80
- , ELECTRONICS IMPLEMENTATION _.. OF THE SOLAR NEUTRON EXPERIMENT DECEMBER 1970 Stephen White . - ' ,; NASA Grant NGR-05-008-0 22 and DOD Support - W00014-69-A-0200-5001 .' \ ... CASE.FIte C /-\ D V V) f I - . r LU EDUCATION RESEARCH SERVICE O •73 RIVERSIDE f £ The Institute of Geophysics and Planet""" ™~>~ . Universitv of I Geophysics and Planetary Physics, . University of California, Riverside, California 92502 https://ntrs.nasa.gov/search.jsp?R=19720016206 2020-04-07T12:32:29+00:00Z

CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

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Page 1: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

- •

, ELECTRONICS IMPLEMENTATION

_..OF THE

SOLAR NEUTRON EXPERIMENTDECEMBER 1970

Stephen White

. -

• ',;

NASA Grant NGR-05-008-0 22and DOD Support - W00014-69-A-0200-5001

.'

•\...

CASE.FIteC /-\ D VV) f I

-

.

r

LU

EDUCATIONRESEARCH

SERVICE

O•73

RIVERSIDE

f £

The Institute ofGeophysics and Planet""" ™~>~ —

.Universitv of

•I

Geophysics and Planetary Physics,• .

University of California,Riverside, California 92502

https://ntrs.nasa.gov/search.jsp?R=19720016206 2020-04-07T12:32:29+00:00Z

Page 2: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

;- -

ELECTRONICS IMPLEMENTATIONOF THE

SOLAR NEUTRON EXPERIMENT'•'

DECEMBER 1970- .

-

'- ••

Wayne A. MillardGeorge M. Simnett

Stephen White

- ••*,. - - - - « - • ' , . -

.| '

. .. '-

. --

-•/.,- • -. ••</.-. - - •"

. ' EDUCATIONRESEARCH

SERVICE

RIVERSIDE* • ••••••

Institute ofPhysics,

California,• •. .Riverside, California 92502.

-

Page 3: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

ELECTRONICS IMPLEMENTATION

OF THE

SOLAR NEUTRON EXPERIMENT

December 1970

Wayne A. Millard

George M. Simnett

R. Stephen White

Institute of Geophysics

and

Planetary Physics

University of California, Riverside

Page 4: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

TABLE OF CONTENTS

Page

1. Introduction 1

2. S.. , S Adder Boards 1

3. S,/S Discriminator Board 8J. &

4. A , A_ Discriminator Boards 14

5. Decision Logic Board 19

6. Pulse Height Analysis Board 23

7. Buffer Memory Logic 27

8. Time-of-Flight Board 30

9. Data Encoder Board 34

10. Azimuth Detector Board 42

11. Temperature Monitor Board 45

12. Logic Events Board 46

13. Power Conditioning 55

14. Bit Synchronizer 55

15. Data Decoder 58

16. Acknowledgments 73

Page 5: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

FIGURES

Figure

1. Overall System Block Diagram

2. S Adder Board Schematic

3. S Adder Board Photo

4. S Adder Board Schematic

5. S Adder Board Photo

6. S /S- Discriminator Board Schematic

7. 8ero Walk Circuit Schematic

8. S /Sp Discriminator Board Photo

9. A Discriminator Board Schematic

10. A Discriminator Board Photo

11. A_ Discriminator Board Schematic

12. A Discriminator Board Photo

13. Decision Logic Board Schematic

14. Decision Logic Board Photo

15. Pulse Height Analysis Board Schematic

16. Pulse Height Analysis Board Photo

17. Buffer Memory Logic Board Schematic

18. Buffer Memory Logic Board Photo

19. Time of Flight Board Schematic

20. Time of Flight Board Photo

21. Data Encoder Board Schematic (Clock, SyncPattern Generator, Control)

22. Data Encoder Board Schematic (Shift Register Section)

Page 6: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

23. Data Encoder Board Photo

24. Azimuth Detector Board Schematic

25. Azimuth Detector Board Photd

26. Temperature Monitor Circuit Schematic

27. Logic Events Board Schematic

28. Bit Synchronizer Circuit Schematic

29. Data Decoder - Main Counting Unit

30. Data Decoder - Sync Board

31. Data Decoder - Error Counters

32. Data Decoder - Data Control Board

33. Data Decoder - Event Interrogator & Transfer Timer

34. Data Decoder - Data Board

35. Data Decoder Photo, Front View

36. Data Decoder Photo, Rear View

Page 7: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

1 . IntrQduction

This report describes the functioning of the electronics

used in the neutron counter experiment. The overall system

block diagram (Fig. 1) shows the electronics assembled on

various boards. On the pages that follow the boards will be

discussed individually.

Functional block diagrams have been omitted from this

report as they appear in Section 1.1 Experiment 1 of the

Themis Renewal Proposal, December 14, 1970. That proposal

gives an overall functional electronics description of the

experiment while the operating details are given here.

2. S,, S Adder Boards

The S, and S2 Adder Boards that are connected to the S,

and S? photomultiplier tube outputs (16 total), perform three

main functions: (1) linear, passive addition of the photo-

multiplier tube outputs, (2) singles rate monitoring and

(3) scintillation cell identification. A brief description

of each follows. See Figs. 2 to 5.

A. Adders. Passive adders were selected to satisfy the

requirements of a large linear dynamic range of 100:1,

isolation greater than 100:1 and fast pulse rise time.

Signals are added two at a time, with hybrid transmission

line transformers. They are constructed from very high

permeability ( p. = 5000) ferrite cores on which are wound

the parallel wire transmission lines twisted in bifilar

Page 8: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

InputsSIScintillate''Tank

trorfl r —

from f —InputsS2 (8)ScintillatorTank

InputsA IScintillotorSheets

Inputs fromA 2ScintillotorSheets

from I —

Fig. 1. Overall System Block Diagram

Page 9: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

6 CONT^x TC52 ABOER

17 SINO.ES RATETO Wa ENCOOSH

19 SINOLES 10TO 0/U« ENCODES

2 SINCi-ES INPUTFROM S2 AOOER

ANGLE STROMFROAt 01.6

a)Approximate impedance value. Selected for optimum isolation.b)All adder transformers wound on Ferronics 11-620-B ferrite cores.

Fig. 2. Adder Board Schematic

Page 10: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 3. S Adder Board

Page 11: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

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Page 12: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 5. S2 Adder Board

Page 13: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

arrangements. Each adder section consists of an unbalanced

to balanced transformer, an adder transformer and a matching

or balancing load impedance to achieve the required isolation.

Once balanced, isolation between inputs exceeds 40 dB when

driving the adder with simulated PM tube pulses (2-3

nanosecond rise time, 10-20 nanosecond fall time).

B. Singles Rate Experiment. Each PM tube input is

connected to a threshold circuit discriminator to prevent

unwanted noise from triggering the following electronics.

High speed core-memory sense amplifiers with adjustable

thresholds and strobe inputs in integrated form (MC 1543L)

are used. After discrimination, the pulses are all normalized

to a fixed amplitude (Emitter Coupled Logic) and then

normalized to a fixed width in one-shot circuits composed of

interconnecting two OR/NOR gates. The signals are translated

to Transister Transister Logic, and applied to a data

selector that acts as a single pole, eight position switch

whose position is determined by binary logic.

With the data selector in some arbitrary position,

scintillator pulses corresponding to that position are fed

into a 12 stage,4096 count, register. When the register is

full, the data selector is stepped to the next position by

using a four stage counter to produce the control logic.

The photomultiplier singles rate is determined by the

length of time required for the register to fill and its

identification by noting when the control counter is full.

Page 14: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

The S and S2 adder boards each has its own data selector,

but the common counter and control logic counter is located

on the S adder board.

