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Massachusetts Institute of Technology Instrumentation Laboratory Cambridge, Massachusetts Space Guidance Analysis Memo #9-67 RECEIVED JUN 1 9 1967 FHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing moment on the vehicle can be produced by an initial misalignment of the thrust vector relative to the vehicle CG. This misalignment can be caused by: (1) An uncertainty in the information, on the CG location, used by the astronaut to pre-align the engine, gimbal servos. (2) A mechanical offset in the positioning of the engine nozzle by the pitch and yaw gimbal servos. (3) A misalignment of the thrust vector relative to the nozzle center- line. The necessity for stabilizing low-frequency slosh and bending modes of the CSM - LM vehicle places some severe limitations on the gain and bandwidth of the CSM - LM digital autopilot filter. As a result of these limitations, the use of the autopilot feedback loop to generate a signal to compensate for thrust misalignment would result in the buildup of excessive attitude errors. Therefore, an auxilliary external correction scheme is needed to augment autopilot action in pro- viding this misalignment correction. A number of such schemes have been proposed and are being investigated.
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Page 1: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

Massachusetts Institute of Technology Instrumentation Laboratory Cambridge, Massachusetts

Space Guidance Analysis Memo #9-67

RECEIVED

JUN 1 9 1967

FHM

TO: SGA Distribution

FROM: Edward Womble

DATE: June 7, 1967

SUBJECT: A Recursive CG Correction Scheme

Introduction

At the initiation of thrust, a disturbing moment on the

vehicle can be produced by an initial misalignment of the thrust vector

relative to the vehicle CG. This misalignment can be caused by:

(1) An uncertainty in the information, on the CG location, used by

the astronaut to pre-align the engine, gimbal servos.

(2) A mechanical offset in the positioning of the engine nozzle by

the pitch and yaw gimbal servos.

(3) A misalignment of the thrust vector relative to the nozzle center-

line.

The necessity for stabilizing low-frequency slosh and

bending modes of the CSM - LM vehicle places some severe limitations

on the gain and bandwidth of the CSM - LM digital autopilot filter. As

a result of these limitations, the use of the autopilot feedback loop to

generate a signal to compensate for thrust misalignment would result

in the buildup of excessive attitude errors. Therefore, an auxilliary

external correction scheme is needed to augment autopilot action in pro-

viding this misalignment correction. A number of such schemes have

been proposed and are being investigated.

Page 2: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

A method for recursively canceling the effects of the

disturbing moment is presented here. A correction signal is applied

to each engine gimbal servo immediately after the first attitude mea-

surement is received from the IMU, and is updated with each subsequent

measurement.

Page 3: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

Statement of Problem

The model of the vehicle used for this derivation is shown in Fig. 1.

1

w

+ a ow

In Fig. 1:

(1) w (t) is a driving signal characterized by unbiased Gaussian 2 noise with the known covariance 6.

(2) r (t) is a measurement error characterized by unbiased

Gaussian noise with the known covariance a 2 .

(3) z is the IMU measurement.

(4) The state is defined to be

x [61 T RB' RB' '

where O RB and eRB are the vehicles rigid body angular

position and angular velocity, and 6 b is the disturbing

moment.

(5) The initial value of the covariance of the state estimate,

P (0)), is known.

A (6) X

3 is the previous best estimate of x

Page 4: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

(7) 6 c is the commanded engine position.

The difference equation corresponding to the state diagram in

Fig. 1 is:

x (n + 1) = (n) ru (n), (1)

where

2 31

AT AT ATk1 AT k 2

2 6

0 1 k AT 17= k AT AT2

0 0 1 J L 0 AT

u (n) = [ S c (n)x3 (n), w (n)1T

The best estimate of the state at the n 1 sample, prior to the n 1 mea-

surement, is

(n + 1) = 4 (n) + ru (n), (2)

where

and

71 (n) = [O c (n) - X3 (n),

0

Q (n) = u (n) u (n) T =

a 2 w

The problem is now to determine the value of O b from the noisy measurement

z .

