CQ tv81
CQ tv81
•T
TELEVISION CLUB .
FEB 1973
1
THE BRITIS H
AMATEU R
TELEVISION CLU B
Committee Members and Club Officer s
EDITORIAL CONTENT S
NOTEBOOK No1 2
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large positive current applied to the base . of current causes the scanning coils, i n
The collector falls immediately to almos t parallel with C7 the flyback capacitor, t o
zero volts and the scan coil has a voltag e oscillate at their natural resonant freque-
step almost equal to the supply voltag e ncy, shown dotted in Fig . lb . However, D 2
across it . will not allow the collector to swing nega-
tive and as soon as the negative half-cycl e
Thecurrent through the coil build s
of the natural oscillation commences D 2
up in a linear manner giving a substantiall y
conducts, driving current through the scann-
linear deflection . At the end of the line
ing coils and starting off the next scan .
scan the transistor is switched off agai n
by reverse biassing the base and the coll- D2 is forward biassed by the potential
ector once more becomes an open circuit . divider R14 and HIS to ensure a smooth cha-
This causes the current and magnetic field nge over from reclaimed scanning current t o
in the coils to collapse producing a rapi d current provided by the line output transis-
deflection in the opposite direction an d tor Tr5 .
generating a reverse voltage having a high An additional choke L2 is provided t o
peak value as shown in Fig . lb . enable shift currents to be passed throug h
the scan coils for picture centring . The
A complete practical circuit of a lin e SHIFT control is RV3 .
scan generator is shown in Fig . 2 . In thi s
Scan amplitude is determined by th e
circuit the line oscillator consists o f
voltage applied to the output stage and
Tr1, Tr2 and Tr3 connected to form an as -
this is adjustable by RV2 the WIDTH control .
table multivibrator . This is synchronise d
at line frequency by negative going lin e With a 12Volt supply rail and norma l
drive or blanking pulses applied to Cl . Em- direct drive transistor type scan coils ,
itter follower Tr3 is included to ensur e this circuit, which is based on the Lin k
good waveshape at C5 . The line frequenc y 101 Camera, will provide more than adequat e
European Amateu r
tv Reporting Syste m
Picture Carrie r
Sound Carrie r
Remark s
B4,5 It should be possible to lock both frame and line by careful adjustment .
B6 The call sign should fill the screen, and it may be necessary to darken the shack to read it .
B7 The picture should be of a well known person, such as the Queen or some local personality .
B8 Scales, and the hands of, watches should be discernible .
B9 3MHz on 625 should be resolved .
B9+ 400 v should be available from the aerial .
7
The amateur who has managed to produc e only, to lowlights, and not lowlights plu s
colour captions by simply feeding the out - highlights as would otherwise be the case .
put of a monochrome camera into the R,G or B Output "C " , also inhibited by blanking ,
input of a coder or a monitor will fee l produces an output when " A " or " B " are i n
that the next step should be to build a a low state and thus produces a signa l
prover " synthesiser " , where the artific- corresponding to the blacks, or backgroun d
ially produced colours are infinitel y of the picture .
variable . Figure 2 shows the output stages . The
The synthesiser to be described split s nine potentiometers provide independen t
the video input (from the monochrom e adjustment of the proportions of red, gree n
source) into three levels, such that a or blue for each of the three levels, an d
different colour can be set up for eac h are the controls which should be mounted o n
level . A total of nine potentiometer s a front panel . The output filters are pro-
are thus required to control the colou r vided to limit the frequency spectrum o f
output . the outputs to that corresponding to th e
625 line system bandwidth .
Figure 1 shows the actual level split-
ter . The video is first clamped, and the n With careful use of crayons applied t o
fed into two level detectors, the switch- a caption made with white " Letraset " t o
ing level of which is made variable by produce three brightness levels (i .e . black ,
means of preset potentiometers . The out- grey and white) quite reasonable thre e
puts from the two level detectors are the n colour captions can be produced using thi s
fed to a gating system ; for output "A " synthesiser . Very colourful effects ca n
(highlights) the signal is inhibited b y also be produced by pointing the camera
blanking, but is otherwise unaffected . at an ordinary scene, and there is muc h
Output " B " (lowlights) is inhibited b y scope for artistic experiments alon g
blanking too, but it is also inhibited b y these lines .
