Cheap ‘flight deck’

My LNR Precision MTR5b always comes away with me and for good reason. It’s small, portable and xyl friendly. It does however, suffer from a lot of wires and bits loosely hanging around. Mrs g7kse regularly takes the opportunity to ‘tidy’ stuff up. This means I can no longer find it. This is ok at home because it hasn’t gone far but a pain when I’m not at home.

Ikea has long been a source of cheap stuff and their chopping boards are just the thing to make into a small flight deck. The one I got is approximately 24cm by 15cm and came as a pack of two with a much larger one that is in use in the kitchen.

I thought the first thing to do would be make up a small tray that I can sit the MTR5b into and then still that to the board. Duly designed and 3d printed. Next up was a small notebook like the boys in blue use, after that some magnets for my palm key (it has a magnetic base). Lastly some velcro tape and 4 m4 nuts, bolts and washers. he optional part is a DC buck converter (just be careful to check dimensions as they change shape and size a bit) that I use to regulate the voltage to 12v (I got carried away and made a really bad case for it)

I thought I’d sink the magnets into the board at then epoxy them in. Mainly because its polypropylene and nothing sticks too well to these waxy plastics. All this took was a bit of careful dremelling and you’re done. The notebook is clipped to the board and the velcro strips stuck down onto the back. The ast ting to do was put 6 feet on it so I didn’t scratch any surface I carelessly chucked the thing on. Here’s a few photos and a link to the parts on Thingiverse.

 

 

 

Here Comes The ’29 QSO Party!

courtesy: Lou, VE3AWA




This Saturday night as well as the next will be the annual Bruce Kelley 1929 QSO Party, otherwise known as the '1929 BK'.





Only transmitters that are 'era-appropriate' are allowed to be used. More specifically, transmitters must employ tubes that were available in 1929 or earlier, and transmitters must be self-excited. No crystals allowed! Crystals were new and largely unaffordable for most hams back in the depression days.

The year of 1929 marked a real turning point in amateur radio as governments finally cracked-down on things such as frequency stability, out of band operations and re-alignment of call districts. In short, hams were henceforth required to behave themselves and to clean up their signals and methods of operation.

courtesy: http://www.arrl.org/
Although the new rules did a lot to improve things when it came to 'signal purity', there was still a long way to go ... but the wheels of improvement had been officially set in motion. The next decade would see monumental changes in both transmitter and receiver architecture, as engineers along with some particularly gifted amateurs, strove to unlock the challenges of this relatively new technology.

If you tune across the CW bands during the next two Saturday nights, you will have the rare opportunity to hear exactly what the bands must have sounded like back in the early '30s'.

For the most part you will hear single-tube Hartley, Colpitts or TNT oscillators along with a few two-tube MOPAs thrown in. Many of them will suffer the same problems encountered by the boys of '29 ... chirp, drift, buzzy notes and frequency instability from antennas swaying in the wind.

Again this year, signals should be a little louder as well, since the previous long-time power limitation of 10W input has been increased to 25W.

The MOPAs will sound much better but some surprisingly nice-sounding signals can be heard coming from properly tuned and optimised single-tube oscillators. I recall being blown away by the lovely sounding signal I heard from such a rig when first tuning into the BK activity several years ago, only to learn that it was a self-excited Hartley using 1/4" copper tubing for the oscillator tank circuit!

The '29 watering-hole on 80m will be around 3550-3580 kilocycles (be careful not to confuse this with kilohertz!) while the early afternoon to post-sunset 40m activity will be found from 7100-7125 kc. There may even be a few on the very low end of 160m. Although many of these transmitter styles were used on 20m and higher, BK rule-makers have wisely decided not to inflict these sounds on the present populace as it would likely keep the 'Official Observers' busy for several days writing pink-slips.

This year I will leave the MOPA on the shelf and set up my Hull Hartley as I haven't used it since building the MOPA a few years ago. If it's very windy (almost assured), the Hartley will really sound like 1929!


