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NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK, WEST VIRGINIA ELECTRONICS DIVISION INTERNAL REPORT No 167 ULO X4 MULTIPLIER BOB MAUZY AUGUST 1976 NUMBER OF COPIES: 150

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Page 1: NATIONAL RADIO ASTRONOMY OBSERVATORY · -a Gi-fi A wp. +32 +2.0 yi d ( I 1". 250-50 0 aNz o dam Power Di vicier 3 3 cl-13 yi Filter Coupler 3 dB Arnp. + 2-5 D-A COO verier Output

NATIONAL RADIO ASTRONOMY OBSERVATORY

GREEN BANK, WEST VIRGINIA

ELECTRONICS DIVISION INTERNAL REPORT No 167

ULO X4 MULTIPLIER

BOB MAUZY

AUGUST 1976

NUMBER OF COPIES: 150

Page 2: NATIONAL RADIO ASTRONOMY OBSERVATORY · -a Gi-fi A wp. +32 +2.0 yi d ( I 1". 250-50 0 aNz o dam Power Di vicier 3 3 cl-13 yi Filter Coupler 3 dB Arnp. + 2-5 D-A COO verier Output

ULO X4 MULTIPLIER

Bob Mauzy

General Description

The ULO X4 Multiplier unit along with a synthesizer, LO frequency control

unit and L-band counter make up the NRAO universal local oscillator (ULO) sys-

tem. The multiplier generates a high level 1 to 2 GHz signal from a synthe-

sizer output and from tuning information from the Local Oscillator Frequency

Control It replaces a manually tuned multiplier permitting complete

frequency control by the computer. The unit contains a 1 watt transistor out-

put amplifier and power supplies in a 5 1/4 inch high rack mounted drawer. See

Figures 1 and 2.

The multiplier unit is a relatively simple assembly with a minimum of

manual controls. It receives a signal in the 250 to 500 MHz range at a 0 dBm

level from the H-P 5105A synthesizer. The Input Level is set by the output

level knob on the synthesizer for mid-scale (100%) on the input level meter.

Control of the synthesizer frequency must come from the LO Frequency Control

unit rather than the local keyboard (Frequency Selection switch in Remote) be-

cause frequency information for multiplier tuning is received from the frequency

control unit.

Multiplier output level is controlled by a multiturn pot and monitored on

a calibrated meter. A calibrated limit switch,concentric with the level con-

trol,permits setting an upper limit on power output for protection of the de-

vices being driven. This feature is most needed when using the remote leveling

mode. In this mode a nominal 5 V level, indicative of the desired drive level,

is generated by the mixer or multiplier being driven. This feedback voltage is

1/ "Computer Control of the Universal Local Oscillator," EDIR No. 144.

Page 3: NATIONAL RADIO ASTRONOMY OBSERVATORY · -a Gi-fi A wp. +32 +2.0 yi d ( I 1". 250-50 0 aNz o dam Power Di vicier 3 3 cl-13 yi Filter Coupler 3 dB Arnp. + 2-5 D-A COO verier Output

returned to the remote level jack on the back panel to control an attenuator

and provide the proper output level. If the feedback cable should be discon-

nected or power removed from the unit being driven, a properly set limit level

will prevent excessive power from being fed to the following unit.

Referring to the block diagram, Figure 3, the major components used are

as follows:

Input power divider and detector - NRAO resistive splitterand BD7 detector.

Amplifier, 250-500 MHz - Microwave Power Devices LLD-055.

Multiplier - Anzac D-6-4 doubler or NRAO equivalent.

Yig filter - Aertech L3001.

Amplifier, 1-2 GHz Avantek AMM2000M.

Coupler, 3 dB - Narda hybrid 4132B.

PIN Attenuator - Anaren 60365.

Power Amplifier - Microwave Power Devices, LWA 1020-1.

Coupler, 10 dB - Norsal 4511-10.

Detector - H-P 423A.

Isolator - Wavecom 137-0150.