C. Scintillation Cell Identification (Angle Information)

Much of the electronics used for the singles rate is also

used for the cell scintillator identification (discriminator,

one-shot and translator). After the translator, each signal

is applied to a shift register (MC4012). The state of the

shift register's input is stored by applying a strobe pulse

to the shift register. This strobe pulse is generated by the

output of the signal gates on the decision logic board, and

thus is present for neutron events. The strobe pulse for the

S, and S~ PM tubes is derived from the S, and S,., signal gates,

respectively. The outputs of the shift registers are fed

to the data encoder.

3. si/S2 Discriminator Board

After the photomultiplier tube outputs of S and S,., have

each been added on their respective adder boards, the added

output lines are routed to the S,/S~ Discrimination Board.

The summed output signals: (1) are fed to a pulse height

analysis board, (2) generate pulse signals with the proper

width and delay for use in the logic events or particle events

circuit and (3) precise timing signals for use in measuring

the time of flight of neutrons and in gating the signal or

anticoincidence gates. Fig. 6 is schematic of the board.

8

Page 15: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

A. Pulse Height Analysis. The added incoming signals

are simply fed out again to a coaxial delay line to provide

sufficient delay (approximately 50 nanoseconds) so that a

gating signal can be generated to record the signal pulse.

B. Logic Events Pulses. Each summed input is applied to

a threshold or noise discriminator (MC1543L) and then the

proper delay and width are obtained by using cascaded one-shot

multivibrators using interconnected OR/NOR gates for the

one-shot. The outputs are fed to the logic events board using

twisted wire pairs.

C. Timing Signal Generation. To obtain accurate time-

of-flight results, timing pulses must be generated which have

fast response times (one nanosecond rise and fall times) and

are input amplitude insensitive, i.e. the time delay through

the timing generator must not be sensitive to the summed

analog input signal. This requirement can also be stated as

a need for "zero-walk" performance. The zero-walk circuit

operates on the summed signals as follows. (See schematic,

Fig. 7 and photo Fig. 8).

The heart of the zero-walk circuit is the charge storage

or step recovery diode. It has the property that when driven

from forward conducting to reversed biased the diode continues

to conduct in the reverse direction until the charge stored in

the diode during its forward biased period is removed. Then,

within a hundred picoseconds or ;so the diode "snaps" off to

a nonconduction state. Therefore by removing charge

10

Page 16: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 8. S Discriminator Board

Page 17: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

proportional to the rate of adding charge, both of which are

dependent on the input signal amplitude, this step recovery

always occurs at the same time with respect to an amplitude

varying input.

In order to cover the large dynamic range of the input

signals (25 mV to 6 volts), amplification of the low level

signals is needed to operate the timing generators. Four

fast amplifier stages are used which amplify and shape the

pulses, with limiting occuring to reduce the dynamic range

of signals applied to the step recovery diode. The diode

first receives a negative signal and starts conducting. Then

through inverting transformer Tl, the signal is delayed and

inverted, and removes charge from the diode until it "snaps"

back to a non-conduction state.

Overall, in spite of some slight timing errors introduced

by the amplifier circuits, the timing accuracy is within 0.5

nanosecond for the dynamic range of 25 mV to 6 volts (a 240

to 1 range).

The output of the zero walk circuit is applied to a

threshold discriminator which is used as a controlled gate and

logic translator. A fast, short, one-shot (MC1660) of ten

nanoseconds follows and is used as the "fast" input to the

signal gate.

Since the zero walk does not provide noise discrimination,

a parallel discriminator circuit, using an MC1543L along with

a MC1660 OR/NOR one-shot, generates an "enable" signal for

use with the signal gates.

13

Page 18: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

4. A , A~ Discriminator Boards

The A and A2 Discriminator Boards receive photomultiplier

tube outputs from the anticoincidence scintillator sheets

around S, and S2> A schematic of both is seen in Figs. 9

and 11 and photos in Figs. 10 and 12.

The two PM tube outputs from the upper most sheet of

both scintillators are added together and the resulting signal

is used four ways. It is fed directly through a coax connector

to a coaxial delay line and then is pulse height analyzed.

It is used to generate logic event signals (by being level

discriminated, delayed and stretched) . Also high-53

discrimination takes place using a 40:1 resistive attenuator

ahead of a discriminator. This high-2 channel signal is used

for logic event signals and to enable the signal or anti-

coincidence gates. Finally, the input signal is also added

with the side and bottom scintillator PM tube outputs. This

addition is accomplished using the passive adders described

in the S.. and S~ adder section.

The PM tube outputs from the side and bottom sheets like-

wise are added to each other and used to generate logic event

pulses. The four event pulses, A _, A13/ A22 and A are

used with the high-2 experiment and are routed to the decision

logic board where their state is observed by the outputs of

the signal gates.

The added signal from all the anticoincidence sheets of

either A, or A2 is discriminated and used for logic events and

for an anticoincidence pulse to the signal gates.

14

Page 19: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Page Intentionally Left Blank

Page 20: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

INt'lll Imm

All I'M I IMII '.ll'll'l

To OLB

AIS-2,5,6.7.8TWi»l«d Pr.To Logic Eventt . ,.

Fig. 9. A-, Discriminator Board Schematic

Page 21: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 10. A Discriminator Board

Page 22: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

INPUT Irow •»81 PM TUBES

(TOP-INSIDE)

To OL8

A 2 - 4T.l.l.d PrTo Logic Evtnli

A23-2.S.7.8 1TWi.t.d Pr. •To Logic E««nlt \tt<*£—<

Fig. 11. A2 Discriminator Board Schematic

Page 23: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 12. A_ Discriminator Board

Page 24: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

5. Decision Logic Board

The Decision Logic Board serves many purposes. It

contains the:

a. signal or anticoincidence gates

b. event counter

c. Ai?' Ai3' A22 and A24 event registers

It also generates:

d. "Start" and "stop" signals for the Time-of-Flight Board

e. mode (solar, albedo, high-3 ) and calibrate logic

f. PHA gate enable pulses

g. strobe signals for the scintillator cellidentification

i. control logic for the logic events data selector

j. the 40:1 PHA attenuator drive signal

"k. reset signals for the PHA and time of flightregisters

1. reset signals for the FET switches in the PHA's

m. a 300 microsecond "processing event" signal forthe data encoder (W line).

The signal lines (Fig. 13,14) from the S-,/S discriminator

board and the A., and A discriminator board are applied to

the fast signal gates of IC2. These are 1 nanosecond MECL

III, the fastest presently available logic. The outputs of

the signal gates go to the 140 nanosecond pulse stretchers

(IC3, 4, used as one shots) and also to mode control gates

(IC5, 6). These gates route the signals coming from the

19

Page 25: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

LOGIC EVENTS BOARD

P. R FROMDATA ENCODER

i ' iFRAME RATE)

TO DATAENCODCR" MODi " 40:1 ATTENUATOR DRIVE

TO SI AND S2 PHABZ5

MODE LOGIC TO DATA T,, . nr.ir FVFMTSTO A, AND AZ ENCOOtR . IS. £2° ° EVE S

DISC. BOARD -UP/ I BOARD' * DOWN" >BIO BIZ A6 AIOAI2

t romAI <rorrA?

DISC.Board DISC. Booio

Fig. 13. Decision Logic Board Schematic

Page 26: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 14. Decision Logic Board

Page 27: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

signal gates using logic generated in 117, 19 to gates 17,

which produce the "start" and "stop" pulses for the time-

of-flight circuitry.