My own Hull Hartley

You can learn more about amateur radio happenings leading up to and following the 1929 crackdown in my earlier series of 'Why '29' blogs here:

Part 1
Part 2
Part 3
Part 4

Those wishing to put something together for next year's event can find everything needed here:

Introduction To Building ... '29-Style

Building '29-Style - Part 1

Building '29-Style - Part 2

Heck, there me even be time to throw something together for the following Saturday if you have a few parts and an older tube or two ... the '27 comes to mind and is readily found in many junk boxes. Maybe you know an old-timer or two with lots of parts that could help you out.

Let's hope for good conditions for this event as the last few years have been adversely affected by geomagnetic storming. Poor propagation or not, I guarantee there will be plenty of '29ers busy calling 'CQ AWA' on the low bands.

Complete BK details are available here.

CLE237 Results

Last weekend's CLE237 was truly a workout. Not only was the format challenging, hunting for different grid square fields, but propagation was superb ... a vast departure from the normal CLE propagation-curse!
This combination resulted in many daytime hours spent reviewing three nights of Perseus recordings, the downside of being able to sleep all night rather than staying up until 0300 while listening live!




All told, 118 NDBs in 41 different grid fields were logged. Of these 118 stations, 12 were 'new catches'. After DXing NDBs since 1985, new catches are getting harder and harder to find but last week's great conditions were the best heard here in several years.

Today's quiet Sun!

With a very quiet Sun for a couple of weeks now, these great MF conditions are what many have been waiting for since the last solar low many years ago ... propagation below the broadcast band can be truly remarkable when these quiet conditions continue for many weeks at a time.

Here are a few interesting CLE catches as recorded on the Perseus SDR.

GREENLAND


MARSHALL ISLANDS
                                            

NDBs QY (Sydney, Nova Scotia), YBB (Pelly Bay, Nunavut)and 3Z (Russell, Manitoba) all sharing 263kHz within a few Hz of each other.



My full CLE237 log is shown below. As usual, a Perseus SDR and an 'inverted-L' (resonated to 300kHz) was used for the activity.


AH
28 13:30  403     TUT   Pago Pago, SMA

AL
28 13:30  400     MDY   Midway, MDW

AO
27 12:30  283     DUT   Dutch Harbor, ALS
27 12:30  341     ELF   Cold Bay, ALS
27 12:30  385     EHM   Cape Newenham, ALS
27 12:30  390     HBT   Borland, ALS

AP
27 06:00  263     OAY   Norton Bay, ALS
27 13:30  275     CZF   Cape Romanzof, ALS
27 13:00  325     BVK   Buckland, ALS
27 13:30  347     TNC   Tin City, ALS
27 13:00  356     HHM   Kotzebue, ALS

BG
27 13:30  352     RG    Rarotonga, CKS

BK
27 13:30  332     POA   Pahoa, HWA

BL
27 14:00  353     LLD   Lanai, HWA

BO
27 12:00  277     ACE   Kachemak, ALS
27 12:00  355     AUB   King Salmon, ALS
27 12:00  394     RWO   Kodiak, ALS
27 12:00  411     ILI   Iliamna, ALS
27 12:00  429     BTS   Dillingham, ALS

BP
27 12:00  212     CGL   Juneau, ALS
27 13:00  257     CUN   Fairbanks, ALS
27 12:00  346     OLT   Soldotna, ALS
27 12:30  347     DJN   Delta Junction, ALS
27 12:00  350     VTR   McGrath, ALS

BQ
27 13:00  376     PVQ   Deadhorse, ALS

CN
27 06:00  378     AP    Mayne Island, BC, CAN (MY NEAREST)
27 12:00  266     SLE   Salem, OR, USA
27 07:00  356     PND   Portland, OR, USA
27 06:00  356     MEF   Medford, OR, USA
27 06:00  404     MOG   Montegue, CA, USA

CM
27 07:00  203     TCY   Tracy, CA, USA
29 04:00  385     MR    Pacific Grove, CA, USA

CO
27 12:00  266     ICK   Annette Island, ALS
27 12:00  358     SIT   Sitka, ALS
27 12:00  396     CMJ   Ketchikan, ALS
27 12:00  414     IME   Sitka, ALS
27 12:00  529     SQM   Sumner Strait, ALS

