low-cost.pdf

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low-cost spectrum analyzer
with kilobuck features
Build WA2PZO's
MHz on the UHF TV == 500 MHz - 800 MHz. When
the sweep width is set at zero, each of these bands
of frequencies may be manually tuned just as in a
single-frequency receiver. Both wideband FM and nar-
rowband FM signals, and surprisingly, even amplitude
modulated signals are detected quite well by the FM
IF amp /detector IC and amplified by the audio IC.
Figure 1 is a block diagram of this spectrum analy -
zer using a Sanyo varactor tuned TV tuner. A ten-turn,
10k pot with + 35 VDC across it is used to adjust the
center frequency of the tuner. A low varactor bias
yields low frequency and a high varactor bias provides
higher frequency on the TV band to which the tuner
is set. The sawtooth sweep voltage that is capacitive-
Iy coupled into the tuner's varactors is the horizontal
sweep voltage from the oscilloscope. If your scope
doesn't have the horizontal sweep output (the Heathkit
OL-1 does not), just mount an RCA phono jack on the
front of the scope and bring out the horizontal sweep
from the scope 's horizontal multivibrator to this point.
The 100 kilohm load across the horizontal sweep out-
put should have little or no effect on the scope's
operation.
Besides the TV tuner and scope , the rest of the cir-
cuit consists of only three integrated circuits. The
second mixer /oscillator chip is a Siemens S042P. The
ceramic filter is a Murata SFJ two-section filter at 10.7
MHz. The combination IF amp /detector/ AGC amp is
a National LM-3089N, and the 1/2-watt audio amp is
a National LM-386N.
useful instrument
for operating position
and lab bench
Although laboratory-grade spectrum analyzers
cost $4500 or more, you can build a spectrum analy-
zer offering many features of its costlier cousins for
about $50. How can such amazing capabilities be had
at such incredibly low cost?
• Through the use of a commercially mass-produced
varactor tuned TV tuner that covers the VHF low, VHF '
high, and UHF TV bands. It will tune down through
the 2-meter and 6-meter Amateur bands without
modification, with better than l-microvolt sensitivity.
By using a crystal-controlled converter and a narrow-
er IF filter, anyone of the HF Amateur bands could
be viewed as well, by simply upconverting to a TV
channel.
• Through the use of consumer-grade integrated cir-
cuits in the oscillator/mixer, dual ceramic filter, IF am-
plifiers / detector, and audio amplifier (offering audio
as well as scope output it is really a spectrum monitor).
• Through the use of your own oscilloscope. Just
about any scope may be used; I used a 1951 Heathkit
Model OL-l with its original cathode ray tube.
construction, testing, and alignment
Figure 2 is a schematic of the analyzer. A printed
circuit board is available from WA2PZO; I recommend
using this and WA2PZO parts kits . (Although the pots,
S-meter, and speaker aren't furnished, most are avail-
able from Radio Shack .I Figure 2A shows the com -
ponent layout on the WA2PZO printed circuit board
(foil side down). Alternatively, you could use perfboard
and point-to-point wiring.
Figure 3 is a schematic diagram of the interconnec-
tions between the Sanyo tuner, the three-IC printed
circuit board, and the scope , Once everything is con-
nected as shown in fig. 3, alignment can begin. (It
should be easy, since there are only four adjustments,
spectrum analyzer applications
Spectrum analyzers allow the user to observe in real
time an adjustable/variable bandwidth of radio fre -
quencies. One of the earliest spectrum analyzers for
the ham bands was the " Panadaptor, " manufactured
by Hallicrafters in the early 1950s. I used one to check
for F2 propagation 6-meter band openings in the
mid-1950s and credit the panadaptor with my earning
the IARU 6-meter WAC award (phone) issued by the
ARRL.
The band of frequencies swept by the spectrum
analyzer described in this article may be varied from
zero up to about 38 MHz on VHF low TV = 50 MHz
- 88 MHz, zero up to about 85 MHz on VHF high
. TV = 135 MHz -
By Robert M. Richardson, W4UCH, 22 North
Lake Drive, Chautauqua, New York 14722
220 MHz, and zero up to about 300
82 UI September 1986
836276906.045.png
the ferrite cores in Ll , L2, L3, and L4.)
With all the parts on hand - and assuming you're
using the PCB - assembly ti me is at most an hour
or two. I t uned up my uni t using only a grid dip meter
as a signal source in about 20 minut es.
Construction of the PCB proceeds as follows:
1. Install the jumper at the lower edge of U3 as illus-
trated in fig. 2A.
2. Install the 11 resisto rs as shown in fig. 2A .
3. Install the 16 capacitors as indicated in fig . 2A.
Since C6 and C7 are electrolytics, be sure to observe
the polarity indicated in fig. 2A.
4. Install t he Murata ceramic filter , FLl . Because it's
sym metri cal, it can be installed in eit her direction.
5. I recommend carefully installing sockets for U1
(16-pin DIP), U2 (8-pin DIP), and U3 114-pin DIP).
