Single Antenna System(SAS)
This is a Single Antenna 10kHz-30 MHz receiving system, generally
useful from 1kHz to 200 MHz. It is a larger version of the Field
Probe and the original PreampA/2m-dipole projects. PReampA and
SAS are low noise antenna system capable of approaching or achieving
the ITU "Quiet Rural" regional noise limit over the entire LF-HF
range when and where a suitable situation exists. Like the other
n6gn OSHW broadband receive system designs it is a highly
symmetrical/differential probe. Because it uses a symmetric dipole
rather than a monopole referenced to earth or to a radial system, as
are many commercially available broad band antenna systems, it can
provide much higher rejection of common mode feedline and ground
noise that can easily reduce system performance. Also because it is
a probe rather than a resonant/matched structure it is an extremely
broad band system that can provide effective coverage from audio
frequencies well into VHF.
A goal of this system is to approach performance dictated by regional
noise limitations as described by Rec. ITU-R P.372-16 rather than by
unwanted local noise sources present at a particular
location.
Caution: The broadband antenna system described here and on
associated pages MAY NOT WORK FOR YOU ! It
cannot operate well in every possible environment. Even with
modifications and adjustments being identified and described and
with very considerable extra effort there will be situations
too difficult to manage. An entirely different receive system
approach may be required.
This kit is not a simple solution by itself. Simply
obtaining or building all the kit necessary to install the hardware
is required but not sufficient. Proper deployment of a complete
system is at least, if not more, important than the equipment
itself. Not understanding and following this advice may result in
wasted time, energy and money !!! Background for this kind of
wide-band receiving systems is provided in a Broadband
Receive Systems overview. PLEASE read that background and also
Deploying a Single Antenna System
before beginning the building process.
In the SAS a high impedance, high CMRR preamplifier is mounted
inside a 3D printed plastic housing located near the middle of
an insulating fiberglass mast and fed with standard CAT5
cable as shown below. This antenna relies on the SWTL model of a
dipole and through the use of small .5mm diameter conductor (not
shown) can allow the nearby CAT5 feedline (also not shown) to
run parallel along the mast for most of the monopole
conductors length before finally exiting near the base. This can be
done without upsetting antenna balance and symmetry which would
otherwise unbalance the structure and possibly raise common mode
noise ingress and decrease the capability. Steps are taken to
avoid shadowing of the monopole's aperture located near its tip.
Scattering & Shadowing
A probe antenna is categorically different from a matched antenna
in that no power is extracted from an incident wave.
Although no power is extracted, the presence of such a probe element
does deform the nearby electric field of an incident
wave which is to be received. Put another way, the presence of
conductive material causes scattering.
For both matched and probe antenna types there is a region of
influence for such an element generally called an aperture.
The sketch on the left below shows rather the reverse of
the SAS use case. In it a scattering dipole is shadowing a
CAT5 90 'monopole' rather than the other way around. Though
the areas are to scale, the shape and field intensity
distribution depictions are not intended to provide precise
information but only a general impression of the situation when a
sensing antenna is shadowed by a nearby scatterer. In this
sketch, possible routes for the CAT5 'antenna' that might be
used to keep it sufficiently far away from the probe "shadow" are
shown. These are ways the interaction between the CAT5
and the probe may be minimized.
NEC2 (4NEC2) visualizations of the resulting vertical e-fields
produced by an incident electric field are shown below to the
right. These are with a uniform linearly polarized incident field
and above a MiniNEC ground. In each case the test frequency is that
where the CAT5is a quarter wave length, where it has highest Q and
produces the largest fields. The bottom of the CAT5 is directly
connected to the 'ground', which produces higher current and more
scattering than an actual use case where a continuation of the CAT5
cable continuing a considerable distance to the ShackBoard
location will have non-zero impedance.
An idea of the degree of scattering may be obtained by comparing
the e-field intensity near the tips of the dipole for the CAT5 90,
CAT5 45 cases and the"bell-bottom" case where the lower
portion of the lower mono-pole element is simply moved away from the
CAT5 at an angle. These strategies are suggested by SWTL theory
which indicates (see
A
New Antenna Model)
- no significant TEM coupling for these geometries between
the CAT5 and monopole element far from the tips
- the aperture associated with radiation is mostly around and
beyond the tip of the element
The fourth plot at the bottom right shows the mast moved 4.9m away
which also seems "far enough".
Though of use only over a limited frequency range it may be that
ferrite chokes or lossy beads placed on the CAT5 line can also
be used to further reduce the shadowing effect. This has
not yet been investigated.
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Empirical measurement
For the SAS use case, induced current in the CAT5 acting as a
feedline will produce re-radiation that counters the impinging
electric field near it and casts a shadow that can overlap the probe's
aperture. Rerouting the CAT5 or reducing current within it can reduce
this interaction. Empirical measurements have shown that a few
percent degradation in WSPR spots is produced when the CAT5 simply
exits vertically, parallel and close to the dipole (CAT5 90) but
not far enough away to escape the shadowing as compared to spots
produced when the CAT5 comes away at an angle (CAT5 45). This
slight rerouting seems to be enough to cause the interaction to be
negligible. For this reason, a revised mounting
technique different from the one shown below is being followed
whenever possible.