CP
27 13:30  222     WY    Wrigley, NT, CAN
27 11:30  254     EV    Inuvik, NT, CAN
27 14:00  284     YOC   Old Crow, YT, CAN
27 08:00  380     YUB   Tuktoyaktuk, NT, CAN
27 12:00  392     ZFN   Tulita, NT, CAN

CQ
29 06:00  321     YSY   Sachs Harbour, NT, CAN

DM
27 08:30  242     EL    El Paso, TX, USA
27 10:00  278     CEP   Ruidoso, NM, USA
27 06:00  326     MA    Midland, TX, USA
27 12:00  338     RYN   Tucson, AZ, USA
27 13:00  341     OIN   Oberlin, KS, USA

DN
27 09:00  233     BR    Brandon, MB, CAN
27 09:00  275     HIN   Chadron, NE, USA
27 09:00  383     CNP   Chappell, NE, USA
27 09:00  400     FN    Fort Collins, CO, USA
27 09:00  414     GRN   Gordon, NE, USA

DP
27 08:00  207     PY    Fort Chipewyan, AB, CAN
27 08:00  212     BY    Beechy, SK, CAN
27 08:00  219     ZRS   Regina, SK, CAN
27 08:00  221     QU    Grande Prairie, AB, CAN
27 08:00  230     VG    Vermilion, AB, CAN

DQ
27 08:30  361     HI    Holman, NT, CAN

EL
27 06:00  260     MTH   Marathon, FL, USA
27 10:00  269     AR    New Iberia, LA, USA
27 10:00  329     HMA   Hondo, TX, USA
27 06:00  332     FIS   Key West, FL, USA


EM
27 07:00  263     CVM   Alton, IL, USA
27 07:00  332     IC    Wichita, KS, USA
27 07:00  335     BV    Batesville, AR, USA
27 07:00  338     UMP   Indianapolis, IN, USA
27 07:00  349     GW    Greenwood, MS, USA

EN
27 12:00  257     JYR   York, NE, USA
27 06:00  329     PMV   Plattsmouth, NE, USA
27 06:00  360     SW    Warroad, MN, USA
27 08:00  368     VIQ   Neillsville, WI, USA
27 09:00  368     PNM   Princeton, MN, USA

EO
27 07:00  212     YGX   Gillam, MB, CAN
27 08:00  216     YFA   Fort Albany, ON, CAN
27 08:00  218     RL    Red Lake, ON, CAN
27 08:00  224     MO    Moosonee, ON, CAN
27 08:00  258     ZSJ   Sandy Lake, ON, CAN

EP
27 06:00  224     BK    Baker Lake, NU, CAN
27 09:00  241     YGT   Igloolik, NU, CAN
27 08:00  263     YBB   Kugaaruk, NU, CAN
27 10:00  329     YEK   Arviat, NU, CAN
27 10:00  335     YUT   Repulse Bay, NU, CAN

EQ
27 04:00  365     YGZ   Grise Fiord, NU, CAN

FI
27 05:00  365     PAL   Palma, EQA

FK
28 05:00  369     ZDX   Saint Johns, ATG
27 06:00  391     DDP   Vega Baja, PTR
27 05:00  415     CBC   Cayman Brac, CYM


FL
27 09:00  376     ZIN   Matthew Town, BAH

FM
29 05:00  198     DIW   Dixon, NC, USA

FN
27 08:00  289     YLQ   La Tuque, QC, CAN
27 08:00  373     YXK   Rimouski, QC, CAN
27 05:00  392     ML    Charlevoix, QC, CAN
27 05:00  407     ZHU   Montreal, QC, CAN
27 07:00  516     YWA   Petawawa, ON, CAN

FO
27 10:00  208     YSK   Sanikiluaq, NU, CAN
27 18:37  323     KR    Schefferville, QC, CAN
27 10:00  351     YKQ   Waskaganish, QC, CAN
27 10:00  390     VP    Kuujjuaq, QC, CAN
27 08:00  396     YPH   Inukjuak, QC, CAN

