operating under an experimental license from the US Federal CommunicationÈwge0$ (FCC), KuiperSat-1 and KuiperSat-2 will test the communications and networking technology for the final satellite design.
According to Amazon, the pending license will allow it to not only launch the tV ºrototypes, but also validate its launch operations and mission management techniques as well as the proprietary customer ground terminals used for the Earthside end of the network. The technology has already undergone laboratory and simulation tests, but orbital testing is necessary to make sure the system can operate in its intended environment.
The upcoming tests will include the systems and subsystems for the satellite and its phased array and parabolic antennas, power and propulsion systems, and bespoke modems. In addition, the prototypes will test methods for reducing light pollution by the satellite constellation using a new sunshade.
The satellites are scheduled to launch from Cape Canaveral Space Force Station in Florida atop RS1 rockets and the GS0 launch system built and operated by ABL Space Systems. The prototypes are designed to reduce space debris by actively deorbiting at the end of the mission so they burn up in the Earth’s atmosphere.
Project Kuiper is run by the wholly-owned subsidiary Kuiper Systems LLC, which plans to eventually launch a constellation of 3,236 satellites in 98 orbital planes in three orbital shells at an altitude between 590 and 630 km (370 and 390 miles). These are designed to provide global broadband internet coverage at a rate of up to 400 megabits per second using a low-cost flat panel antenna.
“Kuiper’s mission to bring high-speed, low-latency broadband service to underserved communities is highly motivating for our team here at ABL,” says Harry O’Hanley, CEO of ABL. “Amazon will play a central role in the next generation of space infrastructure, and we’re proud to have been selected as their launch partner for these critical early flights.”
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Is it time to ditch daylight saving time?
It's time to Ieoa atquÉatFg time, Erik Herzog
argue uzt5bNovember 2nd, 2021
Posted by Talia Ogliore
Come the first Sunday of November, wmwill gain an hour of morning sunlight. The one-hour adjustment to the clock on the wall may not sound dramatic. But our biological clock begs to differ.
Take, for example, the members of society blissfully unaware of social time: our youngest children and pets. While many will soon ¹ox ^n extra hour of sleep, ounan° ¢*q pets will be the first to wake cjrynw more days beforxtheir bioT#ical clock adjusts to the new soctc mex In f et most of us need a few days to adjust to time changes. In the meantime, wtexo”ffer some consequences.
“Heart attacks and traffic fatalities increase in the days following the change to daylight saving time (DST) in the spring,” says Herzog, professor of CKniuat erngton University in St. Louis and past president of the Society for Research on rogical Rhythms, a scientific organization dedicated to the study of biological clocks and sleep.
Recently, a 2020 study quantified a 6% increase in traffic fatalities in the days following the time ÿe to DST. Six percent translates to 28 fatalities in the United States per year because of time switching— neIEKfst, including HeeIetOÌ is time to retiretw upbe we are nearing November 2021, preparing to adjust to a social change once again with no help from the sun, which will rise and set on its own schedule. What is holding us back from eliminating time changes?
Do we keep DST and enjoy more sunlight in the evening hours or standard time (ST) and wake up with the sun? We cannot seem toriVn“ee. ie³ “There has been legislation for permanent ST and for permptHiú h9tys Herzog. He advocates for keeping standard time. “There are currently 19 states considering 45 key pieces of legislation that would eliminate annual time switching. Some already have; Arizona a e.t1waii live on permanent ST.”
Saying goodbye to DST, and the summertime memories we associate with it, can be difficult. But Herzog reminds us that we need sun in the morning.
“Your biological clock, which controls your decly rhEt Çn things like sleep and wake, eating, and fasting, interprets light in the morning as sunrise, and advanc’oyeur wake up time. Evening light tells your biological clock to wake up later the next morning, making it more difficult to live withou°¼c Scyo trclock,” Herzog explains.
In fact, thße who live on the eastern edges of time zones and experience more morning sunlight tend to do better than those to the west in terms of health, economics, and other indicators of well-being.
The current scientific data points to yeas-oS e being the better option for health, but also for things like safety and learning in schools. Will children be safpgoing to school thelouSark in the morning? Does more sunlight in the evening deter crime?
