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From: "Markus Vester" <markusvester@aol.com>
To: <rsgb_lf_group@blacksheep.org>
References: <53507F98.3060009@virginbroadband.com.au>
Date: Sun, 20 Apr 2014 17:12:21 +0200
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Subject: LF: Re: EWE antenna
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Hi Edgar, LF,

both Hartmut and Jean-Pierre are using K9AY receive antennas with a =
cardioid pattern pointing northwest, and their captures of transatlantic =
LF stations from America have been superior to anyone else in mainland =
Europe by a long shot (probably 10 dB in SNR). I think this is mostly =
due to the fact that they can suppress QRN from the southeast and =
Mediterranean sea, which is the dominant lightning area and QRN source =
during our winters.=20

Several times I have attempted to improve my reception by adding a =
signal from the garden loop pair to that of the E-field antenna. Using =
an indoor goniometer (made of two orthogonal coils around the outside of =
a ferrite ring), I was able to make a virtually rotatable loop, which =
could produce a good null to south-easterly QRN and QRM (eg. HGA22). =
During noisy nights, the improvement from the QRN reduction was quite =
significant. However unfortunately this didn't not hold under quiet =
conditions. Compared to the vertical, the noise floor from my loops is =
about 10 dB higher due to coupling to adjacent underground ADSL and =
power lines. This means that adding in the magnetic contribution often =
makes things worse rather than better.

As Richard VK7RO has pointed out, the advantage of directivity may not =
be quite the same for your location in Tasmania: If thunderstorms are =
over the Tasman sea / New Zealand, a cardioid antenna pointing towards =
Europe should have a large benefit. If QRN is coming from the side =
(Australian East coast), a classic magnetic loop may be better. And if =
the noise direction is coinciding with the signal (Northwest), there's =
little you can improve using antenna directivity.

If I understand you right, you're saying that in Orford the resonated =
magnetic loop is not as good as the vertical probe, and the resistively =
loaded cardioid is even worse? I'd like to understand why that is so. =
Could it be that three is also noise predominantly magnetic from the =
vicinity (eg. power supplies, telephone or power lines)? You might want =
to try a comparison measurement of daytime noise floor, with the other =
end of the EWE shorted (ie closed loop, acting solely as magnetic =
antenna) versus open (top wire acting as electric antenna).=20

In my understanding, the flag, EWE and K9AY antennas are all working on =
the same basic principle, ie superposition of an omnidirectional pattern =
from a vertical electric antenna, and a figure-eight pattern from a loop =
with a positive and a negative lobe. This is indeed exactly identical to =
the operation of a properly terminated directional coupler, using =
simultneous capacitive and inductive coupling to a TEM line. In that =
sense, the top wire of an EWE is not simply a feeder to the remote =
vertical leg, but both an electrical topload and integral part of the =
magnetic loop.

On the other hand, you can think about a closed magnetic loop as two =
separate pairs of conductors, one vertical pair spaced horizontally, and =
one horizontal pair spaced vertically. Witrhin each pair there are =
opposed currents, acting as a gradiometer for electric fields. The =
vertical legs produce vertically polarized groundwave radiation, with =
the desired sine (figure-eight) pattern in the horizontal plane. The =
horizontal wires radiate predominantly upwards, which usually does not =
contribute to DX reception in a useful manner. So yes, you could do away =
with the horizontal conductor, leaving only two verticals with antiphase =
currents - very much the same way that an Adcock pair was used to =
minimize "night-effect" direction-finding errors from steep skywave. The =
only disadvantage would be that the antiphase monopoles have a large =
capacitive impedance, which limits the achievable radiation efficiency =
to an order of magnitude below that of a same-size closed loop. But =
given sufficient size and spacing between the vertical elements, and the =
possibility to use a low-noise preamp, this will matter little in a =
receive application.=20

So we have seen that a loop can be replaced by two electric monopoles =
driven in antiphase. Obwiously we can also (and even at the same time) =
drive them in phase, letting them act essentially as a (relatively =
efficient) single omnidirectional vertical. To then produce a cardioid, =
the omni- and gradiometer- farfield components will have to be made =
equally strong. This implies that the antiphase vertical currents (eg. 1 =
A, -1 A) would have to be larger and in quadrature to the inphase =
currents (+0.1j A, +0.1j A). In other words, the two vertical currents =
have to be almost but not exactly in antiphase. This picture naturally =
connects to the "quasioptical" view of a short two-element Yagi, where =
the back lobe cancellation is caused by 180deg+phi phase from the driven =
currents, augmented by - phi from the propagation delay difference.

Best 73,
Markus (DF6NM)
 =20


From: edgar=20
Sent: Friday, April 18, 2014 3:27 AM
To: Markus Vester=20
Cc: Stefan Sch=E4fer=20
Subject: EWE antenna


Hi Markus,

On reading the article on EWE antennas I do not think the loop at Orford =
is suitable for 2200 m reception in the EWE configuration!