FP
27 09:00  277     YLC   Kimmirut, NU, CAN
27 10:00  338     YPX   Puvirnituq, QC, CAN
28 10:00  358     YKG   Kangiqsujuaq, QC, CAN

FQ
29 07:00  256     YCY   Clyde River, NU, CAN

GN
27 10:00  263     QY    Sydney, NS, CAN
27 08:00  280     QX    Gander, NL, CAN
27 08:00  350     DF    Deer Lake, NL, CAN

GO
28 08:00  220     BX    Lourdes de Blanc, QC, CAN
28 08:30  281     CA    Cartwright, NL, CAN
28 10:00  396     JC    Rigolet, NL, CAN

GQ
28 06:00  399     UP    Upernavik, GRL

QJ
27 12:00  366     PNI   Pohnpei Island, FSM

QL
27 13:00  343     ML    Minami Tori Shima, MTS
27 12:00  360     OX    Iwo Jima, VOI

QO
28 13:30  437     OG    Okha, RSE

RG
27 12:30  260     NF    Norfolk Island, NFK

RJ
27 12:00  316     MAJ   Majuro Atoll, MHL
27 12:00  393     UKS   Kosrae, FSM


As always, complete CLE results (worldwide) can be viewed in detail here.

All-in-all, an exhausting but delightful weekend of listening and great propagation ... so many signals to hear ... welcome to solar-low!

Monday’s ‘NRN’ CW Fun

My homebrew Ameco AC-1 clone



A weekly CW operating activity that seems to be growing in popularity is the Monday “NRN”.





The NRN get-togethers are an offshoot of the annual “NRR” or Novice Rig Roundup. Monday’s “Novice Rig Night” gradually grew from those that wanted to see the NRR fun continue, in one form or another, without waiting an entire year for the event to roll around again.

Operating times run from sunup on the east coast to midnight on the west coast ... but basically, people just get on the air whenever they can on Monday and call “CQ NRN”. I suspect that most of the activity takes place between late afternoon and bedtime, with 40m probably seeing the most action. As winter arrives, we may see more activity on 80m but these are only my personal observations from the west coast.

Most folks are using typical Novice-era transmitters and / or receivers, with the Drake 2NT, early Heathkits, Eicos, homebrews and Hammarlunds being popular. The previous Monday I was active with my homebrew Ameco AC-1 clone, a 6V6 crystal power oscillator, at about 6 watts out. Good contacts were had with several eastern stations. There are several AC-1s around and there has been at least one suggestion of an 'AC-1 Night' ... what fun that would be as well!

For last night’s NRN, I brought out my homebrew Paraset.


Once again, good contacts were had with the easterners on 40m: W9BRD in NJ, W3NP in WV,  KD2E in NJ and VE3LYX using his No.19 tank radio ... two WWII radios talking to each other in 2018, one real and one a reproduction!



VE3LYX's No.19 set operating position
The Paraset uses a two-tube regenerative receiver and, like the AC-1, a single 6V6 crystal controlled power oscillator. It's always difficult to judge propagation conditions when listening with a regen ... are conditions as bad as they seem or is it just my simple receiver making the band sound poorer than usual? Such was the case for me last night so next week I will spark-up the Paraset once again for another round of NRN fun. As promised on the NRR Facebook page (now at 1600+ members!), all Paraset contacts will be confirmed with my mid-30s styled QSL and these will be going out this week. 




Here is the formal announcement for the Monday events, with a few additional details. Hopefully you can join the fun (any rig is fair game!), next week.

Hunting For NDBs in CLE 236

AP-378 Mayne Island, BC



How time flies. Once again it's a CLE weekend. It seems like the last one was just a week ago!




 'CLE's are 'Co-ordinated Listening Events, and NDB DXers around the world focus their listening time on one small slice of the NDB spectrum.

This time the hunting ground is the 15 kHz slice from 370.0 - 384.9 kHz.