If a stop signal is generated this indicates that a valid

event has occurred and a 10 microsecond one-shot (18) triggers

and operates the event counter (114, 15, 16), a 0.5 micro-

second one-shot (122) for quickly reseting the PHA and time-

of-flight registers, the 300 microsecond "processing event"

one-shot (123), starts the PHA circuitry operating and

disenables the signal discriminators on the S /S discriminator

board thru 113 and II. The signal discriminators continue to

be held off past the initial 10 microseconds by the "X" line

from the data encoder. This line logically says that a

signal is being processed or has been processed but not

transferred yet to the shift registers of the data encoder.

The PHA holding capacitors are reset to zero both after

an invalid event has occurred and after the buffer registers

have been read out following a valid event via the "X" line.

This is accomplished by gate II, the 1 microsecond one-shot

19, and some transistor level shifting circuits. The A ,

A _, A „, and A«- flip flops are simultaneously reset.

If the system is in the "solar" mode, the S signal gate

will be enabled to receive a pulse but the S,, signal gate is

blocked by feedback from 15. Only after the S signal gate

receives a valid signal is the S signal gate allowed to

operate, and then only for a period of 140 nanoseconds. If

22

Page 28: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

the particle does not interact in scintillator S_, no "stop"

pulse is generated and the system is reset as noted above.

The mode logic discussed earlier is also connected to a

two transistor drive circuit for the 40:1 attenuator. A

calibration logic signal is generated for every 128 events, so

the first 7 lines from the event counter are connected to

NAND gate (118). This calibrate signal along with the mode

logic operates some ECL to produce control logic for the A,

and A discriminator boards.

Strobing signals for the scintillation cell identification

(angle) registers are obtained by delaying and translating

the outputs of the 140 nanosecond one-shots connected to the

signal gates. It is the negative going strobe signal which

reads the cell identification information into the registers

on the S1 and S2 adder boards.

6. Pulse Height Analysis Boards

The purpose of the pulse height analyzer is to convert

amplitude of the PM tube pulses to pulses whose time duration

is proportional to input pulse amplitude. This output pulse

is connected to a clock which sends pulses at a fixed rate

into a counter. Thus the larger the PM tube pulse, the longer

the pulse duration from the analyzer board and the longer the

time the clock sends pulses to the counter. The overall result

is an A/D converter whose counter output is a binary code

representation of the input pulse amplitude. (The clock and

counter are located on the Buffer Memory Logic board).

23

Page 29: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

The circuitry (Fig. 15, 16) consists of a fast current

amplifier (Q7, Qll) that stores a charge on the 9 pF

capacitor following diode D8 proportional to the input

amplitude. Constant current sources (Q4-Q6, Q8-Q10 and

Q16-Q20) place the current amplifiers in an initial conducting

state and establish the maximum current swing possible.

A fast shunt attenuator, used as a signal gate, is

composed of differential amplifiers Q14, 15 and Q12, 13

which switch shunt diode D4 on or off. The gate input drive

originates on the decision logic board, and is derived from

the output of the appropriate anticoincidence gate.

An FET input buffer (Q22-27) follows the holding

capacitor and drives the amplitude to time converter. This

A/T converter consists of a high gain differential amplifier

(Q29-32) with a diode (D14) in the feedback loop. The

circuit is used in a sample and hold arrangement by placing

a 2700 pF capacitor at the output of the amplifier, after

diode D14. Thus the loop has a closed loop gain of unity and

for negative signals the capacitor voltage follows the input.

When the input goes positive, the diode reverse biases opening

the loop and holding the peak voltage on the capacitor.

Shunt FET switches across the capacitor and the 9 pF unit

in the stretcher section are used to reset the capacitor

voltages to zero following an invalid event (a neutron going

through S, but not S~, for example).

A constant current source (Q34) is switched on 10 micro-

seconds after the input signals by a signal applied to the

24

Page 30: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

40:1 ATTENUATORFOR S1/S2

"'

rini 1 ••-* )OR.I VE I

Fig. 15. Pulse Height Analysis Board Schematic

Page 31: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 16. Pulse Height Analysis Board

Page 32: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

PHA trigger input. This signal is a pulse 300 microseconds

wide and is derived on the Buffer Memory Logic Board. The

current flow to the capacitor develops a linear (fixed slope)

voltage ramp bringing the capacitor voltage back to zero.

When close to zero, diode D14 begins conducting again and the

loop once more closes.

Shaping amplifier (Q35-38) monitors the time that the

amplifier loop is open and presents a gating signal output

with a width directly proportional to the input PM tube pulse

amplitude.

The S and S PHA are used both in the neutron mode and

the high-2 mode. Therefore an attenuator must be employed

prior to the PHA when in the high-2 mode to stay in the linear

operating range of the PHA. This attenuator consists of a

resistive attenuator switched in by transistors Q2, 3.

Transistor Ql lightly loads the attenuator and is used as a

buffer amplifier.

7. Buffer Memory Logic Board

The buffer memory logic board (see Fig. 17, 18) receives a

gating signal from each PHA board whose width is directly

proportional to the input PM tube amplitude. This gating

signal applied to a gate enables JK F/F MC7473, allows 2MHa

clock pulses from oscillator ICG and translator IC5 to be

fed into an 8-bit memory (MC7493). The 9-bit memory, that

includes the output state of the F/F, stores the pulse

amplitude in a binary form to be fed to the Data Encoder.

27

Page 33: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

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Page 34: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 18. Buffer Memory Logic Board

Page 35: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

This board also includes the 300 microsecond one-shot for

operating the current sources (through Ql,2) on the PHA boards

and the' input gates of IC2.

8. Time of Flight Board

The measurement of the time of flight of particles between

the top and bottom scintillator tanks is performed on the time

of flight board, Fig. 19,20. The technique is a time to voltage

to digital code conversion. In this case a voltage proportional

to the time of flight is generated, held and converted to a

digital output using an accurate double ramp conversion technique

Prior to an event occurrence, a constant current of 10

milliamperes, generated by the ICl, Q5, Q6 circuit, flows to

the junction of D2 and D3 (Dl is reverse biased) where it

splits equally with 5 milliamperes flowing through D4 (D5 is

reversed biased) to another precise constant current source

of 5 milliamperes formed by the IC2 and Q8 circuits. Since

the currents through D2 and D3 are equal, the initial voltage

across the sampling capacitors Cl, C2 is zero.

Diode Dl is switched into a conducting state when a

"start" pulse (generated in the decision logic board) appears

at the input. The 10 milliampere constant current is then

diverted through Dl and Ql, causing D2 to become reverse biased.

Since the 5 milliampere current is still being demanded, it

is supplied through the sampling capacitors, which thus begin

charging at a constant rate of IT/C volts per second, set at

about six millivolts per nanosecond.

30

Page 36: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

* '£* •. *fe -A.

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Fig. 19. Time-of-Flight Board Schematic

Page 37: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

» o a'„ s a'iJVii'uVi'.'i

Fig. 20. Time of Flight Board

Page 38: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

The voltage ramp across the sampling capacitors is

stopped when the "stop" pulse arrives and causes D5 to be

switched into conduction, so that diode D4 is reverse biased

and the 5 milliampere current is now supplied through Q7 and

D5.

The stored capacitor voltage is sensed by a unity gain

buffer amplifier consisting of Q9, a matched monolithic

dual-FET, and IC-3, used to bootstrap the source on the FET,

keeping the input current to less than ten picoamperes. This

buffered voltage is then amplified by IC-4, connected as a

gain of twenty balanced differential amplifier.