D-to-A Converter

The D-to-A converter card receives 4 digit BCD TTL frequency data from

the LO Frequency Control unit. The conversion is made by a Datel module. See

Figures 4 and 5. The converter module output feeds an op amp driver and level

shifter. The converter range is 0-9999 while the usable range in this applica-

tion is 2500 to 4999. Op amps Al and A2 provide the offset and gain required

to convert the module output current of 0.31 to 0.62 mA to 0-10 V drive for the

yig driver input. Amplifiers A3 and A4 detect the voltage limits, provide a

Page 4: NATIONAL RADIO ASTRONOMY OBSERVATORY · -a Gi-fi A wp. +32 +2.0 yi d ( I 1". 250-50 0 aNz o dam Power Di vicier 3 3 cl-13 yi Filter Coupler 3 dB Arnp. + 2-5 D-A COO verier Output

3

feedback clamping current and furnish a limit signal to the Frequency Limit

light driver. A small negative output is provided to extend the range a mini-

mum of 20 MHz below 1000 MHz to permit some overlap.

The adjustment procedure for the three trim pots is as follows:

Remove op amps Al and A3.

Set the digital input command to 500.0.

Short the D-A converter output through a low impedancemilliammeter.

Adjust the D-A gain pot (500 ohms) for 0.62 mA.

Remove the meter.

Replace op amp Al.

Set the input command to 250.2.

Adjust the offset pot (2 K ohms) for 8 mV output to yigdriver.

Set the input command to 500.0.

Adjust the gain pot (200 ohms) for 10.000 V output.

Check output for 250.2 input setting.

Replace op amp A3.

Yig Driver

The yig driver unit converts a 0 to 10 V input into the current required

by the yig filter to tune 1 to 2 GHz. See Figure 6. The zero control is set

for 1 GHz center frequency with no input and the slope control for 1.9 GHz with

9 V in. This unit was designed by Craig Moore for use in other systems prior

to this application.

Leveler

The leveler card contains the circuits for internal and remote leveling,

level limits, level fail detectors with lamp driver, and the input detector

Page 5: NATIONAL RADIO ASTRONOMY OBSERVATORY · -a Gi-fi A wp. +32 +2.0 yi d ( I 1". 250-50 0 aNz o dam Power Di vicier 3 3 cl-13 yi Filter Coupler 3 dB Arnp. + 2-5 D-A COO verier Output

amplifier. See Figures 7 and 8. Op amp Al amplifies the internal output de-

tector and feeds A4 and A5 for local leveling. The main integrator is A5. A4

is the limit level integrator which captures control of the loop if the output

level exceeds the limit setting in either remote or local operation. Ampli-

fiers A6 and A7 detect errors between the input signal voltage and the refer-

ence voltage determined by the output level control. If these voltages are not

essentially equal, the unit is not leveling properly and the level fail circuit

is energized. A8 is a switched oscillator to provide a blinking Level Fail

light.

Performance and Brief Comments

Three of these units have been in use for several months without any prob-

lems. A problem is expected when an application allows the unwanted harmonics

at 3 and 5 times the input frequency to be within the signal band. These com-

ponents are greater than 60 dB down. An external filter will be added to give

further suppression. Should the spurious signals become a frequent aggrava-

tion, another yig filter, driver, and other components can be mounted in the

drawer in the space provided.

A phase stability vs. temperature check was made using a synthesizer as a

driver. The results indicated that synthesizer drift was much worse than the

multiplier.

Two of the three systems contain NRAO built doublers in place of the An-

zac D-6-4. The manufacturer was unable to build satisfactory units at that

time, so we developed our own.

The output coupler, detector and the operating level of the detector were

chosen to provide a reasonably accurate calibration of output power over a 17

dB range and with little variation with frequency.

Much of the ordering, breadboarding, construction, and testing of these

units was done by Lewis Beale.

Page 6: NATIONAL RADIO ASTRONOMY OBSERVATORY · -a Gi-fi A wp. +32 +2.0 yi d ( I 1". 250-50 0 aNz o dam Power Di vicier 3 3 cl-13 yi Filter Coupler 3 dB Arnp. + 2-5 D-A COO verier Output

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Page 13: NATIONAL RADIO ASTRONOMY OBSERVATORY · -a Gi-fi A wp. +32 +2.0 yi d ( I 1". 250-50 0 aNz o dam Power Di vicier 3 3 cl-13 yi Filter Coupler 3 dB Arnp. + 2-5 D-A COO verier Output

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