This is a somewhat dreaded range for me since my local blowtorch NDB, 'AP' (378 kHz), sits right in the middle of the range. 'AP' is located at the entrance to Active Pass, the main ferry route to Vancouver Island, and the antenna is about 3/4 of a mile down the beach from me. Needless to say, the beacon is about 40db over S9! With careful loop nulling, I can reduce this by about 25db but it's still an enormous signal to deal with.

Hopefully you can put 'AP' in your own log this weekend but its 25-watt signal will be much weaker for you. It's been logged as far east as Illinois and with your receiver in the CW mode, can be found on 378.399 kHz.

All too often our CLE weekends get hammered by geomagnetic disturbances, possibly because our monthly schedule syncs up nicely with the Sun's rotation and the disturbance from the previous month once again rotates into position. Conditions this time surely can't be much worse than for our previous event and today's mid-week check looks promising.


courtesy: NOAA
courtesy: NOAA

Things seem geomagnetically quiet at the moment so lets hope they stay that way. LF and MF propagation can often be amazing in the fall and as summer storms start to dissipate, the band can become much less noisy.

From CLE coordinator Brian Keyte (G3SIA), comes the following CLE info:


Hi all,

Please join us in our 236th coordinated Listening Event which starts
this Friday and celebrates the arrival of the Equinox this weekend.
CLEs are not contests - if you enjoy taking part you will be a winner!

    Days:    Friday 21 September - Monday 24 September
    Times:   Start and end at midday, LOCAL TIME at the receiver
    Range:   370 - 384.9 kHz

Just log all the NDBs that you can identify with their nominal (listed)
frequencies in the range (it includes 370 kHz, but not 385 kHz)
plus any UNIDs that you come across there.

Please send your CLE log to the List in a plain text email if possible
(not in an attachment) with CLE236 and FINAL at the start of its title.
Show on each log line:
    # The date (e.g. 2018-09-21, etc., or just 21) and UTC
          (the date changes at 00:00 UTC)
    # kHz  (the nominal published frequency, if known)
    # The Call Ident.

Show those main items FIRST - other optional details such as Location
and Distance go LATER in the same line. 
If you send interim logs, please also send a 'FINAL' (complete) log.

As always, tell us your own location and brief details of the equipment
that you were using during the weekend.

Joachim or I will send the usual 'Any More Logs?' email at about 17:00
UTC on Tuesday - you can then check that your log has been found OK.
All logs must arrive on the list at the very latest by 08:00 UTC on
Wednesday 26th September.  We hope to complete making the combined
results within a day or two.

To help you to plan your listening, seeklists and maps for your part of the
World are available via the CLE page  http://www.ndblist.info/cle.htm

Good listening - enjoy the CLE.
    Brian
------------------------------------------------------------------
From:     Brian Keyte G3SIA         ndbcle'at'gmail.com
Location:  Surrey, SE England       (CLE coordinator)
------------------------------------------------------------------

If you are interested in some remote listening - maybe due to local difficulties - you could use any one remote receiver for your loggings, stating its location and with the owner’s permission if required. A remote listener may NOT also use another receiver, local or remote, to make further loggings for the same CLE.
 -------------------------------------------------------------------

These listening events serve several purposes. They:
  • determine, worldwide, which beacons are actually in service and on-the-air so the online database can be kept up-to-date
  • determine, worldwide, which beacons are out-of-service or have gone silent since the last CLE covering this range
  • will indicate the state of propagation conditions at the various participant locations
  • will give you an indication of how well your LF/MF receiving system is working
  • give participants a fun yet challenging activity to keep their listening skills honed
Final details can be found at the NDB List website, and worldwide results, for every participant, will be posted there a few days after the event.


The Yahoo ndblist Group has been moved to Groups.io and The NDB List Group will now be found there! The very active group is a great place to learn more about the 'Art of NDB DXing' or to meet other listeners in your region. There is a lot of good information available there and new members are always very welcome. As well, you can follow the results of other CLE participants from night to night as propagation is always an active topic of discussion.

You need not be an NDB List member to participate in the CLEs and all reports, no matter how small, are of much value to the organizers. 

