NOTE: All information on the LFA (Loop Fed Array) Yagi is now release. DUBUS magazine have kindly given permission for us to allow you to see it. This is available for download in PDF format on my download page.
Revolutionary Yagi Antenna Feed System by G0KSC
The LFA design has a patent pending and all G0KSC designs are copyright. Any ham can build for their own use or those of a friend. Where profit or commerical gain exists, express permission of G0KSC must be sort.
Justin Johnson G0KSC, has pioneered a revloutionary new feed system for the Yagi directional beam antenna which will see it's Debut in the next isuue of DUBUS - the serious magazine for VHF and up amateur radio www.dubus.org. Whilst there are many benefits seen with the new system, the most important break through is the suppression of the age old problem of unwanted side lobes within longer Yagi designs.
The feed system (which does not consist of a dipole and no, it is not a Quagi!) has 2 different feed points. Whilst the antenna needs re-modeling in order to change from one to the other, different characteristics are seen from each method. The first enhances the bandwidth capabilities of the Yagi and presentes never-seen-before ultra low return loss, excellent gain and front to back ratio, whilst the other provides more traditional OWA (Optimised Wide-band array) style bandwidth with good improvements in forward gain and massive improvements in front to back ratio.
What people say
'This could be a turning point in the development of the Yagi Antenna' Popa, YU7EF - World renowned Yagi antenna designer/engineer - www.yu7ef.com
'Justin, Indeed this looks like a unique and winning design!' Joel R. Hallas, W1ZR - Technical Editor, QST Magazine
'Hi Justin, Many thanks for the plots, these diagrams look really beautiful! I have never seen such F/B and low sidelobes for a Yagi before' - Joe CT1HZE - DUBUS Magazine
Benefits of the new design
Whilst going to press, experiments are still being conducted with the new Yagi. However, the new fed adds a number of very interesting characteristics to the Yagi which when focus is applied to optimisation, excellent not-seen-before Yagi performance is the result. The list so far consists of the following:
- Superior Front to Back Ratio with very high supression of unwanted lobes
- Extended/alteration of ‘ideal’ boom length
- Exceptional clean pattern performance
- Ultra-wideband characteristics
- 50 Ohm impedance – no matching required
- Easy fine-tuning of feed arrangement itself
Superior Front to Back Ratio
Quad beams are renowned for their superior front to back properties (over Yagi’s) when comparing like to like (number of elements) within small arrays. The New Yagi has picked up this characteristic. In models created so far, front to back figures of between 30-40dB in Yagis of 7 and 8 elements WITHOUT distorting the forward pattern or indeed creating any unwanted side lobes.
Extended/alteration of the ‘ideal’ Boom Length
As any Yagi experimenter will know, there is a boom length for any given frequency/number of elements which provides the ideal balance between forward gain and front to back ratio. If you drop below this point, high front to back and lower forward gain can be achieved (to a point then both drop) and go above this point and forward gain increases whilst front to back drops away.
An interesting characteristic within the new design is the ability to extend this ideal length and as a result, squeeze out additional gain and front to back at the same time. This is in part due to the size of the feed system and the space it takes up on the boom as reflector and first director spacing remains similar to that of traditional Yagi’s although the large feed arrangement is between them. Using 50Mhz as an example, the feed system width (along the boom) is around 45Cms and therefore, on a 5 element Yagi, almost .5 metres length has been added to the boom. I have achieved 11.3dBi forward gain and over 20dB front to back from a 5el 50Mhz beam with a boom length of just under 5 metres.
However, by altering the size of the driven element on the new design (increasing size along the boom) the 'ideal' boom length can be altered and hence new levels of gain and performance achieved. Whilst F/B was compromised slightly, over 12.5dBi forward gain has been achieved from a 5el 70Mhz Yagi with an extremley long boom.
Exceptional Clean Pattern Performance
The new feed system provides an out-of-phase operation along it's Y axis which runs parallel to the boom. It is this side radiation cancellation characteristic which helps the design reduce side and rear unwanted lobes to an absolute minimum. Full details and build information for 2 G0KSC Yagi's will be presented in the next issue of DUBUS Magazine. Both an ultra wide-band 5el 50Mhz Yagi and 11el 144Mhz low temperature Yagi (TanT noise figure below with an antenn using 5mm think elements) will be featured.
When focus is applied to optimising forward pattern along with front to back (in preference to out and out forward gain) very clean patterns with ultra-low noise can be achieved.
This explanation is intentionally non-technical in order that all can understand the basic concepts of the antenna.
Ultra Wideband Characteristics
Another powerful aspect of the new feed system is flexibility of the fed arrangement and how it can alter the performance of the Yagi. Extremely flat curves within minimum reactance and return loss can be achieved.
50 Ohm impedance, no matching unit required
As with all of my designs which keep the amateur antenna builder, novice or professional in mind, no matching unit, coaxial stubs or any other tuning arrangement needs to be added to the antenna. A simple 1:1 balun or coaxial choke balun at the feed point is enough. As stated above, direct feed of the antenna is possible and due to the design of the feed system itself, fine tuning can be achieved easily. Full details in DUBUS! www.dubus.org
Some plots of Yagis created so far:
A preview of the 11el 144Mhz Yagi to be featured in DUBUS below:
Visit www.DUBUS.org for details of the next issue release date.
73
Justin G0KSC