"A " thus producing a signal corresponding
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9
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SECTION ON E
SECTION TW O
1 G3YQC 712 6 G6AGT/T 68Km 2 - 0
Some twenty one /T stations took part altogether, with thirty one sound only stations .
Conditions for the first weekend were above average, which added to the normal range expecte d
for atv .
It is a pity that so few stations submitted an entry, and it is hoped that more will d o
so with the atv cumulative contest now being held . Please note one omission from the publishe d
rules, in that there will be two sections to the cumulative contest : -
A. For those stations transmitting at v
B. For all others .
The results of the September contest have been forwarded to our German friends, and w e
await the results of the International Contest with interest .
11
by Malcolm Sparro w
To receive Amateur Television these days need not be as hard as it used to be in the ver y
early days when A .T .V . had just started ; in fact, using the new Mullard ECL 1043 tuner uni t
makes it just about as easy as possible .
The one saying to remember when trying to receive any UIL' signals is that "A chain is only
as strong as the weakest link in it " . In ether words, provided that there is an ATV signa l
on the air, to receive it one requires : A 70cm aerial, a coaxial cable to connect it to th e
tuner unit, a tuner unit, and a tv receiver . If any of the items does not function properly
then the results will be impaired .
These days it is rarely worth trying to design and construct your own aerial . J . Bea m
Engineering Ltd . of Northampton produce a range of 70cm aerials and the beginner would be wel l
advised to start off by purchasing one of their aerials such as the 18 element parabeam (Cat .
No . 70/18P,) price £7 .45p, which has a gain of 17dB over a plain dipole . (Do not use thei r
14 element skybeam aerial for ATV as this aerial does not have a suitable band width for ATV .
Whichever aerial you finally decide upon, the next thing to consider is where to put it .
In practice it will pay to try to mount the aerial so that it is clear of all the roof-to p
obstructions as wet tiles can make quite considerable signal attenuation at 70cm . Also som e
provision for turning the aerial should be made to enable an incomming signal to be peaked fo r
maximum . This may not coincide with the most direct route to the transmission source .
Having decided upon which aerial to use and where and how you are going to mount it th e
next thing to consider is the coaxial downlead .
This should be as good a cable as you can obtain and afford . There is no point in erecting
a high gain aerial only to loose all the signal before it gets to the tuner unit . One shoul d
use a good quality low loss BBC 2 type coaxial cable such as " Aerialite Type M4205 Aeraxia l
Cable " . This is a e inch diameter coaxial with a cartwheel cross-section . That is, the in-
sulator between the inner and outer cables is partially air-spaced . A point often overlooke d
when using this type of semi-airspaced coaxial cable is that although the air in these hole s
in the cable is dry when you purchase the cable new, it will soon become damp when connecte d
to the aerial way up in the air .
12
Whilst the cable will give first-class results when .first connected to the aerial it wil l
soon deteriorate in performance if steps are not taken to trap the dry air inside the cable .
This is simply acheived by cutting the cable to the required length to be used - always kee p
it as short as practical and do not leave large lengths in use just to avoid cutting a run o f
coaxial cable - and then by melting the insulator at each end of the cable, seal each end t o
keep the dry air in the cable before attaching it to the aerial . This can usually be don e
quite easily by using a dry soldering iron, but take care not to let the inner and oute r
cables short out whilst doing this .
The Mullard Varicap Diode Tuner Unit type ELC 1043 is available from Manor Supplies Ltd . ,
at £4 .50p each plus 25p post & packing . This tuner is built in a tinplate box with detachabl e
sides and is tuned by varying the voltage applied to the Varicap diode in it ; it should b e
connected up as follows :
The aerial lead should be connected to the input terminal which is on one end of the unit ,
the outer of the coaxial cable being soldered to the tuner chassis .
Next, refer to the pins and holes which are located in the base of the tuner unit betwee n
the four mounting lugs . Commencing from the end of the tuner which has the aerial input ter-
minal on it number these holes (some of which have pins in them) 1 to 11 and connect them u p
as follows :
• +I 2 v
-~ O
Pl 2 PIR4 P~V8 PIN 5
Purer chassis A .G .C . r .f . osc/mixer TUN E
Transistor Supplies .