The SA Preamp interfaces to an SDR or other receiver by way of a
ShackBoard while delivering balanced RF output from one of the
100 ohm twisted pairs. Remaining pairs of the CAT5 are used to supply
power, and also to operate a low-capacitance mechanical relay
which can short the dipole terminals to verify CM rejection of the
entire system. One switch on the ShackBoard temporarily energizes the
B pair while a second switch allows removing bias to the high
impedance input buffers. These are used as diagnostics and
verification that the signals being sent to the receiver are indeed
differential originating at the dipole and not common mode
ingress in or after the preamp.
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The SAPreamp PCB is mounted inside a 3D printed enclosure with
antenna wires soldered to pads on the PCB. These wires exit through
the enclosure walls, run along the mast through the clips and
terminate at the top and near the bottom of the mast. The CAT5 cable
exits downward from the enclosure bottom and is clamped by the
enclosure cover which has a silicone rubber gasket. The result is a
water resistant housing for the electronics.
The preamp design uses a
ADA4930
in a transformerless output configuration to drive one pair of the
CAT5 cable.
The SAPreamp and Shack Boards are interconnected with standard CAT5
cable.
With Rp = 2Mohm, Cp=27pF, Rc=2kohm and G=2 for ADA4930 stages in the
preamp and in the shack board, the nominal gain from the dipole
connections to the SMA output using a calibrated 50 ohm VNA measures
approximately unity or 0 dB . When connected to the dipole, the
capacitive reactance of the dipole in conjunction with these values
creates frequency shaping in the overall response which can be used to
adapt a system for a particular location in the presence of very strong
signals that might otherwise overload it.
Characteristics -
- Highly symmetric differential inputs and outputs
- CMRR as great as - 50 dB to 30 MHz (but also a function of antenna
balance/symmetry).
- Connects to Shack Board for power, RF termination and CMRR
verification
- intended for use with 7m-10m fiberglass masts, ground mount and 3D
printed mounting HW shown in the Material List
- Input referenced noise is 2 - 3 nV/rt(Hz), input buffer limited
- shaped gain to optimize noise floor/temperature while limiting
maximum signal level to protect SDR ADCs from overload
- noise figure of about 14 dB
- noise floor near -160dBm/Hz.
- Use with 30m (nominal) length standard CAT5 cable
- SAPreamp is used with associated Shack Board, 12VDC @ ~100mA
The use of ADA4930 differential amplifiers in the SAS instead of
(previously) transformers at both ends of the CAT5 cable allows coverage
from AF well into VHF while reducing cost and achieving very much
greater CMRR, low noise and excellent IMD performance.
The ADA4930 is not a conventional Operational
Amplifier. It has attributes which make it very useful in broadband, low
noise, low distortion applications such as the SAS. It
simultaneously operates in common-mode and differential modes with
separate inputs for each. From Data Sheet ADA4930-1/ADA4930-2 Rev. B |
Page 17 of 25
THEORY OF OPERATION
The ADA4930-1/ADA4930-2 differ from conventional op amps in that they
have two outputs whose voltages move in opposite directions and an
additional input, VOCM. Like an op amp, they rely on high open-loop
gain and negative feedback to force these outputs to the desired
voltages. The ADA4930-1/ADA4930-2 behave much like standard voltage
feedback op amps and facilitate single-ended-to-differential
conversions, common-mode level shifting, and amplifications of
differential signals. Like op amps, the ADA4930-1/ADA4930-2
have high input impedance and low output impedance.
Two feedback loops control the
differential and common-mode output voltages. The differential
feedback, set with external resistors, controls the differential
output voltage. The common-mode feedback controls the common-mode
output voltage. This architecture makes it easy to set the output
common-mode level to any arbitrary value within the specified limits.
The output common-mode voltage is forced to be equal to the voltage
applied to the VOCM input by the internal common-mode feedback loop.
The internal common-mode feedback loop produces outputs that are
highly balanced over a wide frequency range without requiring tightly
matched external components. This results in differential outputs that
are very close to the ideal of being identical in amplitude and
are exactly 180° apart in phase.
Of importance in this application is that the specified noise in
differential mode is very much lower than that when used with the common
mode input. It is for this reason that the SAS has two
operating configurations; Utility and Performance. In Utility mode two
antiphase outputs from the ShackBoard are available but have higher
noise floor. In Performance mode these two outputs are used with an
anti-phase 3dB combiner in order to reject common-mode noise and produce
the lowest noise floor.
The high impedance buffered input of the SAPreamp is similar to
previous preamps, with the addition of catch diodes and value changes to
better meet the characteristics of a 6m probe dipole when used as a
broadband probe with common SDR receivers.