Less than a month after Richard Nixon’s failed attempt to force year-round DST in 1974, leaders of public schools opposed the change after six deaths were directly linked to children going to school in darkness. Meanwhile, data do not show that there is less crime during DST or more crime in states like Arizona and Hawaii on permanent ST.
But Herzog points out that we need more data. In the emvw¿/m, the health benefits of permanent ST are clear. Ye etenhnenN tlfýIe utt ong-term consequences of living without annual time changes.
“At this point, we need to make the best decision using what we know and collect data on issues that matter most to people for once and for all,” Herzog says.
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The reason why I would bother with this topic is twofold: One: I think better antenna systems are actually better; and Two: Technical concepts are central to amateur radio and should be understood and employed as often as possible. I’m discussing these antenna concepts in simple terms in the interest of keeping it accessible. Hopefully it leads to some further investigation and a different way to think about antenna systems.
WHAT IS RESONANT?
In the Venn Diagram world it can be said: Not all 50 Ohm feedpoints are resonant, and not all resonant radiators present 50 Ohm feedpoints. I have seen much confusion between “resonance” and “impedance match” on internet forums/platforms/videos. This what drove me to churn out this post.
Resonance in an RF radiator actually does make a difference. I’m a fan of Hemholtz and resonance is a real thing. When I assess a antenna design I start at the radiating element or elements. If that element is not a known and desirable harmonic relation to the fundamental frequency of interest I consider it a non-resonant design. If there is a matching unit connected to a non-resonant radiator I consider it a tuned circuit. When the goal is efficient and predictable RF radiation you have resonant radiators, and then everything else.
Recently there has been an explosion in the use of end-fed wire antennas. I use a few of them and they are an easy way to get on the air, usually on multiple bands. I have made plenty of contacts on these antennas, but at no point was I under an illusion that I was using an efficient antenna system. The now ubiquitous End Fed Half Wave is a strange bird, It utilizes a half wave radiator with a feedpoint impedance of about 3000 ohms, and is operated without a traditional ground plane or counterpoise. The high impedance feedpoint is matched to somewhere near 50 ohms with a 49:1 or similar toroidal un-un transformer. That is not a recipe for efficiency. The power ratings on the matching transformers tell you all you need to know: These matching units get hot, and that heat is your RF not making it out into the world.
That’s not to say it’s a bad design. It solves a few of the issues that keep many hams from being able to get on HF. You can hang it from a single support, as opposed to needing two or three for a horizontal dipole. It’s also easy to erect on demand, which is great for hams who want to operate portable stations or if they have a compromised (small, HOA, etc…) QTH. I use a 12m Spiderpole and a PAR Trail Friendly when Inwant to get on the air quickly. Also, thanks to the magic of harmonic resonance, it is common to find a match on more than just the fundamental frequency.
Another common design is the random length end fed, usually known by the 9:1 un-un transformer used to feed the non-resonant radiator. The trick here is to find a radiator length that is not resonant on any band you want to work. The hope, and I do mean hope, is that the feedpoint impedance will be somewhere in the 200-800 ohm range, where it can be matched to 50 ohms using a second matching device. Again it has the advantages of ease of setup and multiband capability. The tradeoff is even steeper than the HWEF. This design is force-feeding a non-resonant radiator, has an even lossier (IMO) un-un, and requires a second matching device to get all the way to 50-ohms.
A problem both designs share is the difficulty in modeling a radiation pattern. Even with many analyses and many users over many years nobody seems to be able to say much beyond “omnidirectional”. That’s not too helpful. The main issue in modeling these systems is properly representing the ground/counterpoise. Most installations (mine included) require a common mode choke (CMC) near the radio end of the coax to keep RF from energizing the radio’s earth ground. How efficient does that sound? Do we have any idea what these antennas are actually doing wit the RF that makes it out into the world? Empirically I think we do. Scientifically, predictably, I don’t think we have a good handle on it.
So, how important is the efficiency of a transmitting antenna?
