ICQ Podcast Episode 216 – DA0HQ Contest
In this episode, Martin M1MRB / W9ICQ is joined by Edmund Spicer M0MNG, Chris Howard M0TCH and Ed Durrant DD5LP to discuss the latest Amateur / Ham Radio news. Colin M6BOY rounds up the news in brief, and this episodes feature is an interview with the organisers of the DA0HQ Contest site.
- Malaysian Amateur Radio Licences Changes
- BBC Starts Roll-Out of International Radio App
- US Ham’s Save Kids from Surrounded Campfire
- Earthing and the Radio Amateur
- Ofcom Proposes Ham Band for Wi-Fi
- UK Amateurs Visit 10 Downing Street
- AES Ham Radio Store Closing Down
- New European Table of Frequency Allocations
- Australian Radio Operator Fined and Off Air
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 121
Radiosport vs. Pokémon GO
It should come as no surprise that ham radio operators are drawing comparisons between Pokémon GO and Amateur Radiosport.
ARRL
Growing 6m JT65 activity
On several occasions this week, I have heard or worked dozens of others on JT mode while the bottom end of the band appears void of signals.
AmateurRadio.com
North Korea activates numbers station
A female announcer at the radio station read numbers for two minutes on 24 June and 14 minutes on Friday.
The Guardian
What’s In your rubber duck?
I often refer to the rubber duck as The World’s Most Convenient Crappy Antenna.
K0NR
Life as a blind radio Ham
Anyone can join in the conversation and sometimes you find yourself talking to a dozen or so people across the ends of the Earth.
Largs & Millport
Smartphone vibration motor as microphone
Two researchers from the University of Illinois at Urbana-Champaign have devised a method for turning vibration motors, like the ones found in smartphones, into makeshift microphones, capable of recording the sound around them.
Southgate
How to: GPS spoofing (to hack Pokémon GO)
As satellite GPS signals are very weak while receiving on earth, transmitted signals with the HackRF will be very strong in comparison
Insinuator
A speaker mic NOT to buy
I’m guessing this one didn’t pass through quality control, if there is such a thing at the Baofeng factory.
Digital Mobile Radio
Receiving WSPR with RTL-SDR
Direct sampling mode allows you to receive HF signals on an RTL-SDR without the need for an upconverter
RTL-SDR.com
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.
2016 Summer Trip – Day 55
Wind Cave National Park, South Dakota. Devils Tower National Monument, Wyoming.

Friday, July 22nd – Toured Wind Cave. Once we entered the cave and started to descend, Emily was scared at first but then was ok. After the tour, the girls finished up their Junior Ranger books and received their badges for Wind Cave.
The day started getting hot. The expectation was temps into the upper 90s. I had gotten a prime parking spot in front of the Wind Cave Visitors Center which allowed me to connect to their wifi. I used the wifi connection to make reservations at the Devils Tower KOA. The heat made me want to camp at a location where we could make use of our air conditioner.
We left the Elk Mountain Campground around 1pm. Elk Mountain Campground is a good place to camp if the weather had been a bit more cooperative. I was disappointed in the lack of any substantial Ranger-led evening program.
It was a nice drive in a northeast direction through a national forest to I-90 where we were only on I-90 to go up one exit. Checked into Devils Tower KOA (located immediately outside the monument) and had some food across the street at the trading post. Ended up getting a pull-thru site next to another ham (KF5SA). He has an HF station mounted inside his trailer.
Quick trip up to the visitors center to get Junior Ranger books (from Ranger Erin Cahill). Attended evening program at the campground amphitheater which was blown out by bad weather into the picnic area.

Scott Hedberg, NØZB, is a regular contributor to AmateurRadio.com and writes from Kansas, USA. Contact him at [email protected].
Activating SOTA’s at Philmont Scout Ranch
Philmont rates their treks by the magnitude of difficulty from Challenging, Rugged, Strenuous and Super Strenuous. The trek I was on was in the Super Strenuous category, for those familiar with the system, our Trek was # 31. I have been training for this trek for over a year and would need all that accumulated fitness to make the trip. We had a crew of eight, two adults and six teenage boys. What you learn, or maybe remember, is that youth covers lots of physical ills, in other words, they recover quickly.