For 80 m the wire separations is 0.05 * 80 =3D 4 m.
For 160 m the wire separation is 0.05 * 160 =3D 8m
For 2200 m the wire separation is 0.05 * 2200 m =3D 110 m!=20

This loop is 16m.

>From tests conducted at Orford the reception at frequencies above about =
500 kHz are good.
However less than that  frequency there are poor.

I think I will have to take a different approach.

Regards, Edgar

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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META content=3Dtext/html;charset=3Diso-8859-1 =
http-equiv=3DContent-Type>
<META name=3DGENERATOR content=3D"MSHTML 8.00.6001.23580"></HEAD>
<BODY style=3D"PADDING-LEFT: 10px; PADDING-RIGHT: 10px; PADDING-TOP: =
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id=3DMailContainerBody leftMargin=3D0 topMargin=3D0 bgColor=3D#ffffff =
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CanvasTabStop=3D"true" name=3D"Compose message area">
<DIV><FONT size=3D2 face=3DArial>Hi Edgar, LF,</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>both Hartmut and Jean-Pierre =
are&nbsp;using K9AY=20
receive antennas with a cardioid pattern pointing northwest, and=20
their&nbsp;captures of transatlantic&nbsp;LF stations from =
America&nbsp;have=20
been&nbsp;superior to anyone else in mainland Europe by a long shot =
(probably 10=20
dB in SNR). I think this is mostly due to the fact that they can =
suppress QRN=20
from the southeast and Mediterranean sea, which&nbsp;is&nbsp;the =
dominant=20
lightning area and QRN source during our winters. </FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>Several times I have attempted =
to&nbsp;improve my=20
reception by adding a signal from&nbsp;the garden loop pair to that of =
the=20
E-field antenna.&nbsp;Using an indoor&nbsp;goniometer (made of two =
orthogonal=20
coils around the outside of a ferrite ring), I was able to make a =
virtually=20
rotatable loop,&nbsp;which could produce a good null to south-easterly=20
QRN&nbsp;and QRM (eg. HGA22).&nbsp;During noisy nights,&nbsp;the=20
improvement&nbsp;from the&nbsp;QRN reduction was quite significant. =
However=20
unfortunately this didn't not hold under quiet conditions. Compared to =
the=20
vertical, the noise floor from my loops is about 10 dB higher due=20
to&nbsp;coupling to adjacent underground ADSL and power lines. This =
means that=20
adding in the magnetic contribution&nbsp;often makes things worse rather =
than=20
better.</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>As Richard VK7RO has pointed out, the =
advantage of=20
directivity may not be quite the same for your location in Tasmania:=20
If&nbsp;thunderstorms are over the Tasman sea / New Zealand, =
a&nbsp;cardioid=20
antenna pointing towards Europe should have&nbsp;a large benefit. If QRN =
is=20
coming from the side (Australian East coast), a classic magnetic loop =
may be=20
better. And if the noise direction is coinciding with the=20
signal&nbsp;(Northwest), there's little&nbsp;you =
can&nbsp;improve&nbsp;using=20
antenna directivity.</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>If I understand you right,&nbsp;you're=20
saying&nbsp;that in Orford the resonated magnetic loop is not as good as =
the=20
vertical probe, and the resistively loaded cardioid is even worse? I'd =
like to=20
understand why that is so. Could it be that&nbsp;three is&nbsp;also =
noise=20
predominantly magnetic from the vicinity (eg. power =
supplies,&nbsp;telephone or=20
power&nbsp;lines)? You might want to try&nbsp;a comparison measurement =
of=20
daytime noise floor, with the other end of the EWE shorted (ie closed =
loop,=20
acting solely as magnetic antenna)&nbsp;versus open (top wire acting as =
electric=20
antenna). </FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>In my understanding, the flag, EWE and =
K9AY=20
antennas are all working on the same basic principle, ie superposition =
of an=20
omnidirectional pattern from a vertical electric antenna, and a=20
figure-eight&nbsp;pattern from a loop with a positive and a negative =
lobe. This=20
is indeed exactly identical to the operation of a&nbsp;properly =
terminated=20
directional coupler, using simultneous capacitive and inductive coupling =
to a=20
TEM line. In that sense, the top wire of an EWE is&nbsp;not simply a =
feeder to=20
the remote vertical leg, but both an electrical topload and integral =
part of the=20
magnetic loop.</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>On the other hand, you can think about =
a closed=20
magnetic loop as two separate pairs of conductors, one vertical pair =
spaced=20