Hams with even some basic experience on HF know that you can make contacts on almost anything. Take a simple transmatch design like the MFJ-901, hook it to a rain gutter, and make a contact. Do we know anything about the radiation pattern, efficiency, or bandwidth? No. We are just interested in forcing something conductive to radiate RF, and hope for the best. The magic of radio waves takes care of the rest. If enough of your RF makes it out in the correct direction you will make a contact. Your signal might even be strong! But this is where it helps to be aware of confirmation bias. The science of radio communications involves being able to control where your signal is going, and control the system design to connect you with the intended destination. Having made some contacts is almost inevitable. Making the contacts you want to make when you want to make them is where the game gets interesting.
In the food-chain of antenna designs these lossy designs are somewhere in the “krill zone”. A good efficient design, properly installed is somewhere in the “cordata zone”, and a very efficient directional design mounted high and in the clear with directional control is “blue whale” territory. At some point the operator is limited by their Effective Radiated Power (ERP) and the weakening of the transmitted signal with the square of the distance from the antenna. Using 10-30% of your RF to warm a toroid is cutting in to your effective range. Every system has limitations, but when running 10, 30, 50 watts at the finals, I feel that making the most of it is important. Every improvement in efficiency and pattern control brings you up another link in the radio food chain.
Certainly the parallel popularity of end-fed wires and weak-signal digital modes, best represented by FT8, are not coincidental. FT8 allows working at lower signal to noise ratios which is like getting that lost RF back when compared to working SSB or RTTY. More efficient antennas are always an improvement, but an entry-level HF rig, a HWEF, and WSJT-X is a great path of entry to the HF bands. I’ve gone on about this earlier, but there is nothing in-stone about needing to start with CW or SSB. Hams can get on the air, interact with DX, and get some good contacts in the log. I see nothing wrong with that.
Compact, Broadband, Efficient: Pick Two
In the HWEF and 9:1 design cases the user is giving up efficiency for a more compact, more broad-banded (lower Q) device.
The HWEF, thanks to its resonant radiator, is somewhat more efficient, but the price is being paid for getting wide frequency coverage on a single radiator. Some designs find ways to better balance the equation by sacrificing some bandwidth and band flexibility to increase efficiency. One QRP design I use is the PAR 102040 Trail Friendly. This design uses three techniques to get a three-band end-fed vertical into a single 41′ wire radiator package. Trick 1: It uses a trap to isolate the 20m half wave element from the 40M extension. Trick 2: It uses the characteristic electrical lengthening effect of the trap to keep the 40m extension (and overall length) shorter than a simple 40m half wave radiator. Trick 3: using the second harmonic of 20m to realize some usable bandwidth on 10m. The transformer is pretty much handling the design goal of representing a 3000 ohm feedpoint as a 50 ohm load to the rig. No additional trans match is needed if you have trimmed the 40m extension properly and are ok with the tuning points. It isn’t brilliantly efficient, but it’s not horrible.
Chameleon MPAS Lite – Mini Review:
In early 2021 I picked up that Chameleon MPAS Lite and wanted to give it a run as a portable antenna system for POTA. This unit is extremely compact and is comprised of a ground spike, a un-un, a heavy duty stainless whip and 65’ of wire to use as a counterpoise. With the engineering triangle in mind I knew I was giving up a lot of efficiency for a very compact, very broadband system. And that’s what I got. It works well enough, especially if you are calling CQ and self-selecting stations who can hear you. I found that replying to anything but the loudest stations was a bad recipe for success. In a Chameleon forum I made the comment that these antennas aren’t good DX setups. I stand by that. It isn’t that you won’t work any DX, you would just work more DX more easily with a better DX design. For mid-range and NVIS work I think it is a solid solution. That assumes you are able to make the contacts you need to make. Also, watch the power rating because the un-un will get warm, and will fail under excessive power and duty cycle.
The MPAS system uses a 5:1 un-un design to feed anything from their very nice stainless whip, MIL Whip system, a longwire, or whatever conductive item you decide to use. The 5:1 takes a conservative approach to the non-resonant radiator problem, and a second transmatch (internal or external unit) is required unless you get lucky and dial in a 250 Ohm (or 10!) feedpoint impedance for the Un-Un. Chameleon publishes a perfect omnidirectional pattern for their antennas. That’s a good assumption for the operator since non-resonant systems are difficult to model accurately. Just assume your RF is going in all directions equally. Might as well! In practice I have made contacts and successfully activated a few parks using the MPAS Lite. Chameleon builds a beautiful and rugged product, and supports their users well. II feel like it is a good system and the user will get the best out of it by realizing it’s strengths and weaknesses.