Remember - 'First-time' logs are always VERY welcome!

Reports may be sent to the NDB List Group or e-mailed to CLE co-ordinator, Brian Keyte (G3SIA), whose address appears above. If you are a member of the group, all final results will also be e-mailed and posted there.

Please ... give the CLE a try ... then let us know what NDB's can be heard from your location! Your report can then be added to the worldwide database to help keep it up-to-date.

Have fun and good hunting!

The Fall “Classic Exchange”

W7OS - Radio Club of Tacoma working the CX
This fall's running of the CW "Classic Exchange" will take place on Sunday, September 23 and on Tuesday, September 25. The following week will see the Phone "Classic Exchange", on Sunday, September 30 and on Tuesday, October 2.


The "CX" encourages participants to use older vintage gear including any homebrew equipment, both receivers and transmitters. A unique scoring system provides bonus points for various equipment and combinations as well as encouraging 'repeat contacts' when you switch to different equipment.


W8KM and his wonderful vintage station

No vintage gear? ... no problem! All amateurs are invited to participate and get in on the fun no matter what they are using and submit their scores.


K3MD's Heathkit AT-1 and Hallicrafters HT-37 ready for the CX

The CX is a low-key relaxing affair and the 'extra' Tuesday operating period should encourage a lot of midweek activity from the vast numbers of retired operators who cherish and run older gear.


Lots of combos ready at W4BOH's CX setup



K6ZI, Las Vegas - WWII ARC-5s ready to go


For complete details, see the web site announcement here.

If you've never entered the Classic Exchange, why not give it a try this year as it truly is a case of 'the more the merrier' ... and eastern operators, make sure to keep the porch light on for us out west!

The 630m Portable Adventures of EIØCF


In the years before amateurs in the UK had access to the 630m band as we know it today (472-479kHz), hams there could apply for a 'special research permit' allowing them to operate between 501 and 504kHz.


One of the first and most active stations was operated by Finbar O'Connor, EIØCF, located in the most northern part of Ireland, near Malin Head. In the early days, Finbar might as well have been AC4YN in Lhasa, Tibet, as a 630m or a 2200m QSO with EIØCF was a much prized DX trophy and a genuine 'right of passage' for many little backyard LF and MF stations throughout Europe.

Nowadays, 630m activity in Europe is not as robust as it once was but Finbar is still active on MF from his modest station. He reports being copied in North America on several occasions. Although mainly active in the WSPR mode, Finbar is now considering the two-way JT9 weak signal QSO mode and may hopefully once again, tease east coast North American MF operators with a new rare entity from his seaside location.


Finbar's WSPRlite setup for 630m
Over the years, EIØCF has gone portable as well as marine mobile to demonstrate the viability of this part of the spectrum for very reliable groundwave comms using equipment that is both simple and quick to deploy. Although he used a CW-based system, his conclusions could just as easily apply to SSB or digital modes.

EI0CF/marine on 630m!

What follows is a delightful adventure, in Finbar's own words, describing some of his field trips back in the 500kHz experimental days ... perhaps it will inspire some North American portable work or provide ideas for an emergency prep 630m grab-and-go kit, or just get you excited about our newest amateur allocation.


                                    ******************
              Operating Portable on 501 - 504 khz Medium Wave



Operations on the north flank of Slieve Snacht Inishowen Peninsula.

In June 2009 Ireland joined a growing number of countries permitted to operate on a small portion of the medium wave band, just below the commercial broadcast segment, in the range 501 - 504 khz. Several stations were granted permission and operations commenced. As has been documented elsewhere many stations have been worked, both in band and cross band, at home and abroad, ranging from Continental Europe, across the Atlantic to the USA and Canada, down to the southern end of Ukraine and finally up to Iceland, Norway, Sweden, Finland and also being heard in Moscow.

A notable feature of this band is the steady reliable nature of groundwave coverage and with this in mind I recently availed of the facility whereby portable operations can take place. Comreg, together with the IRTS and the individual involved, require that each event is applied for, giving relevant dates, location, contact details, hours of operation and the power of the transmitter being used.