6. Install L1 through L5, carefully bending the pins
slightly so that they fit easily into the PCB's pre-drilled
o
1----. ~~~~
+3!5VDC
f xce p t as ind ica t. d, dec ima l
~.'u.s of cap.lc Uance . ,. in m ic l O-
'.reds (" Fj; ofha, • • ,. in plco'.,-
ads (p F); , •• i, r. ltCe S .t,. i n oh ms.
/(
O.~
600V
SC OPE
WI DTH
1.000
::::: ' .000.000
M
z
HORIZONT A L
SA WTOOT H
OU T
fig. 1. Block diagram of WA2PZO spectrum analyzer.
R,O
120
R2
12 0
+I2V
+ 12V
,
:Jli
,~
RII
' Ot
4~
~
111Hz
8
'0. 7I11H z
'0
2
~
c,e
L4
u 2
22 0
UI
S042P
C9 L/Ii~OB9
9
0.0 4
2
II
R9
~60
4
6
9
'4
' 2
B
,0
CII
C4
R~
0. '
e
3 3
~t
12
0.0'1
C,O
+ 12V
13
R '
12 0
<t, ' 4 ,1 6
Exce pt as in dicated, de c im al
Y"/ues 0' capac/t. nee . ,. In miCro-
farads (I,F); other s iH e In p icO /i1t .
a ds (pF} ; res isfa nce s a t. In o hms.
" = 1.000
1 0 . 0 ' C6 l/OrOJlF_,",--,
.:;::~,,' 'L--r:-~
+
CI 2
C7
M ::I:
1.000 .000
' OOk
fig. 2 . S chematic of WA2PZO spectrum analyzer.
September 1986 m; 83
836276906.046.png
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84 ~ Septe m be r 1986
836276906.047.png 836276906.048.png 836276906.001.png 836276906.002.png 836276906.003.png 836276906.004.png 836276906.005.png 836276906.006.png 836276906.007.png 836276906.008.png 836276906.009.png 836276906.010.png 836276906.011.png
f ig . lA . C o m p o nen t la yo ut o n th e WA2PZO p rin t ed ci rc ui l b o ard Uo il , ide d ownl.
_
hol es. Because l5, th e 150 p H induc to r. is sy mmetri·
ca l it ca n be ins talled in either d irec ti on.
7. M ost important: lubrica te t he small Iemte COtes of
L'l, L2. LJ, and l 4 with a d rop or lWO o f W D·40 beIOfe
attem p li ng adjustment. These cores are extremely brit-
tl e; use a pl ast ic o r nylon tuning 1001 ma tch ed 10 the
wid th o f t he f err it e slo t s (usi ng a m eta l o ne w ill gua r-
an tee their de st ructi onl.
8 . If you 're not usi ng a 2OO- pA S-m ate r, install a jum-
pe r fr o m ' A ' to g ro u nd .
Testin g an d a lig nment pro ceed a s t allo w s :
1. Connec t th e TV tuner' s V H F inp ut t o yo ur z. m erer
antenna .
2. Se t the V HF / U H F swit ch 10 the V H F p ositio n .
3 . Set th e Hilla sw itc h to Hi.
4 . M ake su re t he to p o f th e ferr it e co re in II is exact -
Iy ev an w ith th e top 01 its shi elded hou sin g .
5 . Se l t he sq uelc h conuol t o ze ro and adjus t the
vol u me cc nuo l fOI a slig h t h iss from t he spea ker WIth
the gai n control at ma ximum res .st ance 110 k ilo h m sl.
6 . Se t the wid t h co nuo t (saw tooth sw eep h o m sc o re !
to zero.
7. Co n nec t a von rneter t o p in
.
..... .......
_ &1<'1 0
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"
. 4 441:'''•
. .. . . .
. - '
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-
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. ~r ••• •
li g . J . S chematic s how in g in !... conn ect io ns bel w e .. n
!u ner . prinled CirCUli b oard. a n d os c illo s c o pe. N Ole ; + 35 .
4 20. a nd
10 o f the
TV tu ner
• 12 VO c SOUfC"", ar e regui llt ed s u p p lies.
+ 3Q·VOII voltmete r range
tve racto r mp u rl . Use the
l adj us t
th e ce n te r
frequency
10k ·tu rn
pol
so
th at
va rec tor bias is below + 30 V OC I.
8 . Turn t he can ter fr equen cy pot slowly dow n treduc -
ing va rac to e b ias vol ta ge) un t il a lo cal TV video earne r
is bot h heard on th e spea ker I buzz ) an d seen on t he
scope . If no TV stations are nearby , use a sign al qener-
a lar w it h mo d ulat ed o u tp ut o r a g rid d ip m et er .
9 . Peak the fe rri te slugs in L2 an d l3 f or m ax imu m
signal o u tp u t o n the scope .
10 . Co n ti n ue tu ni ng th e cente r fr equen cy POI un t il a
TV aud io sig nal is f ou nd , th en adjus t l4 for ma xim u m
Se p tem ber 1986 ~1 8 5
836276906.012.png 836276906.013.png 836276906.014.png 836276906.015.png 836276906.016.png 836276906.017.png 836276906.018.png 836276906.019.png 836276906.020.png 836276906.021.png 836276906.022.png 836276906.023.png 836276906.024.png 836276906.025.png 836276906.026.png 836276906.027.png 836276906.028.png
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~ '"
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