It is this amplified version of the capacitor voltage

which is now converted to binary form by the dual ramp A/D

converter circuit. It is carried out by comparing the

capacitor voltage with a stable reference voltage, developed

across reference diode D8. The comparison is performed by

two FET switches, Q10 and Qll that connect first the amplified

capacitor voltage and then the reference voltage to integrator

IC-5 at the correct time. The output of the integrator is

initially below ground, so the application of the capacitor

voltage (negative) causes the integrator output to be a

positive going ramp with a slope of V f/RC. Upon crossing

zero, the output causes comparator IC-6 to change state,

enabling gate Q10, 11 to pass clock pulses into the 8 bit

(256 count) register IC8, IC9.

With clock pulses coming at the fixed rate of 2 megabits

33

Page 39: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

per second, and a register capacity of 256, the register is

filled after 128 microseconds. It then toggles flip flop

IClO that drives the transistor circuit Q13, Q14, Q15 to

switch the integrator from the time of flight voltage over

to the reference voltage.

The reference voltage is of the opposite polarity

(positive) with respect to the time of flight voltage, so

the integrator output is now a ramp going negative with a

fixed slope of V f/RC. Concurrent with the time the

switching changes, the register also clears itself to zero

and continues counting. The counting continues until the

integrator output again crosses zero, at which time the

register is inhibited. The stored count is now directly

proportional to the value of the integrator output at the

time when the switchover takes place and hence to the time-

of-flight.

Operation of the circuit has been very good and initial

tests have indicated a time resolution on the order of a

quarter of a nanosecond. Faster clock speeds could imporve

on this if system requirements demanded better resolution.

9. Data Encoder

The Data Encoder consists of a clock generator, a

synchronization pattern generator, a control section and a

96 bit memory in the form of shift registers. See Figs. 21, 22, 23.

The clock section (Fig. 21) begins with a 100 kHe

transistor oscillator which is divided by four in a dual

34

Page 40: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

ENCODER

SYNCHRONIZATION PATTERNGENERATOR

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Fig. 21. Data Encoder Board Schematic (Clock, SyncPattern Generator, Control)

Page 41: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

ENCODER

SHIFT REGISTER SECTION

ALL 1C ARE SN 7496

Fig. 22. Data Encoder Board Schematic (Shift Register Section)

Page 42: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

I

Fig. 23. Data Encoder Board

Page 43: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

JK flip flop (MC7473). The output of the first stage provides

a 50 kl-la bus and the Q and Q outputs of the second stage are

defined as the 0 and 180 phases of the 25 kHe clock.

Applying the 180 clock line to the D input of a type D

flip flop (MC7479) with the 50 kHa line on the clock input,

the Q and Q outputs become the 90 and 180 phases of the

clock.

The synchronization pattern generator is composed of two

16 input data selectors (SN74150), their inputs preset to

logical "1" or "0" according to the desired synchronization

pattern format. The 0° clock (25kHa) is divided in a 4-bit

counter (MC7493) to supply the four control lines to the

data selectors. A following JK flip flop (MC7473) provides

Q and Q outputs which strobe on the data selectors alternately

for sync bits 1-16 and 17-32. The sync pattern is shown on

the following page along with the data bit allocations.

The outputs of the data selectors are gated with P and

R signals (derived by division of the clock) in a NAND gate

(MC7420). The output of the NAND gate is then clocked

through a D flip flop with the 180 clock phase and becomes

the synchronization pattern, L, which is combined with the

data bit stream from the shift register memories in a MC7451

to form the composite data frame, 32 bits of sync and 96

bits of data.

The control section governs the transfer of data from

the buffer registers (on the various boards) to the shift

38

Page 44: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Encoder Bit Allocation

Bits PositionSynchronization Pattern

Mode (Solar, albedo, high 2)

Event Counter

Upper Scintillator I. D. (Angle)

Lower Scintillator I. D. (Angle)

PHA SI

PHA S2

PHA Al

PHA A2

A13 event

A12 event

A23 event

A22 event

Time of Flight SI to S2

Singles Rate

I.D.

Temperature Data

I.D.

Azimuthal Data

I.D.

Logic Events

Available for future use

32

2

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9

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1

1

1

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Synchronization pattern: 01010110101001011010011010101111

Page 45: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

register, clocks out the data at the correct time, resets

the buffer registers and controls the acquisition of new

data. The main control lines are the P and R signals, as

the logical OR1ing of these lines is coincident with the sync

and data periods of a frame. The shift registers are clocked

out by a signal derived from a dual AND~OR-INVERT gate

(MC7451). The 0° phase clock is used and this is inhibited

for the duration of "1" (the sync period). Two gates are

used because of fan-out limitations of one gate.

Data from the buffer registers are normally transferred

to the shift register at the beginning of the sync period.

However, if an event is being processed at this time the

shift should not take place. The decision is implemented

by logic line W from the decision logic board , a logic "1"

indicating no event is being processed. This W signal along

with P • R ("1" during sync period), D (one half the clock

rate) and the output of a D flip flop (MC7479) are applied to

a 4-Input NAND gate. The flip flop's purpose is to prevent

more than one preset pulse during each frame. The clock

input to the flip flop is from a NAND gate (MC7420) whose

inputs are p • R and the Q output of the flip flop. When the

conditions for preset are satisfied, a 100 nanosecond one-shot

(MC8601) is triggered to provide Y signal or "buffer clear."

It also changes the state of the D flip flop used to inhibit

further preset pulses. At the end of the synchronization

period, the D flip flop is reset as the P-R signal goes to "0"

40

Page 46: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

The preset signal is fed into a buffer (one half a quad

NOR gate, MC7402) to provide the power to preset 96 bits in

the shift register. This signal along with W and the output

of a JK flip flop go to a NAND gate (MC7420), whose output

is X, a signal used to control the acquisition of new data by

controlling the discriminator strobe inputs (S,/S_ discriminator

board) and gates on the decision logic board. The JK flip

flop is used to inhibit acquisition of new data until after

the buffer registers have been read out for an event that

occurs during the data period of the frame. This is done

by clocking (25 kHB 0° clock) the state of W to the output

of the flip flop, where the signal is summed with P + R ("1"

during data period). The summed signal is used to hold the

flip flop until the beginning of the next sync period.

The data bit stream for the shift register is combined

with the sync bit stream in an AND-OR-INVERT gate (MC7451)

to form the composite frame.

The following outputs are used or available for use in

other parts of the electronics:

R: FrJime rate for commutation

p-R: Logic Events Control

Y: Reset buffers

X: Control Signal Gates

50 kHa clock

Four phases of 25 kHe clock

41

Page 47: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

10. Azimuth Detector Board

The purpose of the azimuth detector is to determine the

azimuth angle between the S, , S~ scintillators and the sun.

This is accomplished by mounting phototransistors (32) on

the periphery of the gondola that look out toward the horizon

with large vertical acceptance angles. The outputs of the

phototransistors, compared two at a time, then indicate the

sun's position relative to the gondola. See Fig. 24, 25.

A clock line from the Data Encoder at the data frame rate

is applied to two decade counters (CD4017D), a "units" and

a "tens" counter. Following the 32nd clock pulse, a signal

appears at the "3" output of the tens counter and the "2"

output of the units counter. These are AND'ed together

(CD4019D) and used to reset all the shift registers and the

D flip flop. The next clock pulse (33rd) causes an output

from the "33" AND gate, setting a logical "1" in the first

bin of the "odd" bits bank of shift registers (CD4015D).

This turns on the analog switch (CD4016D) associated with

phototransistor #1. Likewise the 34th clock pulse enters a

logical "1" into the "even" bits bank of shift registers

("odd" and "even" here referring to the labeling of the photo-

transistors .)

Hence with a "1" present in the first bin of both sets

of shift registers, phototransistors #1 and #2 are connected

through the analog switches to a differential comparator

(MA710). It's output is a "1" or "0" depending on the

relative amplitudes of the two input signals which are

42

Page 48: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

0X0110SHIFT RtCISTEB

CD40I70OfCADC

COUNTER

Fig. 24. Azimuth Detector Board Schematic

Page 49: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

, .-. A. jfezUSfc*1!-*

Fig. 25. Azimuthal Detector Board

Page 50: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

proporLional to the intensity of the light striking the

phototransistors.

