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STUDY OF LOW POWER TRANSMITTER
1. ORIGIN OF DOORDARSHAN
1.1 Introduction:
Doordarshan is the national service of India and is also one of the largest broadcasting
organizations in the world. A network of three nationals, two special interest channels; 10
regional language channels, 4 state network and an international channels. Through a network
of 868 terrestrial transmitters of varying powers it makes available television signals for over
87% of population. 300 million viewers in their homes watch Doordarshan programmes.
Television sets established under various schemes in community centers in villages for a total
number of 450 million viewers (India, 1998). The countrywide class room on national network
is aimed to reach quality education of students in small villages.
Television in India has been in existence for decades now. India did not begin till
September 15, 1959 with a small studio. The service was called “Doordarshan” for the first 17
years, it spread haltingly and transmission was mainly in black and white. Doordarshan was
established as a part of AIR, until 1976, it consisted of one national network and seven regional
networks. In 1992 there were sixty three high power television transmitters, 369 medium
power transmitters, 76 low power stations and 23 transposers. Regular satellite transmission
began in 1982.
Television has come to the forefront only in the past 21 years and more so in past 13.
There were initially two ignition points, the first in the 80’s when color television was
introduced by state owned broad caster. Doordarshan (DD) timed with 1982 Asian games
which India hosted. It then proceeded to install transmitter nationwide rapidly for terrestrial
broadcasting. In this period, no private enterprise was allowed to set up television signals. The
second spark came in early nineties with the broadcast of satellite television by foreign
programmers like CNN followed by STAR T.V and a little later by domestic channels such as
ZEE T.V and SUN T.V into Indian homes. The number of Televisions sets in India increased
from around 500,000 in 1976 to 9 million in early 1987 and to around 47 million in 1994;
increases are expected to continue at around 6 million sets per year.
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If all the doordarshan centres, Mumbai has the most acute language problem,
having to cater to a cosmopolitan and varied audience in Hindi, English, Urdu, Marathi and
Guajarati. In 1984, doordarshan introduced a second channel for the big cities and permitted
cable operators to transmit locally made programs to fill the gaps in the schedule when
doordarshan was not in air. These cable operators grew from a few 100’s in the eighties to
more than 20,000 in the nineties.
Presently Doordarshan operates 19 channels, two All India Channels, 11 regional
languages satellite channels (RLSC), four State Networks (SN) an international channel and
a sports channel. Regular satellite transmission began in 1982. Now more than 87% of
population of the country can receive Doordarshan programmes through a network of
nearly 1044 Terrestrial Television Transmitters. About 46 Doordarshan studios are
producing television software.
The T.V. transmitters can be classified into three types basing on their coverage area,
radiated power.
High Power Transmitters
Low Power Transmitters
Very Low Power Transmitters
TYPE COVERAGE POWER
High Power
Transmitters
80-120 km >1kwatt
Low Power
Transmitters
15-20 km 100watt
Very Low Power
Transmitters
10 km 5-10watt
T1.0Various types of power transmitters &their coverage
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1.2 What is need of LPTS?
HPTS can cover the 80-120 k.m. if the area is flat area i.e. without any obstruction. If any
highest buildings or hills exists then coverage capacity reduces because of the transmitted
signals absorbed by them and they prevents the signal to go.At this time the transmission
system fails to cover some areas which are behind the hills or the tallest buildings, this lead to
the establishment of LPTS to transmit over a small distances of 15-20 km.
BLOCK DIAGRAM OF LPT:
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1.3 TV Programmes Transmission Using Satellite:
Fig1.0 uplink and downlink process of signal
TV Signals from studio are processed and up-linked to the satellite where these signals are
further processed and then down linked to the Terrestrial T.V Transmitters with the help of
transponders of the satellite. The signal received by the parabolic dish antenna is sent to the
TVRO of input output chain with the help of coaxial cable and then it is further processed and
modulated and transmitted into the space.
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2. TRANSMISSION AND RECEPTION ANTENNAS
2.1 Introduction:
Although there are many ways of communication in practice
today,e.g.,linetelegraphy,linetelephony,visual signaling etc.but the radio communication (also
called wireless communication),is the most fascinating and popular system of communication
these days.The essential requirements of any communication system are fundamentally same
eg.means of transmitting the message or intelligence,means to receive the
message.Inotherwords a Transmitter,a medium to carry the message or intelligence from one
place to another and a receiver. Radio frequency waves, produced at transmitter, are carried by
transmission lines to an antenna or aerial which radiate it in the form of electromagnetic waves
into the space.let us define an antenna.
2.2 Antenna
Antenna is a metallic device for radiating or receiving radio waves. So antenna in other words
is a transitional structure between a free space and a guiding device. And this guiding device
may take the form of a coaxial cable or any other transmission line which transports EM
energy from source to antenna.