One concern I have from following a few antenna forums, including a Chameleon product support forum, is the number of users claiming to have “resonant” solutions. An actual resonant radiator would provide a terrible match with a 5:1 un-un. What users are doing is finding a radiator length that presents a 1:5 feedpoint impedance to the CHA transformer so the radio sees 50 ohms(ish). That approach may be usable on that band with no additional matching, but is likely to be worse on other bands.
Another constant question on these forums regards radials and counterpoises. Strangely the solutions discussed are often none, one, or several short radials. All of these are poor solutions. However, when the central design concept is to never be resonant, not require radials, and use almost anything as a radiator, I don’t know what a good solution looks like. The Chameleon counterpoise kit is 65′ of very hunky insulated wire and can help you play with the counterpoise dimensions/layout and maybe help in finding a match. That said I feel like users are trying resonant counterpoise lengths and I think that does more harm than good. With a single counterpoise, stick to the game plan. Why make the two impedances different?
The Chameleon 50′ RG-58-ish feedline with a ferrite bead choke on one end is a decent way to control the stray RF. And it is necessary. Every time I have used it I had to control RF that wanted to energize the radio’s earth ground.
The best application I have seen for these matching units is Chameleon’s own Tactical Delta Loop which uses the CHA as the feedpoint in a system where 5:1 isn’t a bad design value. I will be cobbling a test setup soon out of various Chameleon and Wolf River parts.
If it sounds like I am down on end-fed designs, I’m not. They have a proven track record and get hams on the air. What I would like to get across is that I hope ops get some time on other designs. Building a nice 1/4 wave vertical over a good set of radials is very easy and cheap. Think of a it as a single-band DX Commander style build. I think it is worth the time and small expense to see how a resonant design works and maybe make a few on-air comparisons.
If you stuck with this post I owe you a pint. I don’t write these to be concise blurbs. I like to compose my thoughts on these topics and I figure sharing it is part of the experience. Let me know what you think! Reply on the blog, or look me up on QRZ and drop me an email.
Get on the air, and always have fun. 73, Pete N1QDQ
Posted onJune 14, 2021|Comments Off on 2021 ARRL June VHF QSO Party – Recap
A Little Back-Story:
When I was first licensed in the early 1990’s I traveled a fairly standard ham radio pathway. I bought a Kenwood TH-78a (There were no ‘Fengs) and I already owned a few decent SWL rigs. I had access to all the test equipment I grew up with, and had my dad as a tutor on some electronics concepts. I needed that because I went from Tech to Extra in about 8 months. That also involved learning code. I passed the then-maximum 13wpm, but was able to pass a 20wpm for fun a few months later. The basics of VHF repeater operation and HF SSB/CW are still a large part of my ham radio experience. I also had interests like hiking, camping, road trips, and I liked to build antennas. It wasn’t long before I found out about VHF contesting, and the Rover classification. I worked with another ham, N1QVE, to assemble a rolling station and we did some good work in VHF contests in the 90’s.
I have been in and out of active ham radio operating for about a decade. It wasn’t until 2019 that I started thinking about improving my equipment and getting something better than my attic dipole for HF. I also had one eye on VHF all mode operation. I owned a Ten Tec Scout for HF mobile, and few of the Icom single-band VHF rigs like the IC-202/402/502 for VHF SSB/CW. Then I splurged and bought a “shack-in-a-box” Icom IC706, soon upgraded to the IC706-mkII, and that was my main radio for a few years. I’ve since owned a few of the Yaesu FT-857/817 family, and found them to be great radios. Looking around the catalogs in 2019 there were not many V/U All Mode options. I was running a Xiegu G90 (great rig) but it had no VHF+ capability. I decided on a Yaesu FT-919A and have been very happy with that radio.