The 35th clock pulse causes an output from the "35"

AND gate which resets both decade counters to zero. As

clock pulses continue, the D flip flop alternately clocks

the "even" and "odd" shift registers, and hence commutates

through the 32 phototransistors. Phototransistors 1 and 2

are compared with the 34th clock pulse, 3 and 2 with the 35th

pulse, 3 and 4 with the 1st clock and so on. Therefore a

comparison of all 32 phototransistors is made, each frame

indicating the comparison of another two. Examination of the

differential comparator along with an identification signal

thus provides the information on the relative amplitudes of

the two input signals and the intensity of the light striking

the phototransistors.

The 35th clock pulse causes an output from the "35" AND

gate which resets both decade counters to zero. As clock

pulses continue, the D flip flop alternately clocks the "even"

and "odd" shift registers, and hence commutates the 32

phototransistors.

11. Temperature Monitor Board

The temperature monitor board measures the temperature at

various selected locations in the experiment package to aid

in data analysis. Temperatures to be monitored include the

inside and outside of the gondola, the S.. and S« scintillator

tanks, batteries and various places in the electronics.

45

Page 51: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

The monitor is basically a temperature dependent oscillator

whose frequency is measured. See Fig. 26. The oscillator is

a multivibrator that has thermistors switched sequentially into

one of the collector loads. The resistance of the thermistor

controls the charging rate of the timing capacitor and thus

the period of the multivibrator.

The frequency is counted by a 12 bit counter (3-MC7493).

After the counter is full (4096 counts), the output, after being

translated to MOS logic levels, clocks a decade counter (CD4017D)

one position. The outputs of the decade counter are connected

to analog switches that place each thermistor in turn into

the multivibrator circuit.

With the output of the binary counter connected to a bit

in the data encoder shift register, the states of the last

bit in the counter are observed. The time for the bit to go

from "0" to "1" to "0" (4096 counts) gives the frequency

(f=4096/time). Reference to a calibration curve of frequency

vs. temperature provides the desired result.

12. Logic Events Board

Eight different counting rates are monitored sequentially

by the system electronics, and are referred to as the logic

rates. These counting rates are defined in the Table I,

where the rate number, the detector logic and type of particle

are given. A refers to the anticoincidence detector around

Slf A and A 2 refer to the top and bottom 45" x 41" sheets

of scintillator in A , and A 3 refers to the sum of the four

46

Page 52: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

MULTIVIBRATOR

OUTPUT

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TIED TO PT.

Fig. 26. Temperature Monitor Circuit Schematic

Page 53: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

TABLE I

Rate Detector Logic Type of Particle

C C22

Neutrons and v-rays

Sl A12 A13 A21 S2 A22 A23 Medium energycharged particles

Al SlY-rays

A2 S21Y-rays

Sl A12 A13 A21 S2 A22 A23Multiply chargedpenetrating particle:

Sl A12Low energy chargedparticles

Sl A12 A13 A21 A22 S2 A23Penetrating particles

8 Sl Al2 A21 S2 A22 A13 A23Electrons, downwardmoving

Sl A12 A21 S2 A22 A13 A23 S2Penetrating particles,upward moving

48

Page 54: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

curved sheets of A (sides). An identical notation identifies

the A_ components. S~/ S21 ' S'>-> anc' S2 re^er to tne s?

scintillator ,* the differences are in the delay and pulse width

of the logic signals derived from S- . Similarly, S1 and S

refer to the S1 scintillator. A ' and A' have high signal

threshold requirements. A bar across a detector reference

demands an absence of a signal from that detector.

The schematic of the electronics on the logic events

board is shown in Fig. 27 . All gates used in this board are

OR (or NOR) but negative logic is employed over most of the

board ("0" = TRUE), converting these to AND (or NAND) gates,

and will subsequently be referred to as AND gates.

In order that these events correspond to the indicated

type of particle, stringent timing and threshold requirements

have to met, resulting in 19 separate logic inputs from the

8 detectors. The correspondence of the inputs with a specific

detector, together with the pulse width and delay from the

time of origin are shown in Table II. The logic event inputs

generated on the various adder boards are connected to the

LEB (logic events board) via twisted wire pairs, feeding into

a series of line receivers (MC 1020) . The line receiver

outputs are connected to AND gates (MC1004 and MC1006) to

produce the logic rates shown in Table I. The use of two

different gates here results in a power saving feature, as

the MC1004 has output pull-down resistors which are omitted

on the MC1006 . In those cases where 8 input signals are

49

Page 55: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

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Fig. 27. Logic Events Board Schematic

Page 56: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

TABLE II

Logic Input Detector Delay Pulse Width(nsec) (nsec)

S]_ 95 20

90 75

AI;L 95 21

95 21

6 A13 75 45

7 A12 75 45

8 A12 92 23

9 S2 85 20

10 S21 15 20

11 S22 15 95

12 S2 70 43

13 A2 0 50

14 A^ 0 115

15 ^ 65 55

A22 70 43

51

Page 57: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Logic Input Detector Delay Pulse Wid th(nsec) (nsec)

17 A23 65 55

18 A21 70 43

19 A 80 40

52

Page 58: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

AND'ed output wired OR'ing is used. Hence an MC1006 is combined

with an MC1004 as only one pull-down resistor is needed.

Input 9 is generated from Input 10, which operates a 50

nanosecond one-shot constructed from two MC1004 OR/NOR gates.

Another 20 nanosecond one-shot following is triggered after

the first one-shot turns off, resulting in a 20 nanosecond

pulse delayed 50 nanoseconds from the input.

Rates 1 through 7 are available directly from the outputs

of the AND gates, and represent seven of the eight input rates

that are commutated thru by the data selector, MC 1038. The

control for this selector comes from the decision logic

board and advances the data selector one position each telemetry

frame. The eighth input (Rate 8) represents downward moving

electrons on one commutation cycle and upward moving (Rate 9)

penetrating particles on the next cycle.

Logic input 1 and Rate 2 are two inputs to a MC 1660

gate along with the "UP/DOWN" logic signal, to form Rate 8,

corresponding to electrons. Derived input 9, Rate 7 and

the "UP/DOWN" logic are the inputs to anoter gate, forming

Rate 9, or upward moving penetrating particles. The outputs

of these two gates are stretched 20 nanoseconds, OR1ed and applied

as the eighth input of the data selector.

The output of the data selector is gated by the P • R signal

from the encoder, so that counts accumulate during the time

that the 96 data bits are being read out. The 9-bit counter

consists of a D type flip-flop (MC 1022) and two 4-bit counters

(MC 7493). The nine outputs control the state of 9-bits of

the shift register in the data encoder.

Page 59: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

BIT SYNCHRONIZER

DIFFERENTIATOR 8 BAND PASS F I L T E H SHUNT GATE, INTEGRATOR ft OSCILLATOR

Fig. 28. Bit Synchronizer Circuit Schematic

Page 60: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

13. Power Conditioning Board

Power for the experiment will be supplied by Yardney

Silver cells, arranged as packs of 6.0 volts, each with

80 ampere-hour rating.

Those sections requiring regulation (all TTL and ECL

circuits for example) will be supplied regelated voltages

using 1C regualtors with or without external pass transistors

depending on the particular load requirements. The 1C

regulators will be types MC 1463 and MC 1469.