The lKohm linear Variable potentiometer feeding pin 5 is the tuning control, whilst the
1K preset control should be set to feed pin 2 with 3v +ve to the tuner chassis . The outpu t
from the tuner is taken from pin 10 with the braid of the output coaxial cable being connecte d
to the tuner chassis .
The output lead should be taken to the aerial input socket of the tv receiver and th e
receiver set to channel one . With the tv set turned on and 12v dc . applied to the tuner (an d
the aerial connected to the tuner), you are now all set to watch for ATV pictures provide d
that there are some on the air to start with, of course .
Once a signal has been received the I .F . output coil slug in the tuner can be tuned for th e
best signal but there will probably be only a slight improvement .
13
This equipment will provide an up-to-date ATV receiving system which will be on a par with
any valve tuner plus low noise transistor preamplifier, as the Mullard Tuner noise factor i s
quoted as being 8dB .
It will of course be necessary to change over the detector diode polarity in the tv se t
and also the link time base frequency if you wish to watch 625 line -ve modulation ATV as th e
system as described is intended for 405 line +ve modulation ATV as mainly used by amatuer s
outside the London area .
Finally, do not put more plugs and sockets in your 70cm aerial down lead than absolutel y
necessary, as each time you use one you will lose a little of the signal .
NOTE : If you want to tune the whole of the television band IV with your tuner it will b e
necessary to arrange for the timing voltage on pin 5 of the tuner to be varied between 0 .3v
and 28v +ve, but the circuit as shown should tune the amateur 70cm band without any need fo r
internal modification to the Mullard Tuner unit .
If you are interested please drop me a line immediately . I suggest if you are intereste d
that you sked me on 11 .30GMT on Wednesdays on 1423OKc/s and we can arrange for a contact throug h
the satellite . Oscar 6 is turned on on Thursday, Fridays, Saturday and Sunday evenings as wel l
as Saturday and Sunday mornings . This saves on battery power since one of the solar panel s
is having trouble . If you skeded me on Wednesday we would be ready for weekend passes . Another
way to alert us is to contact the slow scan television net which meets at 1800GMT on 1423OKc/ s
each Saturday afternoon . I am one of the net controllers and can always be reached directl y
or by relay from the Atlantic coast at that time .
Tne procedure for making contacts is to broadcast continually on your chosen frequenc y
for the full 20 minutes of the pass and to check later to see if you were seen or heard . The
early pass of the evening is the only one of that group where we have a chance of seeing eac h
other across the Atlantic . WA9UHV and myself are operating on 145 .930 and 145 .940 respectively .
This brings us out at 29 .480 and 29 .490MHz respectively . If you can sked me I can alert yo u
to the possible passes where we might have success .
Please let me hear from you . Satellite communications are a great deal of fun and ar e
very exciting .
Don C . Miller ,
Waldron, Indiana ,
Box 95, 46182 ,
U .S .A .
OSCAR6
Oscar 6 was launched on 15th October 1972 from Vandenburg, California, piggy-back fashio n
with a weather satellite . The Oscar translator was designed and built by the AMSAT organisation ,
a group of radio amateurs dedicated to forwarding the technology of Radio Communications .
The translator has an input band around 145 .5 and an output band from 29 .45 to 29 .55MHz .
All modes of radio communication can be translated .
The orbit of the satellite is polar with an inclination of 101 .73 degrees and a period o f
114 .5 minutes . There is a telemetry beacon on 29 .45MHz . The "CODESTORE" memory of Oscar 6 i s
capable of being loaded with ground based information while in orbit . WIAW, the official
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American Radio Relay League station, constantly transmits undating information to all intereste d
radio amateurs on the QST published frequencies . Announcements are made in both ' phone an d
RTTY .
The photos show W9NTPs gear which made the first two way QSO through Oscar 6 . The firs t
contact was made on orbits 30 and 41 and by October 40 pictures had been exchanged wit h
WA9UHV . The gear at W9NTP comprises a HeathSB101 high frequency transceiver with 30w out, a
homebrew linear 100w 2m amplifier with a 4CX250 in the final, a 10 element vertically polarise d
2m antenna, rotable in azimuth only, a 10m 4 element rotable Yagi, a NX-303 National Hamban d
receiver on 10m and a homebrew sampling SSTV camera with 7 inch monitor . Similar equipment i s
used at WA9UHV except that the aerials are notable in azimuth and elevation .