2020 ARRL September VHF – Initial Low Drag Rover Concept:
In the summer of 2020, COVID-fever was at a max and any reason to get outside was a good reason. I used my free time to scout a few hilltop locations and figured I would give the ARRL September VHF Contest a go. The design restrictions were pretty simple:
Single Op setup, so everything had to be riggable by me, alone, quickly, in whatever conditions I dared operate in.
I ruled out operating on the road. I would only operate fixed. My days of running a recorder in the car and reviewing audio logs were well behind me.
No major gear purchases. I only do it for fun, so why shell out for an extra few DB here or there
Keep the rove manageable and fun. No slogging through vast stretches of highway in the dark of night for a possible grid activation.
I packed my 991A, my ELK LPDA, and a PVC mast on top of a PA speaker stand, and hit the road. I had a good time and actually racked up a respectable 2,325 points on SSB only, logging by hand, and only having a 5/8-wave 2m whip for 6m. This is how I learned to do it over 20 years ago, so why add more complexity for my first outing?
2021 ARRL June VHF – Lessons Learned
Over the nine months since the September contest I have put together a better portable setup for both POTA-style HF ops as well as VHF hill-topping and contesting. I built a wire Moxon for 6m and tried it out in the January VHF contest (a wind-driven washout), and liked it so much I purchased a PAR SM-50 Stressed Moxon and have been running it for a few months. I also upgraded my homebrew “tesla cell” LiFePO4 battery to a Bioenno 20A unit. As for my antenna rigging, some time in a hardware store with calipers netted me a 12-foot painter’s pole that is a slip fit to the ID of my speaker stand tubing. It also has an aluminum hex shaft which is perfect for the SM-50 mounting clamp.
I am still running RG-8X feedlines, and am not running any preamps, or power amps. This means I am making 50W max on 6m and 25W max on 144/432 with the 991A. It really is enough for the kind of operating I am doing. There is a huge spectrum between “stay home” and mega-rover. Even if the scoring system has no way to identify the details, I know my score came from single-handed barefoot operation with simple and affordable antennas.
I also made the switch to computer logging. While it *almost* violated my “no new gear on contest day” mantra, I picked up N3FJP’s VHF Contest logger and had enough time for a brief dry run before contest weekend. I knew I would have to work out the fine points under contest conditions, but I also brought a pad and pen JIC. I also ran WSJT-X to get me on FT8. I wish I had success with employing the multicast protocol because I missed having GridTracker, but maybe next time. TIP: Let N3FJP handle rig control. I lost mode tracking when I let WSJT-X control the rig.
VHF Digital Lessons/Issues:
I have been lucky enough to operate FT8 during some good 6M Es openings during May and June 2021. My experiences on HF FT8 translated very well. I was able to use the same techniques of moving my transmit frequency, strategic CQ calls, and so on. I expected things to work just as smoothly during the contest. Yes, there is one born every minute.
I had never operated WSJT-X in contest mode before and hadn’t really thought that through prior to the start of the contest. As I set up and started making a few pre-contest trial contacts it hit me that something was different. For one, the QSY on left pane double-click acts differently. As well I was having bad luck when replying to CQs while transmitting in a “clear spot”. I often had to reply on the calling station’s TX frequency. So while the potential for digging out more QSOs by working weaker stations was there, the reality was not so simple. I could have worked SSB stations much quicker, and “run the bands” much easier… if so many stations weren’t ditching SSB for FT8!
I put in a fair amount of time, at least 25%, working non-digital modes. There were times when I was making good contacts, and others where the CW/SSB was dead and FT8 was the only thing where a contact was possible. I was able to work W1AW and W1AN on 6M CW from Mowhawk Mtn. That was pretty cool. As much as I enjoy digital modes I do think the CW/SSB action is more enjoyable.
I decided to activate FN41,42,31,32 this year. The 1800Z start time for Saturday of the contest is a real style-cramper. I get it, but really? For a rover it leaves about seven total hours of daylight on Day 1. With many parks closing at sunset the decision to move locations cuts into a lot of operating time. My memories of driving through the night and only making a few new contacts, while hearing the same big-gun stations made the decision simple: Start on time, wrap it up at dark, get home, get some sleep, and put in a good shift in FN41 on Sunday.