14. Bit Synchronization

A PCM telemetry system requires time synchronization of

the ground data decoding equipment with the airborne PCM

generator. The purpose of a bit synchronizer is therefore

to generate a ground clock in sync (but with a permitted phase

difference) with the airborne clock. Once the ground clock is

generated, it is then used to "clean up" the telemetered PCM

which may have been subjected to fading or other distortion.

The synchronization used here is a phase-locked loop with the

loop oscillator locked in sync with the airborne clock. The

bit synchronizer thus provides clean PCM data along with

necessary clock phases to the data decoder.

The bit synchronizer is composed of four principal parts

(see Fig. 28)/ a differentiator/doubler/filter section, a

shunt gate/integrator/oscillator section, a bit detector gate/

amplifier section and a counter/PCM output section.

The differential/doubler/filter section receives the raw

PCM input signal. After buffering and level shifting in the

55

Page 61: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

input amplifier (CA3015), the signal is differentiated in

the second stage (CA3000), with a balanced differential

output. Each pulse corresponds to a level transistion at

the input. The output is full wave rectified (4-IN270 diodes)

and filtered in a three section RC bandpass filter. After

amplification (CA3000), the balanced differential output is

applied to a shunt gate.

In the shunt gate/integrator/oscillator section, the

input signal from the previous section is applied to a shunt

gate (CA3019) along with a 25 kHa gate drive signal derived in

the counter/PCM section. When the loop is locked, the gate

drive frequency is identical to the input frequency, except

for a phase difference. This phase difference appears as a

dc voltage out of the gate that is amplified and integrated

(CA3015) and the error voltage is then applied to an astable

multivibrator used as the loop oscillator. The error voltage

controls the charging current for the timing capacitors and

so varies the frequency. A coarse frequency control is incor-

porated to achieve initial lock, after which the feedback

maintains lock. The oscillator signal (100 kHe) is buffered

and applied to the counter/PCM section.

The oscillator signal fed to counter/PCM section is

devided by two (50 kHa), then divided by two again (25 kHe).

This 25 kHa signal is fed back to the shunt gate. The

oscillator, the 50 kHa and 25 kHa signals are each inverted

and fed to a NAND gate, whose output is also inverted. Thus

56

Page 62: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

once every 1/25 kHa = 40 microseconds, a 10 microsecond pulse

is generated. This pulse triggers a one-shot (SN74121) for

a period of 23 microseconds. This one-shot signal is fed

to the bit detector gate/amplifier section.

The 23 microsecond one-shot signal is used to operate

a gate that has the buffered PCM input signal applied. With

the one-shot pulses at a 25 kHa rate, the gate is opened

whenever it's possible for a new logic level to be present.

With the NR8 telemetry format, each logic level is held for

the full period, i.e. a "1" will be held at a "1" level for

40 microseconds and if the following bit is also a "1", the

logic level simply remains at the "1" level for another full

period. The gating signal (23 microseconds) is adjusted

to fall inside a given data bit' speriod, so the output of

the gate will be a series of 23 microsecond pulses when

"1" is present at the input. These pulses are squared up by

a diode limiter circuit and amplified and are fed back to the

counter/PCM section.

The restructured PCM pulses operate a one-shot of 32

microseconds in the counter/PCM output section. These pulses

are applied to a D flip flop and clocked out using the 23

microsecond wide pulse stream. The outputs therefore are clean

PCM signals along with two clocks lines, at 0 and 90 phase,

in synchronization with the PCM.

57

Page 63: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

15. Data Decoder

The equipment consists of two standard 7" x 19" panel

mounted chassis. The first contains the electronics and

programming functions and the second a neon display of the

PCM bit pattern. The electronics section is entirely TTL

integrated circuit logic. It consumes 15 watts at 5 volts

while the neon display consumes 20 watts at 135 volts.

The electronics section may be divided into several

functional units, the counting unit, synchronization circuit

board, error counters, data control board, and data storage.

The main counting unit receives an input clock from the bit

synchronizer and generates all necessary internal timing pulses.

The synchronization board inspects the incoming data to find

the correct synchronization pattern. The bit errors entered

in this board are counted in the error counter board which

gives an output pulse to the counting unit causing it to shift

the bit stream by one bit. In this manner, the bit stream, is

inspected until the synchronizing pattern is found. The search

and lock modes are provided in the error counter board to insure

that the identified pattern is the true synchronization pattern

and to prevent the unit from searching due to bit errors caused

by atmospheric noise or other transient phenomena.

The data control board provides the proper driving fan

out for the S/R clocks and storage latch transfer pulses.

Circuitry is provided to read out several 8, 0 and 10 bit words

for analysis. A timing circuit is also incorporated so that

58

Page 64: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

transfer of the bit stream to temporary storage may be carried

out on a continous or a timed basis. The event interrogator

compares event bits in storage with the incoming bit stream

to determine the presence of a new event. The event pulse

generated is used to trigger the serial word output in a

manner such that the output is obtained only when the unit

is locked onto the bit stream and a verified signal is present.

O C^i

A. Main Counting Unit. Both clock phases (0 and 90 )

required for operation of the data decoder are initially

inverted to provide both isolation from the driving source

and the complimentary phase clock for internal timing purposes.

A second inversion then reconstructs the initial clock phases.

In the case of the 90 clock, the inverted phase (270 ) is gated

with the 180° clock to provide a 360° cutoff. An inverted 0°

clock is gated with the 270 error output from the error

counters board and drives a 7 bit binary counter, made from

the 4 bit counters Ml and M2. The error input is used to

provide an extra count in the timing unit to search the bit

stream (see explanation in error counter description). See Fig. 29,

The outputs of the 7 bit counter are inverted and the

proper combination of inverted and normal outputs are used to

provide internal timing pulses by appropriate gating in the

8 input NAND gates M3-7. These gates provide timing pulses

at the 8th, 9th, 10th, 32nd, and 128th clock pulses. The 32nd

and 128th pulses are gated with 0° and 90 clock pulses to

59

Page 65: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

S ISC" C.P. OUT 5V

5 |0° C.P. IN I3|

S ERROR INPUT

5V

7ic. 29. Data Decoder -Main Counting Unit.

Ml,2 SN7493 4Bit CounterM3*-7* SN7430 8-input NAND GateM8*-10* SN7404 Hex invertersMil*,14* SN7402 Quad 2-input NOR GatesM12* SN74121 Monostable MultivibratorsM13* SN7474 D-Flip Flop

*Pinl4: Vcc (5V) ; Pin 7: Ground

Page 66: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

provide both 180 and 270 phases for these pulses, necessary

for internal timing requirements.

The 270 clock pulse is also used to drive multivibrator

M12 which provides a 1 microsecond pulse at 270 during each

clock period that is used for internal timing.

The 32nd (270°) and 128th (270°) pulses are applied to

the preset and clear inputs of D-flip flop M13. The output

of M13 is used to provide gating for the data and I.D. sections

of the bit stream. These outputs are referred to as 32 (270°)

hold and 128 (270°) hold, respectively.

B. Synchronization Board. At the initiation of each

frame, the 128 (270°) hold is applied to a NAND gate (-«S19, Pin 2)

simultaneously with the data input. This allows the following

32 bits to be clocked into the 5 bit Shift Registers, Si-7 on

the 90 clock. An input inverter 1/6S18, Pin 9 is provided

for normal-inverted sync pattern. The 32 (0°) and 90 latch

clock (derived from the output of multivibrator S20) are gated

and open the storage latches for parallel storage of information

from the S/R's. The latch clock must have a lower cutoff than

180° so as not to interfere with the subsequent operation of

the identification cycle (See Fig. 30).

The latch outputs are all inverted so that either the

normal or inverted latch output is available for application

to the preset input of the appropriate bit in the S/R's (i.e.

latch position 27 must be connected, either normal or inverted,

to preset input of bit 27 of the S/R's).