' 9NTP reports that QSB is so severe that it is difficult to get even one complete SST V
frame . The main problem seems to be "power robbing" by other stations, but as can be seen by
the photos (see this page and the front cover), some success has been possible .
Richard Thurlow, G3WW, of Wimblington, Cambridgshire has sent us some information about a ne w
specification for SSTV, as used by the M .P .T ., resulting from some considerable correspondenc e
over the last few months . This is how G3WW tells the story .
"To those of you who I have pestered for information by phone calls, cablegram and letter s
as to why and how the ROBOT camera with its 128 lines is allowed to be used universally in bot h
the 60Hz and 50Hz AC Mains areas of 120 lines standard, I hasten to report that after passin g
on to London the excellent information gathered, especially from K6IV himself, W4BW the Chie f
of the Amatuer and Citizens Division of the FCC . thro my good Attorney friend of 1960 Washingto n
DC visit W3GZ/4, and KIPLP Asst . Tech Ed . QST who reviewed the ROBOT equipment, that in the US A
the 120 line standard is one adapted by the US Amateurs and is not regulated by the FCC, and tha t
ROBOT have departed from the accepted standards in two respects on the grounds that the perform-
ance is improved and the signal from the camera is received well by all monitors i .e . 128 line s
per picture and Vertical sync pulse duration 66 milliseconds rather than 30 milliseconds, I have
16
today received permission from the Ministry of Posts and Telecommunications (per Mrs . A .I .
Campbell) to use SSTV under fresh conditions .
our engineers have now reviewed the technological aspects of the equipment required t o
meet our specifications and I have pleasure in advising you that we are prepared to grant yo u
permission to use the following bands : 7-7 .10MHz, 14-14 .35MHz, 21-21 .45MHz, 28-29 .7MHz ,
144-146 .OMHz two year period etc . P .S . Enclosed is a copy of our revised specification whic h
covers ROBOT 80 ' .
SLOW SCAN TELEVISION SPECIFICATION
Get some ideas from other members in you r address is on page 1, and this time we hav e
area (the Treasurer will tell you who the y a little extra to ask of you . To enable
are) and we will try to get at least on e us to bring our records up to date, if yo u
Committee member to attend to bring you up have a Postcode, could you let us kno w
to date . Just give us a reasonable amoun t what it is . Also, if the address on the
of notice ; remember it takes approximatel y envelope you received this C Q - T V in i s
ten weeks to get a letter into print i n wrong in any way, please let us know abou t
C Q - T V. that too . This will help us, the Post Office ,
and ultimately, yourselves .
Finally may I wish you all you wis h
yourselves for 1973 and here ' s to a mor e At the next vhf Convention, to be hel d
successful, and dare I say, colourful at v as usual at Whitton, B .A .T .C . would like t o
year to all our members and let us al l have an organised display, if at all possible .
remember to try to communicate . Dave Lawton G6ABE/T has taken on the resp-
Malcolm Sparrow G6KQJ/T onsibility for coordinating the effort, s o
Hon . Chairman B .A .T .C . if you will be there and would like to help ,
Once again subscriptions are due - or have some equipment you would like t o
it is only one pound, after all . And thos e show, please contact Dave - his address i s
who don ' t pay, won ' t receive C Q - T V . printed on page 1 .
This article concentrates on the electronics of the scanner rather than the optics . I t
has been used at 03RHI without an optical system to make tape recordings for transmission b y
placing cutouts directly on the face of the station SSTV monitor tube . The contrast contro l
on the monitor is turned right down and the monitor raster is synchronised from the sync puls e
generator in the scanner . Thin card cut-outs or transparent acetate with black letraset letter s
are placed firmly on the tube and the 931A is stood about 12 inches away . Care is taken t o
minimise light leakage between the card or acetate and tube but provided this care is take n
god black and white captions and simple cartoons are recorded . An optical system using 35m m
transparencies would be a real improvement but so far the search for readily available part s
for an easily built lens and transparency changeover system has not been successful . By con-
trast all the parts for the electronics are readily obtained .