In the period leading up to all this it was necessary to build and test a viable portable station based on the use of my Berlingo van. A 30' part of a 40' Spiderbeam fibreglass  pole was used with a simple round wooden peg to secure the 'Tee' wire antenna, which was fabricated from twin twisted multistrand speaker wire. The vertical used both, while the rest was pulled apart to form the two horizontal legs.

A 100 metre roll of 1.5 mm insulated earthing wire was cut into 16 lengths to provide radial wires, with lugs soldered to one end and a bonding bolt used to secure a single point for the radial kit. The far ends formed a small loop which was sealed and secured with insulating tape. The loop provided an eye for a small L shaped stiff wire, fashioned from discarded coat hangers, an ideal and cheap way to hold the ends of the radial wires in place in the ground.

To secure the antenna support to the van, I refer you to the excellent idea described by John EI7BA, on his web page, for a ball hitch connection:

http://www.qsl.net/ei7ba/a_ball_hitch_mobile_mount.htm

Using this superb idea, I got the welder out and made one for myself. It worked perfectly.

I now had the support and wire antenna, with a ballpark figure for what might resonate, along with the radial kit. I next needed a dedicated antenna tuning unit. An old variometer and two extra fixed multitap coils were selected. A home made 1 amp ammeter and SWR twin meter unit completed the fit-out. These were all assembled on a base with a handle on the top, making it easy to move around whilst out and about.

The main antenna for 500kHz was disconnected and left floating and the van set up with all this gear, but no transmitter. Instead, my little antenna bridge running off a 9-volt battery provided the necessary signal to start testing for basic resonance.

Whether from sheer good luck or some sub-conscious input, resonance fell within the range of the variometer with only one of the two extra coils in circuit. The relative height and length also play a part in the range of resonance secured. Matching to 50 ohms was then optimized by selecting 4700 pf Mica capacitors using Croc Clip links. The available value ranged from 1 nF to 14 nF.

I have a selection of 500khz transmitters, two of which are to the design of Roger, GW3UEP, who lives 10 miles inland from the coast, in south Wales. His 500khz web site is well worth checking out, containing plans for versions of his 500khz transmitters, test equipment pictures and recordings of 500khz activities.

http://www.gw3uep.ukfsn.org/

One of these was used to put some RF into this first portable style installation, and by arrangement, Roger listened and heard my signal. We delightedly completed a short contact, with my transmitter running just 10 watts.Things were looking good.

One of the very valuable things about portable operations stems from the need to bring together several elements to secure a working radio station, without the usual backup we enjoy from home. Planning is essential. Doing a dry run, i.e. actually physically building the intended station then notating all the gear required and making a list as well as providing backup items, particularly those that which if broken or lost, would render the whole radio station non-viable. This also extends to the operator of the equipment. Will they be warm or cool enough, have shade, food, water and enough needed rest? Always be prepared to abandon the project if safety is compromised, for whatever reason.



Now that I had a viable portable station for 500kHz working, it was time to head off and test both the equipment and myself in the real world, but without any live transmissions taking place.

Several sites were chosen and tested, with particular emphasis placed on remoteness, i.e. high up on mountains or near the sea. All sites worked very well, but those by the sea proved really excellent. Reception of NDB’s (Non Directional Beacons) provided a ready supply of medium to low frequency signals for range testing. I was now itching to “ have a go “ out in the wilds, on 500kHz! Using the method required by Comreg, an application was made for several sites, on specific days.




In early June I loaded up the van with all the gear and headed off for the mountain above Redcastle, County Donegal. Using a narrow track and climbing higher, to about 270 meters, a place was found leading to an old quarry. Typically, it had started to rain. By the time I had erected the support pole, pulled out and secured the top hat wires using light nylon line and deployed the radial wires around and below the vertical drop wire, my trouser ends were very wet!