61

Page 67: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

LATCH CLOCK OUT (INVERT)!

LATCH OUT (NORMALI-

-9O- CP \H

ERROO OUT(TO ERROR COUNTERS!

1 — 1

SN7400

11 6 14

5 S-20 l iSN74I2I

10

5V

*'•±.001— 1 t-ia

R E F E R S TO PIN NUMBERON THE BOARD, COMPONENTSIDE

(PROGRAM OUTPUTIS CONNECTED TORESET INPUT FOREACH BIT)

CLOCK AND TIMING

PULSES FROM MCU

Fig. 30" Data Decoder - Sync Board

Page 68: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

The 32 (180°) pulse is applied to the preset enable of

the S/R's, while the 270 , 1 microsecond pulse is gated with

the 32 (0 ) pulse and the inverse is applied to the clear inputs.

The programming logic is as follows:

1.) the inverted latch output corresponds to programming

a "1" for the particular bit being considered. The

normal output represents a "0".

2.) e.g. suppose a bit is programmed for a zero (normal

latch out connected to preset input), and a "1" is

clocked into this position at the 32nd clock pulse.

A "1" then appears at the preset enable, and at 32

(J80 ) is shifted into the S/R. Since preset over-

rides clear, the "1" remains in this position at the

end of the identification procedure.

3.) A similar analysis is made for "0" programming.

When all the errors have been entered into the S/R's,

the number of bit errors is then serially clocked out to the

error counters board.

63

Page 69: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

C. Error Counters Board: The bit error output from the

sync board is clocked into the first decade counter (112) of

thi.s board and accumulates the number of bit errors registered

in the identification cycle. Gating to this counter insures

the counting of errors only in the 32 bits succeeding the

identification cycle, and only until the counter has achieved

the desired number of counts. Decoder 115 is used to give a

decimal selector for bit error programming (front panel

switch SW-1). See Fig. 31.

Upon reaching the desired count, the falling edge of the

output of 10 position switch SW-1 triggers multivibrator 110

which provides a gating pulse to NAND gates 121. If the unit

is in the search mode, the 270 , 1 microsecond pulse is gated

to the main counting unit error input and the reset gates of

decade counter 113. If in the lock mode, the 270 pulse is

gated to decade counter 114.

(1) Search. In the search mode, decade counter

114 counts 90 frame rate pulses until a desired number of

counts are reached. When the count is reached, the selected

output from decoder 116 provides a negative pulse to the

input gate of the counter, thus closing the input to further

frame rate pulses. Until the desired count is reached,

the decoder output is in the "1" state and thus is applied

in a normal fashion to 1/3 121 Pin 4 and inverted to 1/3 121

Pin 1. The first gate provides routing of the 270° pulse

to the Main Counting Unit and the reset gates of 113. The

64

Page 70: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

n-i.2.4128(0') IN"n-i

-90"C.P. IN

1-3o* c.p, m~

I - l lERROR IN"~

(FROM SYNC321-180') IN-

1-12

r

1-5

U— 4 S W I I N

fluuSW2 IN

I—,SW3

I-IO

1-30' C.R IN-

1-4DATA IN-

iBITSTSEAM)

1-25V-I- '

G N D -

:

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IN

_

2

,g£—

i.K*r~v% iI .OIJL>jfd-r_

5 614 J

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10 7

— fi^~1 ioi — N.-— ii -i-izoV- ..^-rJiy

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*f.01 J~ftaTL.

5 3

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10 6

q l\ 8

^tt£& 1-

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TO

i h i i2 3 1 « ~

12 -i- 15 3 — 0

9 |4 4 — — — 0

5 6 7,0" '* 1 - °t

i I 1 1 10 • —5V i 16 811 ~ —

4, *

|Q(

9&I24J8~i

t r^[ 16 8 |

Sr- ... 14 1 *

} j, ^ 1-13 a §1 1-16 3 : O

tJi12^ s u r T Vr^ — ' 5 6 7 10 " 9 ..- 0

j [ | J 10

fl^- " ^^ ' L!^ [»*) i-.6-_1* ^LX^ i-e

! i 1-7",- -J rmi r— i i n ^ S"RCMOUT

ufr\o.2_61B>_ ,,.00'^ildT T Ih 1 T T J14 II 10 3 4 7

5 I - l l 6

4fv^_JJ41'3P

La — xjai ,-,, \?Trji12^/ —

- ' -*

3

2 |l-!9 5

5V

I 1 t U2 3 5 10 1

1214 '- :1 1

6"X

-

I 1 b r IU ' 'l2_i-,5 3 0,

73&124). 14 1-14 " 1-17 5 O-SC__X 8 13 6 o

5 32 9 01 I IQ . ,_

5V - 16 811

9. v- f\ . 7« TO SIO^IHjB-^J5l2p«-J

1-9*, 10*, 11*

,3 ,.. I- 12. .13, 14

/i/sN/ 1220"

_5. — .— ;iJ20V_^

»S.O

L

IS™?-1 1-15,16,171-18

v 1-19*^ rrrsv

T-?ni i 13 14 „ ;1^1 n-3 I'21 -

1-23,24

SWI IN* 1"

T_i — 1

o— — o

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^-^S«2

0

DUT (TO M.C.U.)

O

^

S*3

OO

W3 IN<

SN74121SN7490SN7442SN7493SN7474SN7420SN7410SN7404SN7400

4.*Pin 14: Vcc (5V) ;

Pin i: Ground

Fig. 31. Data Decoder - Error Counters

Page 71: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

second sends the 270 pulse to decade counter 114 when in

the "lock stage."

When the unit is in the search mode, the reset gates of

113 are enabled, allowing this counter to return to zero

every time the desired number of bit errors is exceeded.

When the desired search frame count has been reached, the

unit is then locked onto the sync pattern.

(2) Lock Mode. In the lock mode, the 270 error

pulse, if present, is not routed to the Main Counting Unit,

but to the input gate of 114. In the absence of an error

pulse, the inverse 90 frame rate is applied to the clock

input of D flip flop 119 Pin 3, thus clocking a "0" into

this unit (the D input is a 180° clock pulse). The Q input

is gated with the signal loss indicator and enables the reset

gate of 114 which causes this counter to be reset to zero

by the 5 microseconds output of the multivibrator 111

(activitated by the 0 frame rate pulse). If an error pulse

is present, a "I" is clocked into 119 Pin 3 thus disabling

the reset gates. The error pulse is simultaneously applied

to the input gate of the counter, the output of decoder 117

enabling this gate. In this manner if a consecutive specified

number of frames with bit errors exceeds a desired number

decoder 117 changes to a zero state, disabling the input

gate to 114 and resetting 113 to zero, thus re-initiating

the search mode.

This procedure prevents time lost in reverting to

"search" when an excessive number of bit errors occur in a

66

Page 72: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

non-receptive manner (such as might be caused by transient

atmosphere interference with the telemetry signal).

The loss of signal indicator counts the data bits applied

to 118 and must count 16 "1" bits to insure that the

signal is preset (logic "1" appears 18 times in the sync

pattern). Upon reaching the count, the decoded output

disables the input gate and enables the reset gate of 114.

The decoded output is also applied to D flip flop 1/2 119

Pin 12 for temporary storage.

D. Data Control Board. The data control board contains

the clock drivers for the data boards and the serial output

gates for the words to be pulse height analyzed. The latch

clock (multivibrator S-20) from the sync board is applied

to inverter drivers to provide the proper fan-out for the

data board S/R clocks. This clock is also gated with the

transfer pulse and then applied to the latch inverter drivers

to provide parallel data transfer to the Data Storage Latches.

The serial P H A output is generated as follows (See Fig. 32)

The inverse event pulse is applied to the clear input of

C-7. The preset input is connected to the lock output

(from error counters) and the D-input is held at a "1" level.

