The Propagation Jigsaw

Many people derive enjoyment and relaxation from building complex jigsaws. And ‘purists’ will undertake this often-lengthy task without reference to the picture on the box. Initially, there are just a few edges and a corner or two. Later on, small clusters of pieces come together offering a partial glimpse of the full vista. Eventually more substantial areas emerge, and these assist in an accelerating journey to completion.

Developing a sound understanding of radio propagation can follow much the same path. Though, by contrast, timescales can be measured in years, pinpointing the complexity of the topic.

As many know already, propagation behaviour is a strong function of frequency. What happens at VLF is unlike HF, while VHF and UHF are different again. And indeed there are other important factors including the ionosphere and troposphere, time of day and year, the Sunspot cycle, shorter-timescale ionospheric events and so forth. Physical location: on a summit, on an open plain, by salt water etc, with their many aspects and ground conductivities, all matter to varying degrees. Signal polarisation and take-off angles are typically major players. You may well know of more.

And even the experts talk only of probabilities and expectations. There are far fewer certainties in radio propagation than found, say, in the fields of engineering and mathematics. Yet it can be this very uncertainty that draws people into ham radio and associated professional fields.

Today, I offer a couple more pieces for your propagation jigsaw. Chris @DL1CR continues to do good work on 630m. For many, this is a specialist yet intriguing band. Earlier discussions on here covered the propagation of the DCF77 time signal on 77.5kHz from its transmitting site at Mainflingen, in southern Germany.

Encouraged by the above, I recently purchased a budget DCF77 clock. My QTH in eastern Scotland is some 1087km from Mainflingen; the full path is shown in the image below. As you can see, having crossed southern Germany, the signal has an easy journey over the (flat) Netherlands to the North Sea. At this point, it has completed some 40% of its trip. Nearly all the remaining path is over the highly-conductive, low loss, salt water of the North Sea.

The Mainflingen station uses VERTICALLY polarised antennas to deliver a GROUND-WAVE signal on 77.5kHz. The ‘bottom part’ of the wave-front, closest to the ground, is actually conducted by the ground / water over which the signal is passing. There is a resultant ‘drag’ on the lower part of the wave. This causes some forward inclination, encouraging the wave to follow the curved surface of the Earth. See Ref 1 below.

At distant (1000km+) locations from DCF77 there is a big difference between the day-time signal strength (ground-wave only) and the night-time signal strength (ground-wave + sky-wave). Using my TS-590SG + 40m dipole, here DCF77 is S4-S5 during the day, and about S7 at night.

I unpacked my new DCF77 clock early one afternoon. I fitted the two AAA batteries and placed it on an upstairs bedroom window-sill, looking out on a bearing of some 125 degrees towards Mainflingen.

It is more than an under-statement to say I was extremely surprised to see it lock onto the DCF77 signal in about 2 minutes :open_mouth: This is with the low S4-S5 daytime signal level. It has now been locked, day and night, for several weeks. What is more, the setup allowed me to adjust the display by -1 hour, to show UKT rather than the default CET.

This experience has certainly fitted a few more pieces into my propagation jigsaw :slight_smile:

73 Dave

Ref 1 - Propagation and Radio Science by Eric Nichols, KL7AJ. Published by ARRL, 1st edition 2015.

The circles in the image below are at 500, 1000, 1500, and 2000km from DCF77.

8 Likes

I suspect the clock antenna will be a coil on a ferrite core so presumably uses the magnetic part of the transmission/signal?

You are lucky to have about half of the ground wave path across salty seawater. Reading just now about VLF propagation I found it interesting that the D-layer of the ionosphere, so annoying during the day on the lower HF bands for attenuating signals, reflects VLF signals back down, creating the skywave propagation mode that is important for long-distance VLF communication.

I once read an entire RSGB-recommended book on radio propagation thinking at the time how complicated it is. And sadly now I remember only some of it.

3 Likes

I am on same distance from DCF77 as Dave. Just a coincidence, in the past couple of month I am playing with some ferrite antenna builds. Particularly focused on VLF/LF and 630m band. What I did found was small ferrites can indeed make wonders on lower bands if made properly. I am receiving DCF77 with SNR around 25db at night and 15db daytime. The antenna is a 14x stacked ferrit rods, which works great on 630m too.

See the test screenshots I’ve made comparing three different antennas on DCF77. This is a night time signal to noise test. Ignore decibels’ values for a signal strength, look at them as a SNR measure. Note a simple single rod loopstick, which performs almost equaly to its bigger counterparts.

3 Likes

I actually have a wristwatch that synchronises with DFC77. It seems to find a signal pretty much everywhere I’ve been in the last 12 years.

The DCF77 TX generates some 50kW output. A large T-antenna is used, together with a ground-plane/screen comprising many km of copper wire. Base-feeding the T-antenna delivers a vertically-polarised signal. BBC Radio 4 LW (198kHz) does much the same.

As highlighted earlier, for clocks distant (>1000km) from Mainflingen, the DCF77 signal is notably stronger during darkness hours owing to the additional sky-wave. While the ground-wave is vertically-polarised, after refraction by the ionosphere, the sky-wave signal polarisation is liable to be mixed (note 1), and changing with time. As such, constructive / destructive interaction between the ground and sky waves can lead to a measure of QSB.

Recognising all this, to maximise the probability of success, the DCF77 protocol undertakes synchronisation FIVE TIMES PER NIGHT, at midnight, 1, 2, 3 and 4am.

The paper linked below provides more information than you’re every likely to need :slight_smile:

73 Dave

Note 1 - After ionospheric refraction, the signal can be split, and the various components can have wide-ranging polarisations. For newer hams, note that signal polarisation can take many forms, and the electric field can have any angle; it is NOT restricted just to VERTICAL and HORIZONTAL.

1 Like

I can copy DCF77 on my TS-570 with all kinds of simple antennas including just a few feet of wire. MSF from Rugby did improve massively in strength when it moved from Rugby to Anthorn which is probably half the distance it used to be.

I agree … my aged MSF-locked frequency standard now works notably better.

That said, one man’s meat …

Many people on the UK Channel coast struggled with MSF after the move North. Today, they find DCF77 provides a better signal. I suppose the salt water of the Channel has rather less loss than the Pennine hills + Cumbrian fells :slight_smile:

2 Likes

I’d have thought that maybe MSF and DCF77 would be under threat as “old school” time and sync signals as we have ubiquitous GNSS services. But that nice Mr. Putin and his jamming/disruptions have probably given these services a boost to their usefulness :wink:

In case anyone interested … I’ve now set up one of my VLF plotters to display DCF77 amplitude as well. That is running 24/7, just refresh the screen when you wish. You’ll see all the changes in signal strength at my QTH (day/night), the dips at sunrise/sunset etc. It is not as responsive to solar flares, but I have other graphs for that.

VLF/LF plotter No. 5

1 Like