The power supply is conventional . The Crofton Electronics transformer, though not essen-
tial, might well have been designed for the job . The 12 volt supply is standard . The 5 vol t
regulator was placed on the modulator printed circuit board and wired in permanently to mini-
mise the risk of connecting 12 volts to the I .C .s . The photomultiplier EHT is a standard ful l
wave voltage doubler connected to the 200+ volt HT winding on the Crofton transformer . Th e
load is a modest 1mA but safety precautions should be taken since with this transformer th e
EHT voltage is some 480 - 500 volts .
This is enough for the 931A . Higher EHT can be used so long as the total voltage is mea-
sured and the resistor connected between X and the EHT calculated so that the total curren t
through the chain is 1mA using the values in Figure 2 . With EHT connected the tube should no t
be fully exposed to daylight or bright light . One of the old 14 inch coil forms or a piece o f
plastic tube with 3 strips of foam draught excluder inside make a good shroud . The outpu t
voltage of the tube is negative and a positive voltage is needed to drive the modulator . Th e
2N3819 buffer also conveniently inverts the signal polarity and its 2Mohm input control shoul d
be readily adjustable . Screened cable is used between the FET and point B on the modulator .
The modulator circuit includes a sync pulse generator .T7and T8 square the 50Hz voltag e
which is divided in IC3 by 3 and shaped by IC2 to provide line sync . IC4 and 5 together divid e
by 120 to give frame sync shaped by ICI . The heart of the modulator is the multivibrato r
around T3 and T4 . A ganged pot is not available for P3 and P4 but the adjustment of separate
18
19
pots in step is easily done . T5 is a buffer and a square wave is present at the collector whic h
is followed by a low pass filter . The result is a sine wave at the base of T6 which is an amp-
lifier to make up for the losses in the filter . On receipt of a sync pulse T3 and T4 must pro -
duce 1200Hz, and black 1500Hz and on white 2300Hz . T1 and T2 provide the means of varyin g
voltages to control this frequency . To set up the modulator a frequency counter is essential .
For initial adjustment the 2N3819 is disconnected from point B and the SPG is disconnected fro m
point A . The black pot P1 is then adjusted to give an output of 1500Hz . Point TP is then ear-
thed and the sync pot P2 adjusted to give 1200Hz . The FET output is then connected to poin t
B with the 931A covered to simulate black . P1 is readjusted since the frequency will rise a
few cycles in response to the 0 .5 volt or so always present at the FET output . The tube is the n
exposed to a bright continuous raster in a dark room and the 2M pot adjusted to give 10 volt s
at point B . The CRT brightness control is set at a sensible working level without any colou r
filter . P3 and P4 are then adjusted to give 2300Hz . Thus the multivibrator cannot go abov e
this frequency since the maximum voltage is controlled by the 10K resistor connected to th e
12 volt supply and thereby determining the FET operating point . The black and sync frequencie s
are then rechecked by the original procedure since adjustments are to some extend interdependant .
When completed the SPG is reconnected to point A . Prior to this the SPG outputs can be checke d
on a scope for voltage and length of pulses . Even with the so-called new but cheap I .C .s ther e
should be some 2 volts at point A and only 0 .6 volts is needed at the base of T1 . T1 is a
transistor switch which on receipt of a sync pulse bottoms its collector to achieve the sam e
effect as earthing TP during the setting up procedure . Throughout all adjustments a smal l
speaker connected to the transformer wads it and gives a good indication of success or lack o f
it . The unit is now ready for operation . The Mark I version was built on an open chassis whil e
Mark 2 was built in a diecast box with a rectangle cutout to expose the sensitive area of th e
931A .
Lucky the operator who has two monitors or a monitor and a separate CRT unit producing a
raster . With the raster set up in the dark about 12 inches away from the 931A and synchronise d
from the modulator a facsimile of the card cut-out or transparency placed on the face of th e
tube can be seen on the monitor to which the modulator is connected . If a second monitor i s
not available patience is necessary while the picture is tape recorded and then played back o n
See text
20
the monitor originally used to provide the raster . Although time consuming, with experienc e
results are good since the only two variables are the CRT brightness control and FET input . I n
practice the FET is set and the brightness is varied . Operation is best done in the dark s o
tape recording rather than direct transmission is more convenient .
FOOTNOTE : The author has a few printed circuit boards for the combined SPG and modulato r
priced £1 .60 . P1,2,3 and 4 are available fitted to this board at 40p the set . The 931A and
base are stocked be Henry ' s Radio .