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| Baldy Mountain getting closer |
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| Operating from Baldy Mountain AD5A In The Middle and AB5EB On The Right |
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| Baldy Mountain From Scheaffers Peak Yes, We Hiked That Distance |
After the activation of Scheaffer's Peak, we had to put our packs back on and finish the last nine miles of the trek. Another long day, but at the end, what a sense of accomplishment. Hiking 84 miles in rugged back country and activating two new SOTA summits.
Mike Crownover, AD5A, is a regular contributor to AmateurRadio.com and writes from Texas, USA. Contact him at [email protected].
Activating SOTA’s at Philmont Scout Ranch
Philmont rates their treks by the magnitude of difficulty from Challenging, Rugged, Strenuous and Super Strenuous. The trek I was on was in the Super Strenuous category, for those familiar with the system, our Trek was # 31. I have been training for this trek for over a year and would need all that accumulated fitness to make the trip. We had a crew of eight, two adults and six teenage boys. What you learn, or maybe remember, is that youth covers lots of physical ills, in other words, they recover quickly.
![]() |
| Baldy Mountain getting closer |
![]() |
| Operating from Baldy Mountain AD5A In The Middle and AB5EB On The Right |
![]() |
| Baldy Mountain From Scheaffers Peak Yes, We Hiked That Distance |
After the activation of Scheaffer's Peak, we had to put our packs back on and finish the last nine miles of the trek. Another long day, but at the end, what a sense of accomplishment. Hiking 84 miles in rugged back country and activating two new SOTA summits.
Mike Crownover, AD5A, is a regular contributor to AmateurRadio.com and writes from Texas, USA. Contact him at [email protected].
630m – The Path To VK
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| Roger, VK4YB |
I've been exchanging e-mails lately with Roger, VK4YB, in Queensland, Australia.
Roger is located about 30 miles from the ocean and has been the only VK signal that I have been able to hear on 630m WSPR mode. He seems to have the strongest signal out of Australia on 630m with his 90 watts and 120' tree supported wire vertical. John, VE7BDQ, has been heard twice down under with his modest station running at the allowable 5W EIRP limit, being reported in the fall of 2015 and again this spring. As well, John has heard Roger, the only signal from VK that either of us has copied.
I would like to be able to run some schedules with Roger in the fall, when transpacific paths should peak again. With that in mind, construction has begun on a new 630m transverter that will allow me to drive my present FET amplifier at full EIRP. Our schedules will utilize the JT9 weak signal mode, similar to JT65 but designed for the noisier LF and MF bands. It uses about 10% of the bandwidth that a JT65 signal requires, about 15Hz, and gains about 2db more sensitivity. A two-way QSO, under the best conditions, would take four minutes if all went well. A typical exchange of the required information, if initiated at my end, would look something like this:
VK4YB VE7SL
VE7SL VK4YB -20
R -18
RR 73
73 73 (not really needed but indicates RR received)
The path from my end is difficult as I am on the east side of Mayne Island and in Roger's direction, about one mile from a 600' hill directly in line with VK. Any RF heading Roger's way will need to leave here at a fairly high angle, which is likely the case anyway considering the low and short (in terms of wavelength) inverted-L antenna.
The path profile from here to the open Pacific Ocean is shown below, with my end being on the right edge, just behind those two hills. The rest of the obstructions are on Saltspring Island and then Vancouver Island, before hitting open water.
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| VE7SL To VK4YB courtesy: Hey What's That Path Profiler |
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| W7IUV To VK4YB courtesy: Hey What's That Path Profiler |
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| To VK4YB courtesy: Hey What's That Path Profiler |
The path from John, VE7BDQ, already heard in VK, is also easier than from here. Not far from the water, John has a pretty clear shot across Georgia Strait, giving his signal lots of time to gain altitude and clear those pesky Vancouver Island peaks.