The clock is the 8, 9 or 10 inverse pulse.. In this manner,

a "0" output of 8, 9 or 10 bit length is available at the Q

output. The data to be pulse height analyzed is gated with

a 180° clock and this output is applied to a "NOR" gate, the

other input of which is the Q output of the above flip flop.

67

Page 73: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

1

27

LATCH _- CLOCK 9

(SYNC. BOARD

LOCK-!i

TRANSFER -**-PULSE

12

3

II

^ 5< %&*

FROM «QATA S.OATA

BOARDS

2A, DATA

4\. AjDATA

E V E N Tv^3

LOCK **"

_" ^

r H «

^V

ft1+1Pl»

Pt»

CCCCC

5V

I3[icfc»12! [45!>--

II (l^lOU/*

" ' C3\> • KrT~»224 LZP |ic*p

1 ' 3I'C3>4

n~c«v i 'fTo^^^^1 sj 4 cy" e^ ..9 'c^> 8

"[^csy0^^^^^ I3rci>12

• 'PcVto2

'PtJ^B4

rs. K>*a irive1-^

l 9rN^8, , B i l e VX> O

M KcV)!10

"licXV2

PIN A9 .. 15 ^

v _/ Isi 1^^ T *}I2r x1^ (^ ' ' c?\9 Sl^Xo6

i s i C2 F — !tci>L-io — P^... i) — / j-,

~~ — ii — \ », ^csV H^V10

H* y PIN A^ 9jj_55> — ~4i — \ HN A3[i — n' v13 '

9 J-c5^ £~T^"Ntol F

IjJI ™I2 Ir f 4i j j csW *il— "i- PIN 04( ) ( ) PIN Dj

°3 13 9 S

r - C7

0|

o2

'-!*• SN7404 Hex inver•_2*,5* SN7400 Quad NAND'-3*, 4* SN7404 Hex Inver:-6* SN7402 Quad NAND•-7* SN7474 D-Flip Fl

nArv

=IN

3IN

>IN

IN

te

Of

T^X^

e

IB

J9

20

13

16 LATCH-CLOCK

17 TO PINS

24 C ' -2 8 3

25

26

21

22

23 ^

I0\

01

02

PHAOUTPUTS

sr

sr

D

*Pin 14: Vcc (5V) ; Pin 7; Ground

Fig. 32, Data Decoder - Data Control Board

Page 74: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

The output of the NOR gate is then the information contained

in the 8, 9 or 10 bits immediately following the event pulse,

These bits may be taken from any portion of the bit stream

(from the data S/R) and thus any 8, 9 or 10 bit word may be

serially clocked out of the bit stream. The lock function

at the preset input is provided to insure that a word will

not be inspected when the bit stream is not locked in.

69

Page 75: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

E. Event Interrogator and Storage Transfer Time (Auxiliary

Data Control Board). The I.C's on the rear third of the error

counters board and the auxiliary data control board form a

functional unit (See Fig. 33).

An inverse event pulse applied to the B input of multi-

vibrator E-5 while input A-3 is connected to "search", generates

a 12 bit-width pulse at the Q output when the data decoder

synchronizer is in the lock mode. This output activates a

NOR gate allowing a 270 clock pulse to be applied to the

clock inputs of S/R's E-l, 2 and 3. At each new event, the

event information is then clocked into these S/R's and this

data is compared at the frame rate with the bit stream

accumulated in S/R's D-3, 4 and 5 of the first data board by

means of exclusive NOR gates 1-1, 2 and 3. The gate outputs

are combined in NAND gates 1-4 and 5 and a pulse indicating an

event appears if any one of the data bits differ from the

bits held in storage in E 1, 2 and 3.

Transfer of the bit stream to storage (Fig. 34) is effected by

either this event pulse or the framerate pulse selected by

SW-4, on a continuous or timed basis (SW-5). The timing

mechanism is triggered by the trailing edge of the transfer to

storage pulse and enables multivibrator 1-8 to be fired by

the rising edge of the next frame rate pulse. This inhibits

the transfer pulse until the multivibrator returns to the

quiescent state. Two decade counters are provided to give three

orders of magnitude in the inhibiting time for the transfer pulse.

70

Page 76: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

L_SEARCH

3

41

7 14

E-5 ||

10

Li-

*I 1-3*I 4*I 5*I 6*I 7*I 8

E 1-3*E 4*E 5*E 6*E 7E 9,10

MC3022SN7430SN7410SN7404SN7400SN74121

SN7496MC7402SN74121SN7474SN7400SN7490

EVENTOUTPUT

*Pin 14: Vcc (5V) ;Pin 7: Ground

Unless otherwiseindicated, input(output) is to(from) I.e. Pinindicated.

'Sf<)° CLOCK PULSE

Fig. 33- Data Decoder - Event Interrogator fcTransfer Timer

Page 77: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

1 -2-

SV

F5V

F

bF

FCLOCK FROM 5|VDATA CONTROL [_

F

A 9-^d^-

'— 1i516

D-512 H

' 29 ISI

11

I S16D-4 10

1 2 I I

• \l9 IS1

11

5

16

12 II8 B9 151

1

5 "16

0-212 j

" 149 IS|

1 KJ

b IJ16 14

D-l IS128

9

1 r

INVERTED.

Jr

(***

" n3 24 T 4

15 "7

21 B 23I

\LJFRO*

VVPy 3 24 f 4

i6 0-7 ia17

22 2O

i

\

n-cn CLOCKPINS 18— 21)

I

5V

10 91 1 aIS 0-6 IS16 17

12 23I ^v~.. f

.PIN AJ

0

"M *-, T26 A

22 °

20 *

E

pAR

19 *a L

"Is L

"Is °- * u-iz T

puT

-9-8- 7-6

X MOLD 8-{-J-*(«_iy- I«^X NORMAL

[CONNECTOR AND 1LIMSI* VNC* BOARDJ

[l/«CI LOCATED ON 1[DATA CONTROL BOARDJ

D 1-5D 6-8

SN7496SN74100

5 bit S/R8 bit Latch

4 identical serial in-parallel storageout data boards have been contructed.Wiring differences are noted below:

Board 1) a)Parallel output D-5(14,15),0-4(10,11,13,14,15) andD-3 (10 11,13,14,15) toevent interrogator

b)Serial word out (PHA-S,)from D-2 Pin 10 to controlboard

2) a)Serial word out (PHA-S2)from D-4 Pin 14 to controlboard

3) a)Serial word out (TOF) fromD-5 Pin 13 to control board

b) Serial word out (PHA-Aj_)from D-3 Pin 13 to controlboard

4) a)Serial word out (PHA-A2) fromD-4 Pin 10 to control board

Fig. 34- Data Decoder - Data Board.

Page 78: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Photographs of the front and rear views of the data decoder

are seen in Figs. 35 and 36.

16. Acknowledgments

Much of the work has been funded by NASA grant NCR 05-008-022

and DOD Themis contract N00014-69-A-0200-5001.

Special credit goes to Mr. Rokutaro Koga, Mr. Robert Melendes,

Mr. Alan Preszler, Mr. David Register, Mr. Robert Walker and

Mr. Robert Seemann for carrying out a significant part of the

design, construction, and test of the electronics for the

solar neutron experiment. We also thank Mrs. Ildiko Kerek for

the long hours spent preparing the necessary drafting and art-

work for this report.

73

Page 79: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 35. Data Decoder Front View

Page 80: CASE - NASA · thresholds and strobe inputs in integrated form (MC 1543L) are used. After discrimination, the pulses are all normalized to a fixed amplitude (Emitter Coupled Logic)

Fig. 36. Data Decoder Rear View