4

Page 5: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

Derivation

Subtracting (1) from (2) yields:

e (n + 1) = x (n + 1) -x (n + 1 [P (n) - x (n)] (u) - 11)]

Therefore, the estimation covariance at the n + 1 sample, prior to the n + 1

measurement, is

M (n+ 1) = e (n+ 1) e n+ P(n) O rr rQ (11)F T

[S4i (n) - x (n)] [ (n) - u (n)]

[ (n) -

( )1 [x (n) - x (n)]

However,

[ S c (n) - 3 (n)] - (n) -

3 (n)]

u (n) u( ) =

0

w (n) 0 - w (n)

, w (n) = 0, and w (n) and [ IX (n) - x (n)] are independent, therefore,

M (n + 1) = P (n) O T + rc, (n) rT. (3)

If a signal with a gaussian distribution is passed through a linear system,

the output of the linear system has a gaussian distribution.

the distribution function for lc (4) is:

Therefore,

Page 6: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

1 2

e 1 2 0- 2

r 2 2 r

f2

[r (n)] - (5)

1 e -1/ 2 [ (n) - Tc (n)] M - (n) Ex (la) - Ti (OJ T f 1 [x (n)] _ _ 1 3 2 1/ 2 2 1M (n) I

(4)

The probability density function for the measurement noise is

Since the measurement noise is white, r (n) and x (n) are independent;

therefore,

f [x (n), r (n)] = f 1 [x (n)] f2 [ r ( )],

or,

f [ (n), r (n) - 1 - 1 (n) - (n) ] M (n) [x (n) - (ne

2 x 47r a I M (n) I

1 2 e

(6)

The estimated value of x (n) that maximizes the joint probability density

function (the most probable value of x (n)) maximizes the argument of the

exponential given in (6). This then is the Maximum Likelihood Estimator.

The likelihood function is

1 L [x (n)] =

2 (n) - ( ) m -1 (n) [ x (n) _ + 1 r 2 ar2

(7)

Notice that minimizing (7) is the same as maximizing the argument of the

exponential in (6).

Page 7: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

1 1 A ) 2 ) h z (n) + 2 h hT x (n) = 0 -- — o- o-

-1 (n) x M (n) (n) -

r r

From Fig. (1), the relationship between r (n), z (n), and x (n) can be

derived by observation.

r (n) = z (n) - h T x (n) ,

(8 )

where hT = [1, 0, 0 . The substitution of (8) into (7) yields:

L [x (0] = 2 [x(n) - 3E(n)]M -1 (n) [x(n) - TE(n)1 T + 1

(n) - h 1 (n)] 2

2 6 2

r

The first variation of the likelihood function is

1 (5L = dT x (n) M -1 (n) [x (n) - (n)] - dT x (n) h z (n) - hT x (n)].

(9)

The value of (n) which causes L

from (9).

(n)] to be stationary can be derived

1 T -1 1 T - 1 h h + M (n)] (n) = [ 2 h + (n)] x (n)

2 --

o-r

gr

1 h

+ o- — 2

[z (n) - hT x (n) ]

r

Page 8: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

Therefore,

A 1 x = x (n) + (n)

2 [ z (n) - h T x (n)i,

r

(10)

where

-1 (n)= 2 1 h h T M

-1 (n)].

o-r

It will now be shown that qi(n) is the covariance of the estimate at the nth

sample after the incorporation of the nth measurement according to (10).

The time subscript will be dropped for this derivation. Let e =x, then

A _ e=x-x+x-x - -

The substitution of (8 ) and (10) into of, 12 ) yields:

, 1 e y h hT x+r -h

r

or,

1 e = -2

qhr + (I - 1 -2 qi h. hi') (37 - x) - o- - - - r r

From (13) P can be expressed as

(12)

(13)

1 1 P = e e

T = q.i h hT LliT + (I - 1 2 hT) M (I -

2 - - 2 o- o- o-

r

(14)

r r

Premultiplying (11) by 4 and then postmultiplying by M yields

Page 9: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

M = + 12 Lp h hT M, — —

r

or

(I - 12 h hT) M = a — — (15)

r

The substitution of (15) into (14) yields:

P - LP h hT LP T + (1 - h hT) T — — — — o-12

r a-12 r

or

1 T T 1 P= LPhh - LPhh + —2 — —2 —

ar o-

r

Therefore,

P = .

Summary

The correction scheme is summarized below.

(1) Precompute and store in the flight computer the filter

weights for the maximum likelihood estimator as follows.

(a) Let w (n) =P (n) h, where the initial covariance o-r

P (0) is given.

Page 10: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

(b) Extrapolate the covariance matrix using (3)

M (n + 1) =cb P (n) cb T + (n)F T (3)

(c)

Calculate the covariance matrix, after the incorporation

of the measurement using (11)

P (n + 1) = [ 1 T - 2 n+ 1)] (11)

r

(d) Calculate the n + 1 weighting vector from

1 w (n 2

l) P (n+ 1) h CY r

Repeat (b) through (d) until a sufficient number of filter weights have been

calculated.