2.2.1. Antenna Parameters:
1) Power gain
2) Directivity
3) Polarization
4) Radiation pattern
5) Beam width
6) Band width
7) Radiation resistance
POWER GAIN:
The power gain of an antenna is a ratio of the power input to the antenna to the power
output from the antenna. This gain is most often referred to with the units of dbi, which is
logarithmic gain relative to an isotropic antenna. An isotropic antenna has a perfect spherical
radiation pattern and a linear gain of one.
DIRECTIVITY:
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Directivity of a antenna is defined as the ratio of antenna intensity in a given direction
from the antenna to the radiation intensity averaged over all directions. The average radiation
intensity is equal to the total power radiated by antenna divided by 4π.
POLARIZATION:
The polarization of antenna is the polarization of the wave radiated by the antenna ie. the
polarization describes the orientation of electric field into the space.
It can also be defined as " the property of an electromagnetic wave describing the time varying
direction relative magnitude of the electric field vector.
Magnetic fields surround the wire and perpendicular to it, it implies that the electric field is
parallel to the wire. So, this configuration is applied even after radiation of waves from the
wire. So there arises the need for polarization of a radiating element.
Polarization of an antenna refers to the orientation of radiated electromagnetic waves in the
space.
Classification of Polarization:
Polarization is classified based on the orientation of electric field as linear, circular and
elliptical polarization.
Fig2.0 classification of polarization
Linear Polarization:
An electromagnetic wave is said to be linearly polarized if all the cycles of the wave has same
alignment in the space.
Horizontal polarization:
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If an electric field vector E lies in horizontal plane then the wave is said to have
horizontal polarization.
Vertical polarization:
If an electric field vector E lies in vertical plane then the wave is said to have vertical
polarization...
Circular/Elliptical Polarization:
If two linearly polarized waves which are simultaneously produced in the same
direction and are mutually perpendicular to each other with a phase difference of 90 degrees,
then we get a circularly polarized wave.
Circular polarization may be right -handed or left-handed depending upon the sense of rotation
i.e., phase difference is positive or negative. Circular polarization results only when the
amplitudes of the two linearly polarized waves are equal. If the amplitudes of the two linearly
polarized waves are not equal then we result in elliptical polarization.
We yet have another polarization called cross polarization which is basically the radiation in
the undesired direction.
At the TV broadcasting frequencies we generally use horizontal polarization as a
standard. At microwave frequencies the polarization we use depends on the type of
application. In any case the polarization of both receiving and transmitting antennae should be
equal.
RADIATION PATTERN:
A graphical representation of radiation properties of antenna as a function of space coordinator
is termed as radiation pattern.
BEAM WIDTH:
The beam width of an antenna is the angular separation between the two half power
points on the power density radiation pattern. It is also, of course, the angular separation
between the two 3-db down points on the field strength radiation pattern of an antenna.
BAND WIDTH:
It refers to the frequency range over which operation is satisfactory and is generally
taken between the half power points.
There are actually two separate requirements for large bandwidth (in excess of 10%)
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from antennae. The first is for antennae which could be narrowband but which are required to
operate at a number of separate frequencies within a fairly large range. High frequency
antenna's are often of this type, in which the required operation is helped by the fact when the
antenna is switched to a new frequency, compensating circuits can be switched in also.
RADIATION RESISTANCE:
The input impedance 'Zin' of an antenna is the ratio of voltage to current at its input terminals
where the power is fed to the antenna.
Zin = Ra+jXa
Ra = radiation part of impedance
Xa = reactance part of impedance
2.2 TYPES OF ANTENNAS:
Based on these there are different types of antennae. But basically used types of antennae are
as follows:
1) Folded dipole antenna
2) Parabolic dish antenna
3) Yagi-uda antenna
4) Horn antenna
5)v-antenna
2.2.1 Folded dipole antenna:
A variation of the dipole can be a solution to the problems caused due to dipoles,
offering a wider bandwidth and a considerable increase in feed impedance. The folded dipole
is formed by taking a standard dipole and then taking a second conductor and joining the two
ends. In this way a complete loop is made as shown. If the conductors in the main dipole and
the second or "fold" conductor are the same diameter, then it is found that there is a fourfold
increase in the feed impedance. In free space, this gives a feed impedance of around 300 ohms.
Additionally the RF antenna has a wider bandwidth.
2.2.2 Parabolic Dish Antenna:
A dish antenna works on the same way as a reflecting optical telescope. Electromagnetic
waves, light or radio, arrive on parallel paths from a distance source and are reflected by a
mirror to a common point, called the focus. When a ray of light reflects from a mirror or flat
surface, the angle of the path leaving (angle of reflection) is the same as the angle of the
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arriving (angle of incidence).If the mirror is a flat surface, then the two rays of light leave in
parallel paths; however if the mirror is curved, two parallel incident rays leave at different
angles. If the curve is parabolic(y=ax²) then all the reflected rays meet at one point as shown in
figure.