Now that I live in coastal Rhode Island it makes the route-logistics a little more complicated. I started the contest in FN42 at a hilltop in Charlton, MA. That spot is great but they are all only as good as conditions (foreshadowing) allow. If I had just stayed there until dark I would have had a better overall contact/points total, but I was up for a drive and wanted to try a new spot for FN32.
After many different ops operating from hilltops in the NW Connecticut and Western MA area (FN31,32) it is hard to break that habit. They are good locations, but not perfect. That spot was the parking lot at Haystack Mountain in Norfolk, CT. It’s got a lot of trees blocking the RF/View, and the entire northern half of the azimuth is blocked by a mountain, but it isn’t terrible. Not great either. You get about 100 degrees of actual azimuth to play with from maybe 120-240 degrees.. Next was Mowhawk Mountain in Cornwall, CT. Mowhawk is a great location, but there is a lot of RF equipment up there and noise/intermod levels can by nasty. Bring your bandpass filters! Neither location “popped” but I did activate the grids and get a few new worked grids in the log. All in all not worth the drive (points-wise), but on this beautiful June day the drive was spectacular.
I had a nice time operating on Sunday from FN41. A local high-ish spot at a local farm field gave me plenty of elbow room and a safe off the road location to operate from. The RF conditions were not super. Normally I’d be ok with hearing some distant grids but not being able to work them. I wasn’t even hearing that! It was a grind. I did manage to get some good runs on 6m and 2m, add a few worked-grids, and even snag some DX with a VP8 and an EA7. What we had here in the northeastern US was a nice opening to Europe! Even then I wasn’t hearing too many Europeans. It was just a soft day on the bands. After about 5 hours I worked a nice run of locals on 2M FT8 and called it a day.
It wasn’t a terrible contest. For the type of operation I describe here it was a success. It looks like I tallied just north of 3,500pts, activated four grids, and put on about 300mi. Those are Southern New England Miles. It’s like dog years compared to other parts of the US. I think it’s fair to say conditions for this contest didn’t favor my low power setup. I was counting on a strong opening to the mid-west or southeast and it never materialized. Fun was had. I’m looking forward to the next one.
Rovering is a great way to wring out your mobile/portable setups. I feel like my POTA setup got better, and I have a few ideas for improvements.
Something was very odd with beam headings. I felt like I was way off heading on a few contacts where I set the beam heading by ear.
Also, setting the beam heading on FT8 while armstrong-ing the mast with one hand and reading the screen and running a mouse is not easy. Ideally I would watch the waterfall and try to peak a station visually. Easier said than done.
I ran my 20A LiFePO4 DEEP into the cycle and it held up beautifully. I have a Bioenno 1503CAR for charging on the go. It helps to recover charge but won’t fully recover the charge on a short drive. The way to go is probably switching between 2x20Ah, or just a 50Ah cell.
It’s a fun way to get out and play on the high bands. Give it a shot even if all you have is a FM rig and a small beam. If nothing else use an all mode receiver (SDR is a great way to go) and monitor the high bands during a contest. It’s a good way to hear HF-band levels of activity on VHF+ and you might get motivated to join in.
Comments Off on 2021 ARRL June VHF QSO Party – Recap
Preface: I am planning on creating some posts addressing this in a more technical fashion. This is not a comprehensive tech essay full of footnotes. You either know what this is about or you don’t. For now I am sharing this brain dump addressed to all amateur radio operators. We find ourselves in a unique circumstance where great changes have occurred over a long period of low solar activity, and we are now emerging with some very real social turbulence in the ham radio ranks. I think it is useful to take a broad view of this pursuit, this service, and reflect on how we have moved forward, and how we can continue to move forward. 73, Pete N1QDQ
Let’s travel back to the heady days of 2010, when a new ham radio sensation called PSK31 was “taking over the ham bands”. It allowed users with less than massive transmitters and antennas to make reliable keyboard to keyboard contacts on HF. It wasn’t perfect. Many ops ran too much power, or had overdriven signals, or both, and the small stations had a bit of work to do to get through a QSO. The spectrum slices being used were narrow/cramped, and it didn’t take much to interfere with another op. You pretty much had to be on the same frequency/offset as the other station (not reliable in split mode) or it didn’t work, and a big wooly signal would wipe out a quarter of the subband. The advantage was that it took up about a tenth of the spectrum of a RTTY signal, and was more power-efficient. It also allowed many more operators to share the same slice of spectrum. As is the case today it was also a reason for the “big gun” stations to sneer down their noses and tell “lesser’ operators how they were killing ham radio.
