In the park with 5 watts, KX3 and new Endfed antenna
| My outdoor shack |
| Golfball setup |
10m Frequency SWR
28.020 3.8
28.060 3.8
15m
21.020 2.9
21.060 2.9
20m
14.020 3.8
14.060 3.8
40m
7.020 8.4
7.040 8.4
The antenna was mounted in a sloper configuration the high end at about 20 feet off the ground and the other end ground mounted. The tuner in the KX3 was able to bring all bands but 40m to a flat match, I was able to get 40m down to 1.5. The bands were very quite but I did spend some time
| Anchor point |
Mike Weir, VE9KK, is a regular contributor to AmateurRadio.com and writes from New Brunswick, Canada. Contact him at [email protected].
6m Es – Is It Changing?
With the summer Sporadic-E season now approaching its midpoint, it looks as though this year may be another poor one. Having been operating on 6m every summer since the early 70's, I'm beginning to believe that we may be seeing some changes in what was once the normal summer pattern.
This summer, I can count on one hand, the number of good solid openings ... openings lasting for several hours. Over the past forty plus years, summers on 'six' for me, here in southwestern BC, were usually very predictable. The last week of May would usually see the start of regular band openings that would quickly escalate to almost daily openings through June and July. It was not uncommon to see the band open all day, into the very late hours and then still be open the next morning. Intense Es from California predominated the 70's and 80's ... much different than the past several summers here. The stronger openings now, when they occur, seem to be more to the southeast, favoring Colorado and other nearby central states. At times, this will turn into double-hop to the southeastern states, usually favoring the 'EM' grids.
Really long-haul openings have also taken on a different flavor. For more than two decades, openings to Japan on Sporadic-E almost always occurred late at night, near midnight ... late afternoon for the JAs'. The openings rarely favored anything other than the west coast. Openings to Europe from the west coast were, for the most part unheard of, and any claims of summer-time EU contacts were often dismissed as 'wishful thinking' and not taken too seriously.
A huge shift in long haul Es over the past decade has pretty much re-written the rules of what we have always taken to be 'normal'. Summertime openings to Europe, from the west coast, have now become a regular expectance and, although still rare and usually short-lived, somewhat dependable. Our midnight openings to Japan have largely disappeared ... replaced by hour-long, mid-afternoon or dinner-hour JA runs, and more often than not, right over our west coast heads to any U.S. call district fortunate enough to be in the propagation's hot-spot. All of this is so very different than the 70's and 80's!
So why are things different now? Is it subtle influences from our ever-changing sun?

We are now heading into our sixth straight day of a spotless sun, but in reality, solar activity has been slowly winding down for the last several years. Long term studies tend to show that the solar cycle has little effect on summertime Es, but maybe not.
Is it climatic change ... global-warming? The e-layer is supposedly high above any weather influence yet there is evidence pointing to Es being associated with lightning storms and high altitude plasma-driven sprite activity. Maybe global-warming includes ionospheric changes as well and perhaps weather plays more of a role than previously thought.
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| Courtesy: http://www.astrosurf.com/luxorion/qsl-perturbation.htm |
Is it changes in equipment, with an ever-increasing number of 6m stations sporting huge antenna systems and higher ERPs' than ever before?
| Six 7-el Stacked Yagis At W7EW |
Maybe it's the influence of the Internet on operating practices? There is no doubt that having the ability to watch and follow realtime propagation paths, by the very minute, has made a huge difference in operating strategies ... along with big payoffs when it comes to catching those fleeting openings that would likely otherwise have gone unnoticed. On more than one occasion, I have worked Europeans on a seemingly 'dead band', with no propagation indicators at all ... just an announcement on the Internet that said station was calling 'CQ' at the time. Perhaps nowadays, there are just more savvy operators with good stations and a much better understanding of the DX possibilities ... slowly wringing out the best of what 6m has to offer. Maybe it's a combination of several factors.
Let me qualify my observations by saying that these have been my experiences and perhaps unique to the PNW and southwest VE7 only. Longtime Es data-collector, WA5IYX (Pat) in Texas, graphically shows the yearly Es variance in his region. The pattern appears somewhat sinusoidal in nature over the past few decades, but except for the occasional 'stinker', the variances from one summer to the next are not huge.
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| Annual Es At WA5IYX courtesy: http://www.qsl.net/wa5iyx/ |
Are my observations similar to what you may have observed over the past many years? Are the changes real or only imagined? As with most global events being driven by mother nature and continually dynamic, I see no reason why 6m propagation should remain constant from decade to decade ... but I'd sure like to see a little more of it.
Now, usually when I voice complaints about our bad 6m propagation, it seems that things often flip from terrible to amazing soon after. The best Es of the summer often peaks in or close to the first week of July, now fast approaching. Let's hope that this is one 'constant' that hasn't changed as well!
**********************************
Wouldn't you know it. I put above blog together on Tuesday evening, intending to publish it on Wednesday. Early Wednesday morning, before 0900 local time, several Europeans were worked on CW ... perhaps the propagation gods were looking over my shoulder?