F-focus
Fig2.1 parabolic dish antenna
A dish is a parabola of rotation, a parabolic curve rotated around an axis which passes
through the focus and center of the curve. The received signal can be transmitted to the low
noise block converter(LNBC) through feed horn antenna.
2.2.3. YAGI-UDA ANTENNA:
A Yagi-Uda Antenna, commonly known simply as a Yagi antenna or Yagi, is a
directional antenna system consisting of an array of a dipole and additional closely coupled
parasitic elements (usually a reflector and one or more directors). The dipole in the array is
driven, and another element, 10% longer, operates as a reflector. Other shorter parasitic
elements are typically added in front of the dipole as directors. This arrangement gives the
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antenna directionality that a single dipole lacks. Yagis are directional along the axis
perpendicular to the dipole in the plane of the elements, from the reflector through the driven
element and out via the director(s).Directional antennas, such as the Yagi-Uda, are also
commonly referred to as beam antennas or high-gain antennas.
Fig 2.2yagiuda antenna
2.2.4 HORN ANTENNA:
A wave guide is capable of radiating radiation into open space provided the same is
excited at one end and opened at other end. The radiation through this feared out wave guide is
more than through that of a transmission line.
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Fig2.3 horn antenna
2.2.5 V-antenna:
It’s an omni directional antenna fabricated from the light weightAluminium tubes and
flats..The electronic wiring is concealed within the tabular structure of the antenna and is
sealed to prevent moisture penetration.A clamp is provided between the feed for clamping the
feeder cable to prevent strain on the cable connector due to swaying of the cables.Arubberhood
just above the feed point protects the connector from the direct rain. Average gain of V
antenna is 4.3 dbm and power is 100watt,frequency range 174MHZto 232MHZ in UHF band.
Fig 2.4 v-antenna
3. TELEVISION RECEIVE ONLY SYSTEM
3.1 Introduction:
The signal which is transmitted to the terrestrial system by the transponders in the
sattellites to be received by a parabolic dish antenna.The PDA consists of chicken mesh
which decreases the pressure on Antenna.The signal which is received by the PDA is
made to pass through a horn antenna later it connects to the LNBC (low noise block
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converter).LNBC is an amplifying device used to downlink the signal from GHZ range to
MHG range using a local oscillator frequency of 5150 MHZ. After down converting the
signal from GHZ range to MHZ range it is allowed to pass through a RF cable to sent the
received amplified signal to satellite system unit.
3.2 Parabolic Dish Antenna:
A dish is a parabola of rotation, a parabolic curve rotated around an axis which passes
through the focus and center of the curve. The received signal can be transmitted to the low
noise block converter(LNBC) through feed horn antenna.
The azimuth and elevated angles and the direction of the parabolic dish are different for
different satellites. They can be varied by using horizontal and vertical motors from the control
room. The azimuth and elevated angles can be given by the doordarshan organization.The
following table mention the polarization, azimuth and elevated angles of Dish, and the down
linked signal information for different satellites.
T.3.1 TABULARFORM
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PARAMETER INSAT 3A INSAT 4B INSAT 3C INSAT 2E
LOOKINGANGLE 93.5° E 93.5° E 74° E 93.5° E
DIAMETER 7.5 mt 6.3 mt 3.6 mt 6.2 mt
AZIMUTH 149° 149° 220° 180°
ELEVATION 67° 67° 63.2° 70°
POLARIZATION Vertical Vertical Horizontal Vertical
DOWNLINKED
SIGNAL
Regional
Signal
National and
News
National Standby
mode
National
The unlinking and down linking can be done in any one of the frequency bands available C-
band,X-band,KU- band etc.Fore.g.the 100LPT at Srikakulam operated in C-band.The below
tabular form shows the unlinking and down linking frequency ranges of various bands
T.3.2 DIFFERENT BANDS AND THEIR FERQUENCY RANGES
BAND FREQUENCY
UPLINK
BAND, GHz
DOWNLINK
MAJOR USES BAND
WIDTH
C-BAND 5.9 – 6.4 3.7 – 4.2
Fixed, point to point
ground stations,
nonmilitary.
500MHz
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X-BAND 7.9 – 8.4 7.25 - 7.75
Mobile(ships,
aircraft).Radio relay,
military only.
500MHz
Ku-
BAND
14 – 14.5 11.7 – 12.2
Broadcast and fixed-
point service; non
military
500MHz
3.3 Low Noise Block-Down Converter:
Fig3.1 Ku-band LNB with both sides uncovered.