16v
+ A B
Bridge
C
1 10p F
T1
VR_ RS components MVR 1 2
NEWSF LASH
INTEGRATES PART 11
CIRCUITS
A.CRITCHLEY Dip El; C Eng ; MIERE .
d /Rf
phase after feedback would cause oscillation .
I i = (v i - v n (/R i and I£
=(v o - v
Phase-shifting of the high-frequency response of a
high-gain amplifier is inevitable in circuits containin g
many transistors - as Cp . Amps . do . The technique use d
in taming these amplifiers is to ensure that the gain o f Ri Rf Rf
the system at the troublesome phase is less than unity .
or v i - v n = (vn - v o ) .Ri/Rf
So what is involved?
v i = Ri .( v n - v o ) + vn
Rf
The basic inverting amplifier uses a resistive feed -
back network as shown below and has a gain of -Rf/Ri - but vn = - v o/A, V . - Ri v o - v o -v o
assuming that the open-loop gain is infinite and that al l Rf( A A
other _`actors are perfect .
- Rf 1
Ri
i + 11Ri + Rfl
For an inverting amplifier the sum of the current s
A` Ri
at the inverting input is zero . i .e . I i + In + If = O .
2 2
Now B = R i /(R i + R f ), so the actual closed-loop gain 0 is : - The diagram can be simplified to the asymptotes onl y
and is then called a Bode plot . Such a reducing respons e
is always accompanied by a phase-change - in this case 90 °
lagging due to capacitor Cs - but transistors themselves
do have phase-changes at very high frequencies . With a
G - - Rf l 1 resistive NFB network the phase, in this example, will no t
Ri 1
+ 1 reach '- 180° and the system will not oscillate .
AB
The closed-loop gain depends on open-loop gain as w e
have already seen and to give an expression for the closed-
For the non-inverting amplifier G is : -
loop gain of such an amplifier we have only to include a
factor for the H .F . loss due to a CR network .
This is :-
A e A
G + Rf 1 w
1 + jw/wo
(
Ri}- 1 + 1/A B
The closed-loop gain is .-
These equations show that the closed-loop gain is reduced.
if the open-loop gain is reduced .
so co =wo ( 1+AB )
Bandwidth
This shows that the bandwidth of the closed-loop gai n
For a practical Op . Amp . the open-loop bandwidth i s greater than the open-loop bandwidth by an amount w o .AB
ris ,
that frequency at which the open-loop gain is 3 dB down
or the original bandwidth multiplied by loop gain .
on its value at low frequencies and a typical characteristi c
is shown for an amplifier containing a single time-constant . A 0PErv-LOP GAu
W. .A6 -''I
Above A and G are equal and loop-gain is zero .
woGL
The loop gain is seen to be maximum between d .c . and coo
and then to reduce at -6 dB/octave to zero at
w oC L
That is, it reduces because the open-loop gain reduces .
A 1
-ed~atwe
, j
r..Jux r . 1/c .R, .t
(Oak AK'8waasi)
Thee' -■ddg/odete Cd,
GAM
o I C
0 -
site
But, H = G and
min – Gregd Gregd _ A – A B
so H = G . However, G
For more feedback and less closed–loop gain C will b e min – (A – AB) min = A – w o2/w o l
larger . so Rint/R = A – w a AB – w
o 2/w ol – A + AB o 2/w o l
Unfortunately however, the closed–loop gain G is stil l
likely to be greater than unity by quite a considerabl e Thus R = Rint
amount . Luckily there is a better way to overcome this , aB – w
02f" ol _
Maximum–Bandwidth Lag Compensatio n
0 is found from w 2 = 1/CR, and since w 2 co ol ,
This uses part of the response of the Op . Amp . t o
attenuate the loop gain by putting a series resistor wit h C = 1/w
the compensation capacitor . o1 .`i
RP
Rp = Ri .R f
Ri + R f
B Ri alp
Ri + Rf Rf
25
Also v = A .Ic(R + 1/jwC) i .e . A times the voltage between Nov 1/w 1 (2Rp + R) = 1/w2R so w2R = w1 2Rp + w 1 R
the two input terminals . col
and R(w 2 — w 1 ) = w1 .2Rp, R e 2Rp .
w2 col
So v = Ri .Ic + D . (v o — vn )
n w
= Ie .Ri + v .Ri — v .R i
Rf n Rf 1
vn + v n .Ri = Ic .Ri + v o Ri w
Rf .Rf
It will be seen that these two formula Dare not dependan t
vn I1 + Ri= Ri I on the Op . Amp . As in the case of the maximum—bandwidt h
Rf
lag compensation w2 should be put at the original firs t
/ break frequency co
so v = Ri Ie + o Ri .Rf I Ic + v ol .