As is so often the case with these relatively new types of openings between EU and the west coast, there were no particular propagation clues from this end, other than a brief reception of the KØGUV/b in Minnesota. I was only alerted by the EU propagation reaching as far west as Colorado (KØGU) and a posting on the ON4KST 6m propagation logger that K7RWT in Oregon was hearing the VA5MG/b, sometimes a precursor to PNW propagation over the pole. The propagation map at the time shows no real indicators out this way ... once again, the value of realtime prop-watching via the Internet seems to have played a big role in finding these types of openings.
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| courtesy: http://www.on4kst.org/ |
Steve McDonald, VE7SL, is a regular contributor to AmateurRadio.com and writes from British Columbia, Canada. Contact him at [email protected].
Field Day – ’29 Style!
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| courtesy: WA3TTS & NO3M |
In Eric's own words:
I had a 1920/1930s style Field Day setup this weekend and a bunch of guys over. 80M doublet with homebrew open wire line (approx 550 ohm), the transmitter was a 27-24-24-865 job more or less straight out of July 1931 QST, but with a Hartley instead of crystal oscillator. 27 tuned to 80M, first 24 to 40M, second 24 also 40M, and the 865 on 40M. About 10W. Never did get a chance to try her out on 20M by using the second 24 as a doubler.
I also built the complementary amplifier using a 203A from the August 1931 QST article. I had not even tested the amplifier, only having been finished at 1AM Saturday morning!! It is somewhat different in that the grid circuit is composed of the driving rig's antenna coupling coil/cap, re-wired to be in parallel, not series, of course. It was coined as being a good amp for any existing power oscillator or MOPA, We did a quick job of neutralizing while the gang was here and fired it up..... no modern measurement devices in sight, so we were only going on RF current. 0.9 amps into 50 ohm (pre-tuned the homebrew link coupled, balanced tuner with an analyzer beforehand)... so about 40 watts. I was hoping for 100W.... anyways, after most guys left, a couple of us starting messing around with it more, mainly tightening the output coupling of the MOPA and amp tanks. NICE! 1.45 amps, ie. 105W on 40M.
Anyways, I'll have a full writeup and photos on my website in a few days. We used an HRO5 for a receiver; everyone commented on how good it sounded and well it handled. Of course, this is from a bunch of guys that grew up with this stuff and/or has owned one at one time or another. Everyone had a great time and lots of good discussion and visiting, including 153 QSOs with that pile of junk!
73 Eric NO3M
Most will agree that Eric's station is far from a "pile of junk" as his superb homebrewing skills are clearly evident! Setting up this old style gear can be challenging at any time, but doing it for an outside weekend operation must have been a ton of work. Well done Eric!
For more information about building and operating '29-style transmitters, see the links on my blog sidebar.
Steve McDonald, VE7SL, is a regular contributor to AmateurRadio.com and writes from British Columbia, Canada. Contact him at [email protected].
Weekly Propagation Summary – 2016 Jun 27 16:10 UTC
Here is this week’s space weather and geophysical report, issued 2016 Jun 27 0346 UTC.
Highlights of Solar and Geomagnetic Activity 20 – 26 June 2016
Solar activity was very low during the entire summary period with only B-class flare activity observed. No Earth-directed CMEs occurred.
No proton events were observed at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit reached high levels on 21-22 Jun and 25-26 Jun following coronal hole high speed stream events. Normal to moderate levels were observed on the remaining days.
Geomagnetic field activity was quiet on 20-21 Jun. Mostly quiet conditions were observed early on 22 Jun but activity increased after 22/1800 UTC due to enhanced solar wind parameters and unsettled to minor storm levels were observed. Quiet to unsettled conditions with isolated active periods were observed on 23-24 Jun due to negative polarity CH HSS effects. Quiet to unsettled conditions were observed on 25-26 Jun with an isolated period of active conditions observed from 26/2100-2400 UTC due to CH HSS effects.
Forecast of Solar and Geomagnetic Activity 27 June – 23 July 2016
Solar activity is expected to be very low throughout the forecast period with a slight chance for C-class activity.
No proton events are expected at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at high levels from 27 Jun to 01 Jul following CH HSS effects. Normal to moderate levels are expected on 02-03 Jul as a CIR redistributes electrons. High levels are expected to return from 04-07 Jul following a recurrent CH HSS. Moderate levels are expected from 08-21 Jul followed by moderate to high levels on 22-23 Jul following another recurrent CH HSS.
Geomagnetic field activity is expected to begin at unsettled to active levels but decrease to mostly quiet levels by midday on 27 Jun and remain quiet through 29 Jun. Quiet to unsettled conditions are expected from 30 Jun to 05 Jul with isolated active conditions possible on 03 Jul due to a recurrent negative polarity CH HSS. Quiet conditions are expected on 06 Jul. Quiet to unsettled conditions are expected from 07-12 Jul with minor storms possible on 11 Jul and active periods likely on 12 Jul due to effects from a recurrent positive polarity CH HSS. Mostly quiet conditions are expected to return from 13-18 Jul with unsettled periods possible on 14-15 Jul. Quiet to unsettled conditions are expected on 19-21 Jul due to negative polarity CH HSS effects with an isolated active period likely on 19 Jul. Quiet conditions are expected for the remainder of the period.