A low noise block-down converter (or LNB) is the receiving device of a
parabolic satellite dish antenna of the type commonly used for satellite TV
reception. The device is sometimes called an LNA (for low noise amplifier),
LNC (for low noise converter) or even LND (for low noise down converter) but
as block-down conversion is the principal function of the device, LNB is the
preferred term, although this acronym is often incorrectly expanded to the
incomplete descriptions, low noise block or low noise block converter
It is functionally equivalent to the dipole antenna used for most terrestrial
TV reception, although it is actually waveguide based. Inside the LNB waveguide
a metal pin, or probe, protrudes into the waveguide at right angles to the axis and
this acts as an aerial, collecting the signal travelling down the waveguide.
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Fig 3.2 LNBC block diagram
The LNB is usually fixed on the satellite dish framework, at the focus of the reflector,
and it derives its power from the connected receiver, sent "up" the same cable that carries the
received signals "down" to the receiver. The corresponding component in the transmit link
uplink to a satellite is called a Block up converter (BUC).
4. SATELLITE SYSTEM UNIT
4.1Introduction:
The amplified downlink signal from the LNBC is given to the satellite system unit
through a cable of impedance 75Ω and 6MHZ bandwidth. The satellite system unit protects
the remaining system components from lightening and thunders. The received signal can be
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given to the exciter through the different stages. They are integrated receiver decoder (IRD) s,
audio programming amplifier, video programming amplifier TV demodulator and monitoring
amplifier. A distortion/noise level meter is there to show the signal level.
4.2 IRD:
IRD means an “integrated receiver to decoder”, which can be used to decode the
original baseband signal from the received one. In the past analog receivers are used but at
present analog systems are replaced with the digital receivers as they are more advantageous
than the analog receivers. It takes the received signal as input and seperatesaudio and video
signals from it. It has two output ports one is audio signal output and another is video signal
output. The audio and video signals are given to the audio programming amplifier and video
programming amplifier for correction purpose respectively.
Fig4.1 Integrated receiver decoder
4.3 AUDIO & VIDEO PROGRAMMING AMPLIFIER:
The unit I designed using latest devices and technology. This unit provides distortion
less audio output it has wide bandwidth and excellent signal to noise ratio(S/N ratio).This unit
has both line and microphone inputs. A VU meter is present in the unit for monitoring and
several other features such as short circuit protection in audio outputs and power supply. The
applications are in audio signal processing and used in sound monitoring applications in
studio, broad casting networks etc.
The function of video programming amplifier is to correct the video signal.
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4.3.1 AUDIO/VIDEO SWITCH:
The “audio switcher/electronics patch panel” is used in monitoring and test equipment
rack for a LPT.It receives the video signals and audio signals from different sources and
selects any one of them for further processing and transmission, with minimum deterorationin
the characteristics of the signal. Its special feature is that we can monitor any input channel
been selected for transmission without disturbing normal transmission. The main use of the
audio/video switcher is channel selection.
4.3.2 TV DEMODULATOR:
It is precision monitoring equipment for checking the quality of a TV transmitter in the
VHF and UHF bands. It reconstructs original baseband signal and connected to the exciter
stage.
4.3.3 TV PATTERN GENERATOR:
This unit consists of several LED lights .the signal from the receiver connected to the
pattern generator. to check whether the circuit good or not. when we connect the signal to TV
pattern generator ,then at the output(on TV set) we can observe the color pattern lines.
4.4 SYSTEM UNIT:
This unit consists of two switches which are used to operate two motors.one motor is
for adjusting the vertical angle of PDA. Another for adjusting the horizontal angle of PDA.
4.5 VESTIGIAL SIDE BAND TRANSMISSION:
In the 625 line TV system, frequency components present in the video signal extend
from 0 Hz to 5 MHZ. A double side band AM transmission would occupy a total bandwidth
of 10 MHz. To reduce the channel bandwidth and power, Vestigial sideband Transmission is
in practice. In the video signal very low frequency modulating components exist along with
rest of signal. These components give rise to sidebands very close to carrier frequency which
are difficult to remove by physically realizable filters. Suppressing one complete sideband
also not possible. The low video frequency contains the most important information of picture
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and any effort to completely suppress the lower sideband results in objectionable phase
distortion at these frequencies; it will look in the picture as smear. Therefore only a part of
lower side band is suppressed and radiates signal with full Upper Side Band together with
carrier and vestige of the partially suppressed Lower Side Band. This is called V.S.B or A5C
transmission. In the 625 line system, frequencies up to 0.75 MHz in the lower sideband are
fully radiated. So it is a double sideband transmission for lower video frequency.
