January 1953 QST
Table of Contents
Wax nostalgic about and learn from the history of early electronics. See articles
QST, published December 1915 - present. All copyrights hereby acknowledged.
Author Edward Tilton discusses here the tradeoff between
bandwidth and sensitivity in receivers, given that broadband noise power follows bandwidth in a 10 log
BW fashion. Pulling in the most distant stations requires very low noise in able to get the SNR as high
as possible, which requires the minimum bandwidth possible. Prior to highly stable local oscillators,
operating successfully in a narrow bandwidth for voice (phone), and particularly for CW (Morse code),
dictated the use of a fixed frequency crystal to keep from having to constantly re-tune the station.
Nowadays, of course, what used to be considered a metrology grade oscillator can be bought for tens
Some ABCs of V.H.F. Receiver Design
Hints for Improving Weak-Signal Performance at 50 Mc. and Higher
By Edward P. Tilton,* W1HDQ
The receiver engineers can pass this one up. It is written for the fellow who, knowing little of
the factors that make for good reception, tends to judge a receiver by its price tag or its appearance.
He is more likely to choose a receiver that harmonizes with his wife's interior decorating scheme, or
one that sounds best in the broadcast band, rather than the receiver that will deliver optimum performance
in the ham bands. And as for building something in the receiving line for himself - well, he shudders
at the thought - if, in fact, he has ever gotten around to thinking about it.
Fig. 1 - Some typical receiver selectivity curves. The narrow curve, A, is about
the best that can be obtained with a 455-kc. i.f. without crystal filter. It will be superior to the
high-fidelity curve, B, in weak-signal v.h.f. reception. Curve C is representative of the response of
receivers having higher intermediate frequencies.
Now there are many good reasons why we tend, more and more, to let the receiver manufacturers do
the dirty work in designing and construction for us. Unless we have extensive shop facilities, good
test equipment, and considerable experience in receiver work it is difficult to build a complete receiver
for 3.5, 7 or 14 Mc. that will equal one made by an outfit having these assets. But even if we intend
to work only on the lower bands, we should not fall into the habit of letting the engineers do all our
thinking for us, too! And if we are going to concentrate on the frequencies from 28 Mc. up, we have
little choice but to build our own gear, if we expect to do a first-class receiving job.
What Makes a "Sensitive" Receiver? We all want to be able to pull in the weak ones. To be able to
hear signals that other fellows miss is a universal amateur aim, regardless of the frequency we work
on. Before we invest a month's pay in a new communications receiver, or start in building a v.h.f. converter,
therefore, we should know something of the factors that make for superior weak-signal reception.
Up to around 20 Mc. or so there is no very marked difference in the weak-signal capabilities of the
better receivers. Below this region nearly all tubes work well, and the limiting factor in receiving
weak signals is noise generated outside the receiver. Additional r.f. amplifier stages, no matter how
well designed, will serve mainly to increase such noise in direct proportion to the signals we want
to hear. Thus, adding r.f. gain is similar to tacking on another stage of audio - it will make the signals
louder, but no more readable. In some of the simpler receivers having no r.f. amplifier stage, or an
ineffective one, an external r.f. preamplifier may be needed to bring up the level of the weakest signals,
but in a majority of cases the only way to hear more DX on 3.5, 7 or 14 Mc. will be to put up a better
antenna, or move to a quieter location.
As we approach the v.h.f. region the picture changes, and our noise level comes from a different
source. Tube performance falls off as we go higher in frequency, and amplifier stages have to be run
"wide open" to produce enough gain to make weak signals audible. There is still some external noise,
to be sure, but much of the "shush" that is characteristic of a hot v.h.f. receiver is tube noise, generated
within the receiver. At 3.5 Mc., a good receiver with its a.v.c. off and its gain controls set for optimum
weak-signal reception makes little or no noise when its antenna is disconnected, or the terminals shorted.
A good v.h.f. receiver makes plenty! What, then, are these "low-noise front ends" we talk about in QST
and the Handbook?
The point to remember here is that the noise generated within the receiver, not that coming in on
the antenna, is the limiting factor in v.h.f. receiver sensitivity. This condition begins to show at
28 Mc. It is much more marked at 50 Mc., and it is all-important at 144 Mc. and higher. Thus, the more
gain an r.f. amplifier stage provides for a given amount of noise generated, the better will be its
To make the best use of this information, we have to know what makes "tube noise" and what tubes
develop the least for a given amount of gain. Most of this noise results from electronic action within
the tubes, so other things being equal, the more elements within the tube, the more noise it will make
as a v.h.f. amplifier. Thus, a pentode (with a plate, screen, suppressor and control grid, all contributing
to the total cathode current) will make more noise than a triode, when the upper limit of its useful
frequency range is approached. And these elements add to the input and output capacitance of the tube,
resulting in more capacitive loading of the tuned circuits to which it is connected.
The principal advantage of the pentode is that, by isolating the grid and plate circuits it makes
possible high gain (over its normal frequency range) without external neutralizing circuits. When the
limit of its operating range is approached it gives way to the triode, with some circuit tricks added
to achieve stability. Well designed pentode stages work just about as well as triodes at 21 and 8 Mc.,
but at 50 Mc. and higher the triodes take over almost exclusively. And even at 21 and 28 Mc., the pentodes
don't do so well unless the circuits are designed specifically for these frequencies.