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| VE7BDQ To VK4YB courtesy: Hey What's That Path Profiler |
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| VE7CNF To VK4YB courtesy: Hey What's That Path Profiler |
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| VA7MM To VK4YB courtesy: Hey What's That Path Profiler |
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| VE7CA To VK4YB courtesy: Hey What's That Path Profiler |
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| VK4YB Path To Pacific courtesy: Hey What's That Path Profiler |
As the solar activity slowly abates (but not this week!), propagation on 630m will slowly get better and better ... hopefully along with increased levels of Canadians transmitting on the band, and lots of stations in the USA. It is hoped that our enthusiastic neighbours to the south aren't too far away from getting the band fairly soon. Better get those soldering irons warmed-up so you are all ready to go!
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 Jul 18 16:10 UTC
Here is this week’s space weather and geophysical report, issued 2016 Jul 18 0416 UTC.
Highlights of Solar and Geomagnetic Activity 11 – 17 July 2016
Solar activity was at very low levels from 11-14 July with only a few simple sunspot regions. Region 2565 (N05, L=175, class/area Cko/350 on 17 Jul) rotated onto the east limb on 11 July as a simple Hsx spot class with a simple alpha magnetic class. By late on 14 July, another spot group began to emerge behind Region 2565 and was numbered 2567 (N05, L=165, class/area Dhi/330 on 17 Jul). Region 2567 quickly grew to over 300 millionths in area and was initially classified as a beta-gamma-delta magnetic group before some magnetic simplification occurred on 16 July. The region was downgraded to a beta-gamma magnetic class for the remainder of the period. Region 2567 became the most active region during 15-17 July producing 13 C-class flares. However, the close proximity of the two regions, as well as an active inversion line between the two, resulted in several flares to be attributed to Region 2565 on 17 July. The first was a long duration C1/Sf flare at 17/0803 UTC which was responsible for two CMEs observed in SOHO/LASCO C2 imagery beginning at 17/1124 UTC and 17/1248 UTC. The first was a faint asymmetric halo CME while the second was directed mostly off the east limb. Initial WSA-Enlil model output of the events showed a slow transit with effects possible on 21 July. The largest flare of the period, however, was a C6 at 17/2335 UTC which also occurred on the inversion line and was subsequently attributed to Region 2565.
No proton events were observed at geosynchronous orbit.
The greater than 2 MeV electron flux at geosynchronous orbit reached high levels throughout the period with a maximum flux of 5,512 pfu observed at 17/1630 UTC.
Geomagnetic field activity ranged from quiet to G1 (Minor) storm levels. The majority of the period was under the influence of high speed solar wind streams from a large, positive polarity, polar connected coronal hole as well as an isolated, positive polarity coronal hole. Solar wind speeds reached highs around 550 km/s early on 11 July, 650 km/s late on 12 July, and 700 km/s early on 15 July before finally decreasing to around 440 km/s by the end of the period. Total field during the period only managed to reach a maximum of 9 nT at 12/0552 UTC. Prolonged periods of southward Bz reaching -8 nT on 12 July and -6 nT on 14 July resulted in periods of G1 (Minor) storm levels on 12 July and active periods on 14 July. The rest of the period was at quiet to unsettled levels with quiet conditions observed on 17 July.
Forecast of Solar and Geomagnetic Activity 18 July – 13 August 2016
Solar activity is expected to be at low levels with a chance for M-class (R1-R2, Minor-Moderate) flares from 18-24 July as Regions 2565 and 2567 transit across the visible disk. Very low levels are expected for 25 Juy-04 August. A return to low levels with a chance for M-class flaring is expected for 05-13 August with the return of Regions 2565 and 2567.
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 on 18-19, 23-27 July, and again on 05-13 August due to recurrent CH HSS activity. Normal to moderate levels are expected for the remaining forecast period.
Geomagnetic field activity is expected to be at unsettled to active levels on 19-20, 22-24, 28, 30 July and on 03-08, 10-11 August with G1 (Minor) storm levels likely on 03-04 and 08 August due to recurrent CH HSS activity. A CME associated with the 17 July long-duration C1 flare is likely to arrive early on 21 July causing unsettled to active levels.
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/
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