(Fig4.2 Theoretical representation of the side bands in VSB transmission )
(Fig 4.2.1 F Curve of TV setTheoretical)
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4.5.1 RECEPTION OF VESTIGIAL SIDE SIGNALS:
Because of filter design difficulties it is not possible to terminate the bandwidth of
signal abruptly at the edges of sideband therefore attenuation slope covering 0.5 MHz is
allowed at either end.
(Fig4.2.2 Response for VSB reception)
Now these visual and aural signals are given to the exciter for further processing. In the
exciter stage, blocks like video processing unit , diode bridge modulator , delay equalizer ,
V.S.B filter , video up converter , linear amplifier , power amplifier and diplexer and
frequency multiplier process the video and audio signals. The combined visual and aural signal
after arriving the diplexer block is transmitted to mast antenna.
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5. EXCITER
5.1 EXCITER:
The audio and video output of the program to be connected to the Exciter unit. The
audio input is feed to the aural modulator through ‘blank module’, while the video is passed
through a video processor unit to its respective modulator.
The audio is frequency modulated using 33.4MHZ IF while video signal is amplitude
modulated using 38.9MHZ IF.
The modulated signal are combined in combiner and then up converted to the desired
transmitted channel frequency in IF channel convertor unit.
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Fig5.1 exciter
The video output power level is 10MW synchronous peak while audio is 1MW. In this
automatic level is available on real panel of the exciter, which can be feed from driver unit.
Exciter needs 28V for operation, and its supplied from 28V, 25A PSU units which was
connected in parallel as shown in block diagram.
A DC-to-DC converter provided in the exciter derives +5V to +15V to be supplied to
individual sub systems in the unit.
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fig 5.1.1.internal block diagram of exciter
Exciter is functionally divided into seven modules namely:
1) Video processor.
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2) Vision modulator.
3) IF corrector.
4) Aural modulator.
5) IF combiner.
6) IF channel converter.
7) DC to DC converter.
5.1.1 VIDEO PROCESSOR:
The externally applied video signal is feed to the video input amplifier. This amplifier
has high input impedance in order to provide the high ohmic loop through facility. The
amplified video signal is feed to the potentiometer and to the synchronous separator.
The potentiometer control the amplitude of the video signal from the input amplifier and
there by it determines the modulation depth. This signal is applied to switch directly as well as
through receiver pre corrector. The group delay equalizer introduces a pre distortion of the
video signal.
The synchronous separator consists of detector and a comparator. The peak level of the
synchronous pulse is applied to detector. The output from detector is used as reference level
for the comparator, which means that the synchronous pulse is sliced at 50% of the
synchronous peak level.
The back porch of the synchronous pulse initiates the “clamp pulse generator”. During
this clamp pulse period the transistor is off and saturated, where by the video signal is clamped
to zero in the junction. The clamp pulse does not affect the 4.43MHZ band stop filter ensures
that the color burst in the video signal. In the same period the synchronous separator is also
clamped to zero.
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When no synchronous is applied, the “DC restore” is switched. In this case the peak
value of signal is maintained.
A part of the video signal is also applied to the “video level detector” via low pass filter.
The video level detector consists of a peak detector followed by a DC amplifier. The DC
output goes to the meter in IF combiner unit.
5.1.2. VISION MODULATOR:
The vision IF 38.9MHZ is generated by a ‘TCXO’ and split in to three identical signals
by means of power splitter, The IF carrier is feed to the “vision modulator” which is doubled
balanced ring modulator. In order to obtain a carrier as well as the side bands from the
modulator the applied video signal is properly clamped to zero in video processor unit.
The white level is adjusted by means of R8. The capacitive balance is adjusted by
means of C1 and C28. The “VISION IF AMPLIFIER” which is a wide band amplifier
amplifies vision modulated. Amplifier further amplifies the vision IF to +10dbm. A SAW
VSB filter performs VSB filtering of the side bands with minimum group delay and high
reliability. Amplifiers compensate the insertion loss of VSB filter and finally band pass
amplifier amplifies the vision IF to a level to 10dbm. The power splitter splits the amplified
vision IF from amplifier to two identical signals, one for combiner and other for monitoring.
5.1.3 IF CORRECTORS:
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Fig5.2 IF corrector
Correctors are of two types. They are amplitude linearity and phase linearity
corrector.
1)Amplitude linearity corrector:
The transistors Q1 and Q2 form a linear amplifier, input to which is controlled by
potentiometer RV1. Transistors Q3 and Q4 form a non-linear amplifier input to which is
controlled by potentiometer RV2.
Adjust RV1 for minimum input to transistor Q1. Check for amplified input signal at
collector of Q4. Vary RV3 and check for appearance of distortion at Q4 output, because of
non-linearity. Set RV3 to position where distortion just appears.
Adjust RV2 for minimum signal at Q3 base. Check for distortion less amplified IF input
at collector of Q2. Next adjust RV1 and RV2 approximately for 50% signal passage, and
check for availability of amplified, IF at collector of Q5. Demodulate the IF output available at
TP3 through a TV demodulator and measure the synchronous picture ratio.