Rf~ _ \ Rf
w,,/w in dB gives the necessary attenuation in d B
1 + Ri Ri + R f required to lower the minimum stable closed—loop gain
Rf to the desired value .
Hence R is also 2Rp/(H — 1 )
Ri(Io .Rf +v o) Hence vn = B(Ic .R£ + vo )
Ri + R f The values for a 702 (see also further on) are given
but Io = v i — vn or Ic(Rp + R + 1/jwC) = v i — v n as examples
Hp + R + 1/jwC
Gmin is +40 dB, for a gain of 0 dB, H = 4 0
1 + A .B(1 R + I/,jwC
12Rp + R + 1/jwC
Comparing this with \ A which is the expression fo r
1 + A .B the gain of an amplifier ,
there is a modifying factor :
C
R + 1/,jwC
2RP + R + 1/jwC
ml is placed at the second break frequency of th e With simple lag compensation, 0 .1 µF to earth gives a
Cp . Amp, and the required attenuation is (dB) . 0 dB bandwidth of 501 KHz and m is at 250 Hz whilst A i s
.03/mo2
70 dB . This form of compensation is thus ideal for l .f .
This places at mo3 .
m2 integrators or other l .f . applications, but little else .
bz
W, 4a,3 R_20(l+Rf )
`` Hi
C = 0 .01(1 + Rf/Ri) µ F
LEAD Cen P.
CL
This extends the bandwidth in the same ratio as th e Rp = Ri .Rf .
RI + if
open--loop gain is reduced . The new closed-loop gain ca n
be lower by twice this amount and the loop gain greater .
As a guide to a typical Up . Amp . response, the 702 Rf 10 KR, CL 50 pF, Gain 0 dB, iiandwidth 23 MHz, R 200 ii ,
has the following value s and C 1 nF .
At high frequencies then, there has to be a compromis e So far in this series on Integrated Circuits the Op .
between amplitude and frequency - you can't have both . Amp . has been considered only with Negative Feedback, NFB .
What is the effect of Positive feedback ?
The spew-rate and the bandwidth are often quote d
separately from the full-output maximum frequency whic h This is of course feedback from the output to th e
non-inverting input . With no feedback at all the ver y
can be very mis-leading . Likewise the slew-rate is
often quoted at a high gain figure instead of Atunit y high gain of the Op . Amp . usually ensures that the outpu t
will be in a saturated state due to inherent imbalance s
gain where it is much less .
in the input circuitry . There is only a small region o f
Maxim frequency for full output,with no distortion , input voltage near Ov where the amplifier can in fac t
and clew-rate are related by the equation shown belo w amplify - this is (+Vsat - Vsat)/A . It should b e
(the gain, being unity) . - remembered that Op . Amp . supplies are normally two-rai l
or positive and negative .
The voltage at which the change occurs is called th e The oscillator can be symohron ; s d by inserting narro w
threshold and has the value *- Vosat RiARi + Rf) . pulses into the non-inverting input .
4 D
In this case the voltage across C cannot go more positiv e
than about 0 .6 V which is arranged to be less than th e
threshold voltage . The trigger pulse is negative--goin g
in order to make the output go negative .
The output will change state for a time : -
c
The operation is that the Op . Amp . saturates at som e t = CR log e (i + Ri/Rf )
voltage *-Vosat The voltage at, the non-inverting inpu t
. Reversing the diode gives a reversed output pulse an d
is then determined by the feedback ratio and is '-Ve Ri the input trigger must also be reversed .
sat Ri + R f
If the Op . Amp . is in positive saturation then the fe d Heave table - 2
back voltage is also positive and so C charges positively .
via R until Vc reaches +Vo w„+ . Ri/(Ri + Rf) . Another type of moves table can be made in which th e
period is determined by a reference voltage .