FFW to today, and we are in much of the same predicament with a newer mode called FT8. It is even more flexible than PSK31, works at even lower signal to noise ratios, and is implemented primarily through one application called WSJT-X. It does not support anything much beyond the bare bones exchange of callsign, location and signal report. That makes sense since the suite of modes associated with Joe Taylor K1JT, Steve Franke, K9AN, and a cadre of experimenters was developed for very weak signal operations like Earth-Moon-Earth (EME) and Meteor Scatter. It turns out some of these modes, specifically FT8 and FT4, are very robust over traditional HF frequencies and propagation modes. And yet, despite allowing a large number of contacts over a small slice of spectrum, with lower power, and lower s/n ratios, FT8 users are again subject to ridicule by keepers of the mid-20th century technology flame. This extends to purposeful QRM, sneering memes about how FT8 ops are not real hams, how their QSOs don’t count, how it is “cheating”, and so on. Even as predictable as it is, it puts the ugly side of the “friendliest hobby” at the forefront of the much needed conversations around how our spectrum allocations are utilized, and how they will be used going forward.
Which is a shame, because these computer-controlled weak signal modes on the HF bands are nothing if not entirely consistent with the traditions of ham radio, and the central thesis of evolving to incorporate new technology as it emerges. The integration of existing and new technologies into radio communication is the hallmark of ham radio. What began as the transmission of Morse Code (tech adapted from the wired telegraph industry) using a spark gap transmitter, quickly evolved to a continuous-wave (CW) transmission based on the implementation of the vacuum triode as a tunable oscillator and amplifier. The spark-gap blasted RF across a big slice of RF spectrum. CW turned that on its head and allowed for more efficient narrow-band communications. Suddenly there was more room for more operators to communicate with less power over longer distances.
When modulated carrier audio came into being, it was double-sideband full carrier amplitude modulation, or AM. This is what we hear when we listen to the AM broadcast band. It takes a lot of power to generate that signal, and it also takes up a lot of spectrum. As the need arose for more efficient communications modes (portable equipment, lower power requirements, covering greater distances) it was found you could do away with the carrier (which was the reference frequency for the audio sidebands) and then one of the two sidebands. Thus Single Side-Band (SSB) was created. By giving the receiver the necessary oscillators to rebuild the audio information, the transmission could be made using much less power. This mode relied on the many improvements to vacuum tube technology, including miniaturization, lower power circuitry, and the use of multiple oscillators in new configurations. These fundamental modes of radio communication, data and audio, integrated new technology as it appeared, and hams were pivotal in their widespread adoption. As well, hams were pivotal in the development of new modes of radio communication based on these principles. They were, as now, radio experimenters. They were doing for free what governments were doing under much less liberated circumstances.
Radio technology eagerly adopted every advance in electronics tech, from vacuum tube minaturization, to the semiconductor, the integrated circuit, the standardization of component packaging, and then the microprocessor. Microprocessors were a natural fit for radio communications because they can manipulate control voltages and logic states at a blinding pace. The earliest and slowest microprocessors were adding communications capabilities beyond the analog realm. It also turned out you could emulate an oscillator with a microprocessor. Even at audio frequencies this was a giant leap for oscillator miniaturization and stability. Once these microprocessors were integrated into computing platforms, handling user input, program code execution, data storage, and data output, the modern era of computer/radio hybridization was in play.
It is simple enough to state that a radio station operating without some form of semiconductor and microprocessor technology is indeed a rarity. I know of no hams who are aching to go back to drifty oscillators and inefficient transmitters. Yes, that gear is still in use by a few stations, but I’ll bet each one has a modern rig right next to it. While modern technology has come to dominate the scene, all of the historical phases of electronics technology still have a place in the pursuit of radio communications (ok, maybe not spark gap). The fundamentals of radio still apply regardless of the technology.