horizontally, and one horizontal pair spaced vertically.&nbsp;Witrhin =
each pair=20
there&nbsp;are opposed currents,&nbsp;acting as a&nbsp;gradiometer for =
electric=20
fields.&nbsp;The vertical legs&nbsp;produce vertically polarized =
groundwave=20
radiation, with the desired&nbsp;sine (figure-eight) pattern in the =
horizontal=20
plane.&nbsp;The horizontal wires radiate predominantly upwards,=20
which&nbsp;usually does not contribute to DX reception in a useful =
manner.=20
So&nbsp;yes, you could do away with the horizontal conductor, leaving =
only two=20
verticals with antiphase currents - very much the&nbsp;same way =
that&nbsp;an=20
Adcock pair was used to minimize "night-effect" direction-finding errors =
from=20
steep skywave. The only disadvantage would be that the =
antiphase&nbsp;monopoles=20
have a large capacitive impedance, which&nbsp;limits the achievable =
radiation=20
efficiency&nbsp;to an order of magnitude&nbsp;below that of a same-size =
closed=20
loop. But given sufficient size and spacing between the vertical =
elements, and=20
the possibility to use&nbsp;a low-noise preamp, this will matter little =
in a=20
receive application. </FONT><FONT size=3D2 face=3DArial></FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>So we have seen that a loop can be =
replaced=20
by&nbsp;two electric monopoles driven in antiphase. Obwiously =
we&nbsp;can also=20
(and even at the same time) drive them in phase, letting them&nbsp;act=20
essentially as a (relatively efficient) single&nbsp;omnidirectional =
vertical. To=20
then produce a cardioid, the omni- and gradiometer- farfield components =
will=20
have to&nbsp;be&nbsp;made equally strong. This&nbsp;implies that the =
antiphase=20
vertical currents (eg. 1 A, -1 A)&nbsp;would have to be&nbsp;larger =
and&nbsp;in=20
quadrature&nbsp;to the inphase currents (+0.1j A, +0.1j A).&nbsp;In =
other words,=20
the two vertical currents have to be almost but not exactly in =
antiphase.=20
This&nbsp;picture naturally connects to the "quasioptical"&nbsp;view of=20
a&nbsp;short two-element Yagi, where the back lobe cancellation =
is&nbsp;caused=20
by&nbsp;180deg+phi phase from the&nbsp;driven currents, =
augmented&nbsp;by - phi=20
from the propagation delay difference.</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>Best 73,</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial>Markus (DF6NM)</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial>&nbsp;&nbsp;</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT>&nbsp;</DIV>
<DIV style=3D"FONT: 10pt Tahoma">
<DIV><FONT face=3DArial></FONT><FONT face=3DArial></FONT><FONT=20
face=3DArial></FONT><FONT face=3DArial></FONT><FONT =
face=3DArial></FONT><FONT=20
face=3DArial></FONT><FONT face=3DArial></FONT><FONT =
face=3DArial></FONT><FONT=20
face=3DArial></FONT><FONT face=3DArial></FONT><BR></DIV>
<DIV style=3D"BACKGROUND: #f5f5f5">
<DIV style=3D"font-color: black"><B>From:</B> <A=20
title=3D"mailto:edgarjtwining@virginbroadband.com.au&#10;STRG + Klicken, =
um Verkn=FCpfung zu folgen"=20
href=3D"mailto:edgarjtwining@virginbroadband.com.au">edgar</A> </DIV>
<DIV><B>Sent:</B> Friday, April 18, 2014 3:27 AM</DIV>
<DIV><B>To:</B> <A=20
title=3D"mailto:markusvester@aol.com&#10;STRG + Klicken, um =
Verkn=FCpfung zu folgen"=20
href=3D"mailto:markusvester@aol.com">Markus Vester</A> </DIV>
<DIV><B>Cc:</B> <A=20
title=3D"mailto:Stefan.Schaefer@iup.uni-heidelberg.de&#10;STRG + =
Klicken, um Verkn=FCpfung zu folgen"=20
href=3D"mailto:Stefan.Schaefer@iup.uni-heidelberg.de">Stefan =
Sch=E4fer</A> </DIV>
<DIV><B>Subject:</B> EWE antenna</DIV></DIV></DIV>
<DIV><FONT size=3D2 face=3DArial></FONT><FONT size=3D2 =
face=3DArial></FONT><FONT size=3D2=20
face=3DArial></FONT><FONT size=3D2 face=3DArial></FONT><FONT size=3D2=20
face=3DArial></FONT><FONT size=3D2 face=3DArial></FONT><BR></DIV>Hi =
Markus,<BR><BR>On=20
reading the article on EWE antennas I do not think the loop at Orford is =

suitable for 2200 m reception in the EWE configuration!<BR><BR><IMG =
alt=3D""=20
src=3D"cid:68D0584DAF3A46908DB38617DF7FA17A@White" width=3D374=20
height=3D143><BR><BR>For 80 m the wire separations is 0.05 * 80 =3D 4 =
m.<BR>For 160=20
m the wire separation is 0.05 * 160 =3D 8m<BR>For 2200 m the wire =
separation is=20
0.05 * 2200 m =3D 110 m! <BR><BR>This loop is 16m.<BR><BR>From tests =
conducted at=20
Orford the reception at frequencies above about 500 kHz are =
good.<BR>However=20
less than that&nbsp; frequency there are poor.<BR><BR>I think I will =
have to=20
take a different approach.<BR><BR>Regards, Edgar<BR></BODY></HTML>

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