The PCB is enclosed in a 3D printed housing and cover. Dipole wire
connections are made through small holes in the enclosure's wall where
they are soldered to pads on the PCB. Those holes and a channel in the
cover are filled with silicone rubber or a gasket to help keep the
inside dry. The CAT5 cable is clamped by the cover and exits from
the bottom of the enclosure The entire assembly is fastened to a
vertical mast approximately 24mm in diameter using TyWrap fasteners.
In operation, one switch on the Shack Board allows verification
that unwanted common mode ingress after the preamp is
sufficiently smaller than differential signals from the dipole so does
not significantly degrade recovered SNR of received signals. A second
switch activates a mechanical relay to short the input at the
SAPreamp itself. In a similar manner, this allows the entire
system to be verified at time of installation and also provides a way to
measure the total receive system noise floor/temperature. It should be
understood that there may still remain mechanisms which provide coupling
to unwanted near-field noise sources when the dipole lies along the
gradient of an offending field.
In the 0-60MHz spectrogram below, taken during the daytime from a
suburban location in Fort Collins, CO, note the relative absence of
local QRN signatures and a reasonably flat noise floor demonstrating the
lack of susceptibility to common mode noise. Also notice the wide signal
dynamic range being tolerated.. Thus, in this case to a large degree,
"The antenna truly is the antenna".
Below are plots of estimated Rec. ITU-R P.372-16 "City" through "Quiet
Rural" output noisewhen using a 6m dipole. The maroon colored plot is from
a model of internally generated noise due to the preamplifier. The
propagated noise, which is the desired target exceeds local system
noise everywhere over the .01 to 30 MHz range.
Caution! :
This estimate is subject to change as the system model is adjusted and
shaping optimized. The QUCS model
still needs to be verified. Above 5 MHz where the dipole is greater than
one tenth-wavelength, propagated noise voltage at Ra may be
somewhat higher . This is not reflected in the model.
The short-dipole antenna model which is used for part of this modeling,
is itself only an approximation.
The fiberglass mast can be ground-mounted with a screw mount for
freestanding operation. For permanent use, the pole should be guyed. It
can also easily be collapsed and moved to a different location.
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Material List
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What you will need to build this kit
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Item Description
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Provider
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Source Code
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Notes
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Approximate Cost
(excluding setup fees and shipping) |
Assembled
SingleAntenna Preamp
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==> JLCPCB
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==>
KiCad
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Beginning alpha-test
to determine optimum antennas length and component values
for world-wide use. Investigating Overload
mitigation problem. Contact me before ordering. D3&D4
are experimental.
TLE2426 rail splitter will probably need to be pre-ordered
at JLCPCB else Global Order C59459 $2 from Mouser
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~US$30 |
Assembled
SingleAntenna ShackBoard
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==>
KiCad
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Dual Output Transformer-less
design intended to be compatible with previous PreampA &
PreampB (though without LPF/HPF for Hybrid operation).
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~US$20 |
3D Printed
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Preamp Enclosure,
Cover. Gasket & mast clips
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==> JLC3DP
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==>
FreeCAD
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Simply "OK" to accept the risk
when JLC3DP cautions about too-thin wall thickness. |
~US$10 |
N3AGE Mast Clips
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These are Elmer's, n3age, split design using TyWraps. I
like these the best. Fab at JLC3DP not yet tested but seem
good when home-printed:
Layer Height 0.3 mm
Wall count 4
Infill Density 30%
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38x88x100mm Clam Shell
Enclosure
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Other sources possible.
Enclosure needs to accept 84mm wide PCB. |
US$12 |
38x88m Enclosure Front
Panel
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US$2 |
38x88mm Enclosure Back
Panel
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Telescoping Fiberglass
Mast
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~US$55/US$65
~$46
$70 (+ shipping !)
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Mast Screw-in Ground
Mount
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Not required if mast is to be clamped to a wooden post
rather than used freestanding.
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~US$30 |
Miscellaneous
CAT5 cable, 6-32 HW, Tywraps, Camo Paint, 12VDC PS ...
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Local HW store |
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Assembly, Test, Deployment & Optimization
As received from JLCPCB, almost all PCBs have worked without
problem so need no special attention unless there are missing
components or values to be changed. Preamp enclosure will need to
have Silicone rubber or a preformed gasket added.
Once the Shack Board is also complete, this leaves deployment the
large remaining item. As previously mentioned, this kit is not a
turn-key solution or a "silver bullet". To achieve the best
performance and make full use of the capability of this antenna
system's capability, the candidate area should first be surveyed
to find the lowest noise location. A Field Probe may be a useful
tool for doing this. At some sites dipole size and component
values may need to be adjusted to avoid overdrive of the input
buffer amplifiers. At the output of the ShackBoard which follows
some SDRs may need to have attenuation added to avoid overload.
To begin this process, please read Deploying
a Single Antenna System.