So I ask, earnestly: How did this illustrious, enjoyable, and diverse pursuit of technology applied to radio communication become beholden to gatekeepers who selectively decide which modern technology is appropriate, and which they believe makes one a “fake ham”? It is almost universally the cry of hams who are “fortunate” enough to have a tower(s) supporting a big directional antenna(s) fed by a kilowatt(s) of RF, using modes established in the WWII era, who demand that they be crowned the gatekeepers of What Is Correct.
The facts are decidedly at odds with their position. If they were in any way in the majority it would be reflected in radio equipment sales and development. I believe the “average” ham has a somewhat modern 100W transceiver with a simple antenna, and a few helpful accessories. Additionally, they own a computer, which has become not only extremely cheap, but extremely effective. Somehow, in the middle of a deep and prolonged solar minimum, the airwaves are increasingly being used by many low power stations using compromised antennas, often with portability in mind. One reason this has been possible has been the development of modes like FT8. When you can run a 1-30W transceiver into a $20 homebrew end-fed wire, controlled by a $50 Raspberry Pi “toy” computer, and make a contact 10,000 miles away, it opens up the accessibility of radio communication in a myriad of ways. I made my first JA contact from my new QTH using 35W into a wire vertical, and FT8. It’s just as valid as any other contact.
I agree that the FT8 QSO is not very satisfying from a “chat about the weather and your radio” perspective. But let’s be honest, a typical CW conversation is name, location, rig, antenna, and brief weather observation. It’s fun. I love it. But it isn’t exactly deep bonding going on there. FT8 is giving the user more of a “contest mode” QSO. Being that it is good enough for the biggest stations in the world, as long as an actual contest is afoot (every weekend, #jussayin), why is it less appropriate in weak signal work? Maybe it’s has to do with the fear of losing status? Maybe it’s the need to ensure that kilowatt stations using 80 year old tech continue to dominate the way hams use their HF spectrum allocations in the 21st century? I can understand it, objectively, though I have not been able to assemble that kind of station. I also understand bullies. All too well. Ham radio needs to face up to the fact that it has a bully problem.
Unless you have been under a rock you know that every slice of the radio frequency spectrum is being eyed by some monied interest somewhere across the globe. Each time you see a nation kick their amateurs off an allocation it should raise an alarm. One would think the response of established spectrum users would be to promote increased usage and improved spectrum efficiency. It is counterintuitive to act as if relying more heavily on old tech is some kind of hedge against spectrum loss. I also fear that hams hold themselves to a standard that is not recognized outside of ham culture. An objective survey of the HF allocations would hear a small segment of intense activity in the bottom 100KHz, and then a lot of SSB voice spread out across the rest of the allocation.
My purpose here is to begin a conversation not end one. This is the scenery as I see it, from my perspective as a ham who has held an Extra Class license for almost all of my 27+ years of ham-life. I am often operating portable equipment, often at QRP or slightly higher power levels. I try to enjoy all that ham radio has to offer. I like HF QRP CW, as well as digital modes, as well as VHF/UHF contesting, as well as SSB, and SWL, and applied electronics concepts, and so on. I feel that there is a disturbing social pushback on the current practices and adaptations many hams have made in the era of condo rules, suburban/urban constraints, restricted public space access, and accommodating family and work life, by a small population of operators who don’t share those constraints. All of the tools available to hams have a place. And it is a great credit to hams everywhere that there is a general respect for gentleman’s agreements and international spectrum guidance. What I hope we see as this next solar cycle heats up is not just continued cooperation, but greatly enhanced cooperation. There is room for everyone, and every facet of the hobby. There has to be. The alternative is unimaginable, avoidable, loss.
Endnote: One piece of Amateur Radio News that spurred me to write this piece is this: FT8 Ruling The Airwaves from DXWorld.net. I believe it shows how a more efficient mode of communication increases the effectiveness of the power output on hand, and how attractive that is to many hams. I don’t think it is more complicated than that.