Vary RV2 and RV1 and ensure that the synchronous picture ratio can be varied by +/-
5%. Feed multi burst pattern from VTSG and adjust the frequency response to best possible
extent by varying VC1 and VC2.
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2) Phase linearity corrector:
The input signal is splits into 2 branches. Signal passing through Q8 and Q9 stage is
delayed using delay line and the other signal is processed through a non-linear amplifier
combining these two signals introduces phase difference in the output signal.
Disconnect the cable from TP1 and TP2 and solder it on TP5 and TP6. Adjust RV7 for
minimum signal at Q8 base and RV5 for maximum signal at Q6 base. Check for amplified IF
signal at collector of Q7 and introduction of distortion by RV6. Set RV6 to position, where it
just introduces non-linearity.
Adjust RV5 for minimum signal at Q6 base and RV7 or maximum signal at Q8 base
and check for the same IF signal at emitter of Q9. Adjust RV5 and RV7 for approximately
equal signal at base of Q8 and Q6,and check for amplified IF signal at collector of Q10.
5.1.4 AURAL MODULATOR:
Aural modulator unit consists of the following sections in a single
PCB.
1) Audio amplifier
2) 1KHZ oscillator
3) VCO
4) Mixer
5) APC
6) Meter circuit
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Fig5.3 Aural modulator
Audio amplifier:
The balanced audio signal at a level of +6dbm from the TVRO is converted in
to unbalanced signal by the op-amp U8. The output of U8 is taken through a front panel
potentiometer R83 to the audio amplifier U7. The audio amplifier uses a hybrid micro circuit
BNC 1003. A 50μsec pre emphasis is provided, which can be adjusted by the potentiometer
R87. The output of the audio amplifier is applied to the varactor junction of VCO to frequency
modulate the VCO signal.
1 KHZ oscillator:
The 1KHZ oscillator is consists of two operational amplifiers U9 and U10. The
frequency of the oscillator can be adjusted by R94 and distortion in output signal is minimized
by R92, oscillator is powered with negative supply only when front panel of audio selection
switch is in “INTERNAL” position. The output of the oscillator is level adjusted by R99 for
±50 KHZ deviation.
VCO:
The voltage controlled oscillator is a varactor tuned oscillator, the frequency of
which can be varied manually by the coil L5. Transistor Q16 forms the oscillator. The output
of the oscillator is taken through a buffer Q18, amplified by two stages Q19 and Q20. The
output of one of the amplifiers Q19 is feed to the mixer in the modulator unit and the output
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from the other amplifier Q20 goes to the IF combiner unit through front panel BNC connector.
The output of the VCO is frequency modulated by the audio signal from the audio
amplifier/internal 1KHZ oscillator, the DC bias current for the diodes is provided through the
resistor R48. The output level of the VCO is about 0dbm.
Mixer:
The visual IF carrier from the vision modulator unit and the aural IF signal from
the VCO are injected at the base of the mixer transistor Q1. The mixer output is at 5.5MHZ.
This signal is amplified by a common emitter amplifier Q2, the output of which transformed
into square pulses by the pulse shaping network formed by diodes D1 and D2. This square
wave signal is further frequency divided by a chain of dividers to give an output square pulse
at 537HZ which is feed to the APC. The division is carried out to minimize the phase error
caused by the frequency modulation of audio signal in the VCO.
APC:
The automatic phase control circuit is a sample and hold circuit using a CMOS
analog gate for sampling. The square wave signal from the divider chain of mixer is
transformed into a triangular wave by means of transistors and the output is taken through a
source follower. The output from the source follower is capacitive coupled to the analog
gate.
The sampling of reference pulses for the analog gate is derived from a
temperature controlled crystal oscillator at 1.1MHZ, the output of which is frequency divided
by a chain of dividers. The frequency if the signal from the divider chain is equal to that of the
divided signal from the mixer under the locked condition of the phase locked loop. The
analog gate acts as an error detector and the output of the gate is applied to the varactor
junction of the VCO, to correct the frequency through a low pass filter formed by R31, R33,
C18 and C30.
Metering:
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The meter circuit consists of an AC amplifier and a peak detector followed by a
DC amplifier. The DC output is feed to the modulation meter in IF combiner unit via back
panel wiring.
5.1.5 IF COMBINER:
It combines vision IF with sound IF’S and composite IF.
IF is automatically level controlled with feed back from IF channel converter.
Vision IF is detected for presence of synchronous pulse and inter carrier is sensed to
declared system health.