Plugging in the 12-volt supply, the receiver was very quickly perked up, using the variometer. The Morse key connected to the QTX transmitter and the transmit / receiver switch flicked over. Time to get some RF flowing in the antenna. Sure enough, on key down, the antenna current meter shot right up to 400 mA, but the SWR match was not exactly perfect. Time to work those Croc Clips and start selecting shunt capacitors to find the perfect match. Soon I had that sorted to my satisfaction, with antenna current now up to 550 mA. A quick return to receive showed that Roger, GW3UEP was already tuned up on frequency.




"..... GW3UEP DE EIØCF/P HW K"

He came back straight away! Oh joy, we were on the air on 500, in a remote mountain area, the top of my antenna almost tipping the clouds as they swept past. I was open to the elements, standing at the back door of the van with the tips of my fingers reaching for the knob of my very favourite old Amplidan morse key, snug beside the other bits and pieces of equipment on the van floor!

My logbook, with its pages flapping back and forward in the wind, soon had the first 500kHz portable contact documented. A full hour later, solid steady signals continued at a distance of 250 miles. Proving just how good groundwave signals can be, I terminated communications from the remote portable location, happy with the results. Within 12 minutes I had dismantled the station and was on my way to Moville, along with a strong cup of coffee at the café on the town's main street.

Several other portable operations have since taken place. A number have also occurred at my home location. We live right beside the sea; high tides lap up on to the salt marsh, which is part of the property.




Driving a single earth rod into the sea shore to a depth of 1 metre, with no radials and just a single wire between the rod and the ATU earth, the 1 amp RF meter had its meter needle slamming against the end stop. Lots of antenna current for 15 watts transmitter output power. Those same 15 watts only providing, at best, 550 mA, whilst up on the mountain sites.

Finally, it was thought productive to try a kite-supported antenna from the seashore portable set up. Winds on the day selected seemed strong enough to enable my Delta shape kite to head aloft with a flying line and antenna wire attached. The Berlingo van was driven down on shore, everything connected and tuned up. All was well, or was it?

The receiver now seemed quite dead with no band noise and no antenna current on transmit. Looking skywards I could see nothing. My eye followed the antenna wire heading for deeper water. Then I saw it. The kite had plunged into the sea! The following 30 minutes entailed untangling loads of seaweed with the line wrapped around rocks, barnacles and everything imaginable. What a mess! I almost gave up, but knew that Roger would be coming up on frequency, on sked, in about 15 minutes.

Eventually I managed to get the kite skywards again but by now the wind was acting more unpredictably. I established contact with Roger and he immediately gave me an S 7 report for my 15 watts. This equated to the report I would get from my main station antenna running 100 watts. My single ground rod and 150 feet of wire were doing the business.

We carried on our contact, but what remained became a battle of wits, with a kite constantly diving down and soaring up again. Several times the antenna wire was in part lying on the sea shore and antenna current way down to 200 mA or lower. My left hand was on the variometer tuning knob, tweaking the setting as best as possible, while pulling in the slack to keep the antenna wire off the ground. Feeding the wire out again to a misbehaving kite, I kept keying away with my right hand, keeping Roger updated so he could understand why my signal was changing both in pitch (sudden antenna mis-match conditions) and signal strength.

Luckily he was also making a recording, which proved later to be a fascinating record of a difficult portable antenna and station operation. It’s remarkable how tolerant, despite the wildly changing antenna conditions, the system actually was in practice. Communications were maintained despite all these negative factors and severely decreased radiated power at times.


Several other tests were conducted within these experiments which would have been almost impossible to conduct without the challenges thrown up by my portable operations. To my mind the 501 – 504khz band exhibits a distinct advantage for enhanced groundwave coverage over that available to higher frequencies.

Relatively simple equipment deployed in remote locations, with or without the availability of the power grid, would provide a solid backbone link or network in times of emergency. Transmitter power output was kept deliberately low to ensure that a higher ERP would not mask any possible weakness in the system. I am happy to conclude that Medium Frequency CW proved it’s worth once again.

Already I have further plans to test smaller, more compact portable antenna and earthing systems in more remote locations.

Finbar O’Connor EIØCF Malin, County Donegal.


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  • Matt W1MST, Managing Editor