(2) In the flight computer

(a) Extrapolate the state using (2)

3:E (n + 1) = x (n) + (n) (2)

where x (0) is given.

(b) Incorporate the measurement using (10).

A — x (n + 1) = )e (n+ 1) + w (n + 1) [z (n + 1) - h T x (n + 1)] (10)

(e) Apply the thrust vector misalignment signalcor (n + 1) A , , ,

= x 3 (n + 1) =Ab

(n + 1)

1 0

Page 11: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

A block diagram of this correction scheme is shown below.

Figure 2. A Block Diagram of the Implementation for the Recursive Correction Scheme

Equations (2) and (10) can be simplified for programming as follows:

Equation (2) written out is

A A (n + 1) (n) + AT 8 (n) AT A

2

—2-- 6b (11) + k

2 6 (n) 16\ (0] c b

(2a)

(n + 1) = 8 (n) + k AT 16;3 ( )+ k AT [ o c (n) 16;3 (n)]

(2b)

T (n+ 1 (n) (2c)

, or,

79- (n+ 1) 8 (n) + AT 0 (n) -F

0 (n + 1) = 8 (n) + k AT o c (n)

b(n + 1)=&b (n)

11

Page 12: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

9 (n+ 1) + w 0 (n+ 1) (16)

8 (n+ + w 1 c (n+ 1) (17)

b (n) + w2 c (n+ (18)

0 (n+ 1) =

e (n+ 1) =

b (n+ 1) =

Substituting 2') into (10) yields:

where w (n + = [w 0 (n+ 1), w 1 (n+

and c (n+ 1) = z n+ 1 ) hT x (n + 1) = z (n + 1) - 9 (n+

12

Page 13: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

Results

This correction scheme has been applied to the CSM and the

CSM - LM vehicles. A total thrust vector misalignment of 1 was used

for each simulation.

Plots of the attitude, engine angle, and the velocity error verses

time for the CSM vehicle are shown in Figs. ( 3) thru ( 5). Correspond-

ing plots for the CSM - LM vehicle are shown in Figs. (6 ) thru ( 9).

Page 14: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

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Page 15: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

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Fig. 5. A plot of the velocity error versus time for the CSM.

16

Page 17: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

10 . 0 15.0

Time (sec.)

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Fig. 6. A plot of attitude error versus time for the CSM-LM.

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Page 18: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

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Fig. 7. A plot of the commanded and the actual engine position versus time for the CSM-LM.

Page 19: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

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19

Page 20: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

Conclusions

It was found that the attitude errors were less than 3 degrees for

the cases shown in Figs. (3) and (6). The curves shown in Figs. (5) and

(8) indicate that the velocity error for a 25 second burn without steering

never exceeds 0.5 ft/sec. in the case of the CSM vehicle, and 4 ft/sec. for

the CSM - LM vehicle.

Figures (3) and (6) indicate that there might be -a relative stability

problem produced by the addition of the corrective signal. However, the

resulting system does appear to be stable in an absolute sense The curves

in Figs. (4) and (7) show that the correction signal rapidly approaches the

value required to cancel the the initial thrust misalignment and then oscil-

lates about this value. Therefore, the correction process could be termina-

ted early by supplying a constant bias equal to the average value of the os-

cillating signal after approximately 10 seconds. This would eliminate the

stability problem.

The interaction between the estimator and the original system is

being investigated to determine the resulting stability margins. It is hoped

that these studies will lead to approaches for improving the overall system

stability through revised estimation procedures, and better coordination be-

tween the autopilot design and the estimator selection.

20

Page 21: FHM -  · PDF fileFHM TO: SGA Distribution FROM: Edward Womble DATE: June 7, 1967 SUBJECT: A Recursive CG Correction Scheme Introduction At the initiation of thrust, a disturbing

References

Battin, Richard H. , Astronautical Guidance. New York: McGraw-Hill,

1964, pp. 303 - 317.

Bryson, Arthur E. and Yu-Chi Ho, Optimization, Estimation, and Control.

Waltham, Massachusetts: Blaisdell,(to be published), ch. 12.

Cherry, George and Joseph O'Conner, "Design principles of the lunar

excursion module digital autopilot, " M. I. T. Instrumentation Laboratory

Technical Report No. R - 499, July 1965.

Frazier, Donald C. , "A new technizue for the optimal smoothing of data, "

Sc. D. thesis, M. I. T. , Cambridge, January, 1967.

Stubbs, Gilbert, "A block II digital lead-lag compensation for the pitch-

yaw autopilot of the command and service module, " M. I. T. Instrumentation

Laboratory Technical Report No. R - 503, October, 1965.

21


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