Don’t forget to visit our live space weather and radio propagation web site, at: http://SunSpotWatch.com/
Live Aurora mapping is at http://aurora.sunspotwatch.com/
If you are on Twitter, please follow these two users: + https://Twitter.com/NW7US + https://Twitter.com/hfradiospacewx
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Visit, subscribe: NW7US Radio Communications and Propagation YouTube Channel
ICQ Podcast Episode 214 – Calibration
In this episode, Martin M1MRB / W9ICQ is joined by Leslie Butterfield G0CIB and Matthew Nassau M0NJX to discuss the latest Amateur / Ham Radio news. Colin M6BOY rounds up the news in brief, and this episodes feature is Calibration.
EURO 2016 Amateur / Ham Radio Award
Ofcom Remove Amateur / Ham Radio Statistics
White House honors Limor Fried AC2SN
Russia Trial Electromagnetic Warfare System
FCC Technological Advisory Council Noise Floor Inquiry
New National Belize Amateur / Ham Radio Society
RadioShack Photography Competition
ZS1TWO Cape Town 2m Beacon
Colin Butler, M6BOY, is the host of the ICQ Podcast, a weekly radio show about Amateur Radio. Contact him at [email protected].
ICQ Podcast Episode 214 – Calibration
In this episode, Martin M1MRB / W9ICQ is joined by Leslie Butterfield G0CIB and Matthew Nassau M0NJX to discuss the latest Amateur / Ham Radio news. Colin M6BOY rounds up the news in brief, and this episodes feature is Calibration.
EURO 2016 Amateur / Ham Radio Award
Ofcom Remove Amateur / Ham Radio Statistics
White House honors Limor Fried AC2SN
Russia Trial Electromagnetic Warfare System
FCC Technological Advisory Council Noise Floor Inquiry
New National Belize Amateur / Ham Radio Society
RadioShack Photography Competition
ZS1TWO Cape Town 2m Beacon
Colin Butler, M6BOY, is the host of the ICQ Podcast, a weekly radio show about Amateur Radio. Contact him at [email protected].
Amateur Radio Weekly – Issue 117
Field Day 2016 is upon us!
Sean, KX9X, Media and Public Relations Manager for the ARRL comes by to share the League’s perspective of the event as well as some tips and tricks to make this Field Day one to remember.
HamRadio360
Field Day 2016 site locator
To find a location near you, type in your town and state in the Location or Call Sign box on the left.
ARRL
It’s Field Day weekend 2016: find a local event, have fun
If you live in North America and have an interest in becoming a ham radio operator, this is the weekend to check out what amateur radio is all about.
The SWLing Post
Are you ready for Field Day?
I’ve been working on my set up for portable HF operations for the last couple of months. It is nothing elaborate or even remotely fancy. It does work and that is good enough for me.
N0RVS
VLF, LF, MF experimenters will transmit ARRL Field Day greetings
A number of Experimental (Part 5) licensees — nearly all of them radio amateurs — have been plying the depths of the radio spectrum as the ham radio community awaits FCC action on the new 2200 and 630 meter bands.
ARRL
Field Day 2016: Activate Off Grid Systems!
Be flexible and understand that Field Day means different things to different people. For some, it’s a serious disaster preparedness drill. For others, it’s a contest, a public outreach effort, or a picnic in the park with radios.
Off Grid Ham
Checklist for a GOTA station
So, I don’t forget to bring anything, I thought I’d come up with a checklist for the station.
KB6NU
Special event station K1D to operate satellites on Field Day
In an effort to encourage more kids and their families to get involved in the hobby, the kids at Ham Radio (dot) World are working to put an all-kids Special Event ARRL Field Day station on the air.
Southgate
“Amateur Radio Week” proclamations abound in advance of Field Day
Several states, counties, and communities across the US have officially recognized the public contributions of Amateur Radio.
ARRL
New Mexico wildfire emergency threatens some Field Day sites
Amateur Radio Emergency Service (ARES®) volunteers in New Mexico late last week responded to the Dog Head fire, which is affecting Torrance and Bernalillo counties, and that activation continues.
ARRL
Field Day 2016 rules [PDF]
Field Day is open to all amateurs in the areas covered by the ARRL/RAC Field Organizations and countries within IARU Region 2. DX stations residing in other regions may be contacted for credit, and may submit entries as check-logs.
ARRL
Amateur Radio Weekly is curated by Cale Mooth K4HCK. Sign up free to receive ham radio's most relevant news, projects, technology and events by e-mail each week at http://www.hamweekly.com.




