Fig5.3 Block diagram of IF combiner
5.1.6 IF CHANNEL CONVERTER:
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This Units Converts the IF input to the channel frequency and
attenuator at the input is used for setting the output level to the nominal level of 10dbm. A
wide band double balanced mixer is used for frequency conversion. A TCXO provides LO
input to the mixer and the up converted signal is filtered in a helical band pass filter. The
signal at the output of the filter is further amplified using two hybrid amplifiers. A directional
coupler is used for providing a monitor output at the rear of the module. The main output
passes through another band pass filter to reduce further unwanted signals. The final output is
available at the front. LO monitoring is provided on the front panel. This is achieved using a
resistive divider network.
5.1.7 DC TO DC CONVERTER:
DC-to-DC converters with very low input respectively output voltage ratings
have, due to the high current ratings, a relatively low efficiency. Therefore, it is necessary to
operate several converter stages in parallel to achieve an acceptable total efficiency. Here, a
possible solution for such a converter is presented. The input voltage of a (e.g. a solar
buffered) battery (12 V or 24 V) has to be converted into a DC-voltage of 350 V, e.g. for a
power transmitter. The total power to be managed is 1 kW. In the case of a single stage
inverter, this leads to about 100 A input current (causing peak values in the power switches of
up to 200 A). The resulting component stress is very hard and the design is also difficult to
handle. To overcome this problem a topology was chosen, which uses several converter stages
operating in parallel. All these stages operate at the same transformer leading to an optimal
flux exploitation of the core. In the case of the 1 kW converter described here, four stages are
used.
5.2 PRE-EMPHASIS &DE-EMPHASIS
In processing audio signals, pre-emphasis refers to a system process
designed to increase, within a band of frequencies, the magnitude of some (usually
higher) frequencies with respect to the magnitude of other (usually lower) frequencies in
order to improve the overall signal-to-noise ratio by minimizing the adverse effects of
such phenomena as attenuation distortion or saturation of recording media in
subsequent parts of the system.
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De-emphasis is a process designed to decrease, within a band of frequencies, the
magnitude of some frequencies ( usually earlier pre-emphasised ) with respect to the
magnitude of other frequencies in order to improve the overall signal-to-noise ratio by
minimizing the adverse effects of such phenomena as attenuation differences or
saturation of recording media in subsequent parts of the system. It is the mirror of pre-
emphasis, and the whole system is called emphasis. The frequency curve (response) is
decided by special time constants, from which one can calculate the cutoff frequency.
It may be recalled that 7 MHz bandwidth is provided in band 3in VHF range. At these
frequencies, propagation takes place by space waves limited by maximum line of sight
distance between transmitting and receiving aerials. The signal strength at any place in
the service area must be large enough to overcome noise at that place and provide
satisfactory picture. The radiated power of transmitter is usually expressed as effective
isotropic radiated power (EIRP). In a TV transmitter, amplitude modulation of picture
carrier by video signal can be carried out at high level or a low level modulation.
In early transmitter designs, direct modulation was used. The picture was directly
modulated by video signal. This can be done at a high level modulation in final power
amplifier or at low level RF driving amplifier. At present, I.F modulation at low level is
used.
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T.5.1 TECHNICAL SPECIFICATION OF THE EXCITER
1 TV STANDARD CCIR B/G PAL 625
2 FREQUENCY470 – 860 MHz (BAND-IV/V)
channel selected according to site requirement
3 MODULATION
3.1 Vision NEGATIVE AM C3F
3.2 Aural FM F3E
3.3 Colour PAL B
4 VIDEO INPUT
4.1 Level 0.5V TO 1.5V p-p / 75 OHMS.
4.2 Return Loss -30 dB OR Better (0 TO 5 MHz)
5 CARRIER FREQUENCY
5.1 Vision Carrier Channel Frequency ±150 Hz
5.2 Aural Carrier Channel Frequency ±150 Hz
6 IF FREQUENCY
6.1 Vision IF 38.9 MHz ± 40 Hz.
6.2 Aural IF 33.4 MHz ± 40 Hz.
7 OUTPUT
7.1 Level 0 TO +10dBm
7.2 Aural to Vision Ratio 1 : 10 dB.
8INTER-MODULATION
DISTORTION-60 dBc OR Better
9 SPURIOUS
-5.5 MHz -55 dBc OR Better
+11 MHz -55 dBc OR Better
10OUTPUT STABILITY
(Peak Power)0.3 dB OR Better
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6. DRIVER UNIT
6.1 Driver unit:
The upconverted signal from the exciter is fed to an attenuator which is placed at the front
panel for adjusting the input level suitably the signal is amplified using class A driver stages.
The overall gain of the amplifier can be adjusted by the front panel attenuator control to be
about 33db such that 25/50W (sync peak) will be available at the output at driver unit.