Here, then, is the main reason why the best "all-band" receivers fall down on 28 and 50 Mc., compared
to even the simplest converters of the home-built variety. The first stages of any receiver that covers
the broadcast band and the lower ham bands are designed to give optimum performance there - in the range
where they will be used most. Stability over a wide tuning range, good response to automatic volume
control action (needed to work that popular accessory, the S-meter), and freedom from cross-modulation
troubles dictate the use of tubes that do not perform well at 28 Mc. and higher. It's a hard fact of
receiver design, and no reflection on the ability of the engineers who develop our commercial receivers,
that you can spend close to a thousand dollars for a receiver and still not get as good performance
on 28 or 50 Mc. as is available with a converter you can build yourself for twenty dollars or less.
Maybe there will be a really good commercial receiver for the v.h.f. bands someday, but it has not
appeared on the horizon thus far, except in limited-production converter form.
The Role of Selectivity
Too many v.h.f. men think of selectivity only as an aid to separating stations on crowded lower frequencies,
not realizing that it is also directly related to the effective signal-to-noise ratio that can be achieved
when the receiver is used with a converter for the v.h.f. bands. All other things being equal, the greater
a receiver's bandwidth the more noise it will make for a given amount of over-all gain.
Let's look at Fig. 1 for a moment. Here are "selectivity curves" showing relative receiver response
as we tune through a signal. When we understand that the signal-to-noise ratio of a v.h.f. receiver
is inversely proportional to the area of its selectivity curve, we see at once why we want to use no
more bandwidth than is necessary to pass an intelligible signal.
Curves A and B were taken from the instruction manual of the new Hallicrafters SX-73. They show the
passband of this superb receiver in two of its six selectivity positions. Curve A is for the sharp i.f.
position, without crystal filter.
Curve B shows the broadest response, used mainly for high-fidelity broadcast reception. From B we
see that to drop the signal level 6 db., we have to tune out 7 kc. either side of the center frequency.
To drop it 60 db. we must detune 17 kc. On curve A, we see that the 6-db. points arc only about 3 kc.
removed from the center frequency, and the 60-db. points are only about 8 kc. from the center.
Now we know that to receive voice modulation with good readability, we need only about 5 or 6 kilocycles
bandwidth, and we can get along with even less, if we have to. Thus, there will be little, if any, difference
in the sound of a 2-meter signal with the selectivity control in either of these two positions, but
the receiver noise that will be present on a weak signal will be vastly greater with the wide bandwidth.
Consider curve C. This was not taken from any particular receiver, but it is about the best that
could be expected with a receiver having a high intermediate frequency and no crystal filter. It might
be one of those Command sets, with the 2830-kc. i.f. systems, for example. One look at its selectivity
curve shows that this is not going to make a hot v.h.f. receiver, no matter how good a converter we
put ahead of it. The bandwidth would be fine for 2-meter mobile work, but don't rely on it for home-station
use if you want to hear the weak ones.
The bandwidth of the SCR-522 is even broader. That was a fine receiver for non-critical fixed-frequency
work, the purpose for which it was intended. It is not a top-flight weak-signal receiver, and no amount
of work on the front end will make it so. The way to hop up reception with a 522 or any other broad-tuning
receiver, assuming that you've already done a job on the front end, is to take the output of the high-frequency
i.f. and feed it into a communications receiver, where the passband can be reduced to the minimum needed
for voice intelligibility.
This noise-bandwidth relationship also shows why it is a waste of time to convert radar-type receivers
to amateur use. Progress in our 420-Mc. band has been delayed several years because of the availability
of the APS-13, the BC-645, the BC-788, the ASB-series receivers and other broadband devices on the surplus
market. They're fine for local work, receiving the broad emissions of modulated oscillators, but useless
for weak-signal DX reception. Just imagine their bandwidth of four megacycles or more presented in the
manner of Fig. 1, and you see why one of these receivers is a millstone around the neck of the ham who
has just jumped into the u.h.f. pool!
One last thought on this selectivity business. So far, we've been talking about the minimum bandwidth
needed for voice. We can't clip much sharper than 3 kc. and still copy voice modulation. But we can
go down to a bandwidth of a few hundred cycles and get along nicely on c.w. There is an obvious point
here for the fellow who wants to work real v.h.f. DX - there's no way to do it like using high selectivity
Many of the newer crop of double-conversion receivers have selectivity that was impossible heretofore.
With them, and a good v.h.f. converter, we can dig down into the noise level in a way that we never
could before - if we will take advantage of the possibilities that c.w. operation affords.
You Can't Work 'Em If You Can't Hold 'Em
High selectivity is great stuff - but you don't get that boost in signal-to-noise ratio for nothing.
When you start thinking of bandwidth in cycles, you come up against stability problems. A wandering
oscillator doesn't cause much trouble when the i.f. bandwidth is 50 kc. or so, but to use selectivity
effectively the converter oscillator has got to stay put!
This rules out tunable oscillators for the average v.h.f. man, so we turn to crystal-controlled injection
sources. A crystal-controlled converter is nice to have, even on 28 Mc. It is more of a pleasure on
50 Mc. At 144, 220 or 420 Mc. it becomes a necessity for narrow-band work. Fortunately, crystal control
in the converter is not difficult. Even for 420 Mc., two dual triodes and a low-cost crystal will provide
enough energy in the vicinity of 380 Mc. to replace a one-tube oscillator covering the same frequency.
And what a difference! - 420-Mc. signals received on a crystal-controlled converter tune in as easily
as a signal on 7 Mc., and c.w. is just as practical. No more holding one's breath, or tuning signals
in and out by waving the hands a foot or two away from the receiver. It is no exaggeration to say that
the general move to crystal-controlled reception at 144 Mc. and higher in late years has been one of
the most potent factors in demonstrating the utility of these bands for amateur communication.
* V.H.F. Editor, QST.
Posted September 13, 2016