The amplifier output then changes state because th e
inverting input starts to go more positive than the non - The timing capacitor is placed in the Pith path an d
inverting input . That is , the output goes negative . the output is normally at +Vosat' The inverting inpu t
C then begins to charge towards -Vosat .Ri/(Ri + Rf) and so on .
will be at -Vref (as is the other input) .
The period of oscillation is : -
The input trigger pules must exceed Vref in order t o
unsaturate the Op . Amp . i .e . it must be positive-going
2CR log 1 + Ri/(Ri + Rf)
2CR log e (1 + 2Ri/Rf ) with an amplitude greater than Vref . The output voltag e
l - Ri/(Ri + Rf ) change from + Vsat to - Vsat is passed via C to the non-
inverting input and C charges via R until the voltage a t
If Ri = Rf then t = 2,2 CR econds .
29
Constant-current sourc e
(ems) Vs RI z {— Rf -v
> JjAyrr
L .r e
t
+v ; pen I
The Op . Amp . can be ccnsisdered to have a gain of + 2 p0
4
at the non-inverting input since the PIFB resistor is th e ru ViY —
same value as the input resistor . On the other han d
R{
there is positive feedback to the same input which i s
attenuated by 2 because of R2 and N . Any change at th e
non-inverting input is thus accompanied by an, identica l
change at the same point due to the Op . Amp . This can It is evident that this form of constant-curren t
be considered as a resistor with the same voltage at bot h source is very useful and it has two more advantage s
ends - it has infinite resistance . The non-inverting yet, The first is that either positive or negativ e
input thus exhibits infinite resistance which is th e currents may be obtained by positive or negativ e
condition for a constant-cu rrent source . Another name voltage (low impedance) to Rl or by negative or positiv e
for this principle of 100 % feedback is bootstrapping . voltage (low impedance) to Ri . The second is that by
Cvm'tsi( nI = 'tr varying the ratios of the feedback arms the linearity o f
Re a sawtooth waveform can Abe varied in both directions .
R, 2 R f Furthermore, the linearity control is to a large exten t
R, R C independent of the amplitude, i .e . it does not cause an
amplitude change . This system of sawtooth generation
is therefore ideal for a scan generator .
R Rf
Errat a
This circuit provides a convenient way of generatin g The next part of this series wail examine enure mor e
sawtooth waveforms as the next diagram shows . The trans- uses of Op . AM-pa ., also better Op . Amps, than the (41
istor is used to discharge the capacitor to start th e and will include some other types of Linear ICn shic h
sawtooth . The voltage across the capacitor is directl y have been held ever from this time ,
proportional to the current in R1, which is proportiona l
to +V, and so a positive ramp results as C charges up . It is also hoped to describe the (-segment decoder s
and i.ndieaters in the next issue, a.s well as some mor e
The sawtooth level may be detected at a certain leve l digital circuitry ,
by means of a net mitt-trigger or similar level-dependan t
circuit and the output used to turn on the dischargin g Reference s
transistor . This results in a free-running generator .
A uni-junction transistor could be used too . Manufacturers' information shhets for IC date .
~ raft Wireless World, Fob 1969 - Series on Operational Amplifier s
by G .B .Clayton, B .Sc .,4 .Inst .P . (in nine carts . )
Mullard Linear .Appliaatior Note TP 308 6
SGS/Feiiehilf, The application of linear micron-resit s
RCA, Linear Integrated Circuit Fundamentals - Technica l
Series IC-40
Linear Integrated Circuits . Theery and Applications b y
Jerry Rimbinder . John Wiley and Sons .
Acknowledgemen t
R5 Rf
If a histahle is driven from the voltage-detecto r The author wishes to thank the Directors of EMI Soun d
the output can be used to change inputs to the constant- and Vision Equipment Division for permission to publis h
this article .
current source so Mist the ramp, instead of being taker.
31
A .W . Critchley ,
The 47 F should be a reversible type, The 70 Sussex Road ,
330 ohm resistor is best adjusted for min- Ickenham, Uxbridge ,
imum modulation . The idea came from a Middx . U810 8PN
fairly vintage Sylvania S .P .G . Tel . Ruislip 39148
33
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