The output of the amplifier is fed to a direction coupler where in samples of transmitted and
reflected power is obtained and fed to metering unit which detects the signal and suitable
voltage to a dc meter placed at the front panel.
The S portion switch on the front panel selects the parameter to be monitored
viz,vision,power,aural power & reflected power readings are to be read with black picture an
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ExciterDriver unit
Divider &
Combiner unit
Antenna
PA 1
PA 2
Block diagram of Driver Unit:
Video in
Audio in
Feed back signal
RF out RF out
RF out
RF out
RF in
RF in
ALC
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aural power indication is valid along with black picture only.A portion of the output power is
takeof the front panel if the driver unit for monitoring purposes.
The back panel output called ALC can be fed to exciter EXTALC is at rear panel to keep the
driver output constant.The availability of the output power “28v” to the unit is indicated
through a seen LED an the front panel.’DC Check’ facility in provided to moniter currents of
four stages of power amplifier by indicating a chord’ to ‘DC Check’ meter on
divider/combiner unit
Fig 6.1 driver unit
6.2 Divider and Combiner Unit:
This unit caters for three purposes:
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1)To divide the power from driver unit which is to be fed to two final power amplifier.
2)To combine the output power from the 50w power amplifier to obtain 100w sync peak
power and make available at antenna port.
3)To provide filtering for spurious sidebands using notch filters of frequency -5.5MHZ &
fs+5.5MHZ
Monitor unit detects the samples of forward and reflected power
from the power amplifier &feedssuitable DC voltage to front panel meter for monitoring
vision,reflected and aural power.the current/voltmeter and rotator switch provided at the top
front panel are used to monitorthe current drawn by various transistor stages of dividerunit and
power amplifier unit.
6.3 Power Amplifier Unit:
This unit comprises of two similar 50w power amplifier modules.RF power is fed to driver
unit and if divider into two signals and feed it to divider/combiner and then to each 50watt
power amplifier. Each power amplifier is fed with power input which is amplified to 50
watt(sync peak) by four class A parallel power amplifier stages with a gain at approximately
10dbm.This output is fed to a direction coupler to obtain samples of forward & reflected
power for monitoring purposes for the control unit. Thermistor serves the temperature at heat
assembly & provides DC voltage control.one green led is mount over the front panel to
indicate “normal” when FWD power reflected power & heat sink assembly temperature are
within satisfactory limits.where any of three red LEDs indication denotes the parameter
exceeds beyond the limits the control with cutsoff the transistor bias from bias assembly
placed in power amplifier unit, then tripping off the power amplifier.The system can be
restored back after rectifying the fault & restoring the indications in the front panel using the
push button switch ‘RESET’. Seperate power supply available for each power
amplifier(28V,20A) placed at bottom portion of chauin assembly.A DC voltage is
proportional to current drawn by each at the transistors in power amplifier is available from
bias unit on DC check connector placed over the front panel.
6.4 VSWR Measurement :
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After installing the antenna panel, junction box and U links it is verified whether the panels are
mounted as required. It is also verified if the correct lengths of branch feeder cables are used
for each face. The d.c resistance is measured by using a bridge connecting it between inner and
outer conductor of the U link or junction box. The d.c resistance is calculated as follows:
If R is the d.c resistance from U link or junction box
R = a + b + c + d + e milliohms
N
Where,
a = Antenna pannel ( about 5 mΩ )
b = Branch feeder cable ( depends on the cable size and length and is
measured separately)
c = Contact resistance of the junction box terminal, 1mΩ
d = Junction box, 1mΩ
e = U link
If the d.c resistance is very much higher than the calculated value it may
be due to bad contact of the branch feeder cable with the junction box or poor contact of other
matting surface. If the d.c resistance is higher than the nominal value, tap all the contact
portions with a rubber hammer observing the meter in measuring instrument. The meter needle
will kick back and forth while tapping the portion where the contact is poor and so the defect
will be rectified.
Measure the VSWR at the U link or junction box and by terminating the
other U link with 50Ω. Repeat the same procedure at the other U link input end. The VSWR
should be less than or equal to 1.05 at vision carrier frequency and 1.1 at other frequencies in
the channel. If VSWR is high it can be improved by slightly adjusting the pannels. Improper
fixing of branch feeder cables can also deteriorate the VSWR . A platform is provided at the U
link level ( JB level ) to keep the measuring instruments to perform tests.Thus VSWR
measurement is carried out at doordharshan.
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CONCLUSION
This report is a case study on the “100 watt low power
transmitter” that how the signals are receiving from the satellite ,their processing
and transmission in the terrestrial system.
The transmitter service involves the great equipment that deals
with monitoring section exciting system and we learn about the equipment of the
doordarshan center and its working
We learned about the procedure of transmission, reception and
strengthening of the signal and retransmitting the signal into the space for the
broad cast around the range of propagation.
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