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A Case Study in NASA-DoD - The Black Vault

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-127-<br />

Table B-2<br />

POWER SUMMARY<br />

Characteristic AEM STPSS MMS<br />

Peak array power possible, W 238 a 1200 :6600 b<br />

Average array power available<br />

to space vehicle dur<strong>in</strong>g<br />

illum<strong>in</strong>ation, W 133 1200 3600<br />

Average power available over<br />

a low altitude orbit, W 68 500-600 1200<br />

Average spacecraft housekeep<strong>in</strong>g<br />

power, exclud<strong>in</strong>g experiments<br />

and associated<br />

telemetry, W 28 100-200 350<br />

Cont<strong>in</strong>uous or average power<br />

available for experiments<br />

over a low altitude orbit, W 40 400 850<br />

a<strong>The</strong> 238 W is the peak of the power curve which<br />

roughly resembles a positive half s<strong>in</strong>e wave, s<strong>in</strong>ce the<br />

array is not sun-track<strong>in</strong>g.<br />

b<strong>The</strong> 3600 W is set by the peak power handl<strong>in</strong>g capability<br />

of the PRU; actually, there is no maximum s<strong>in</strong>ce<br />

still higher power arrays would merely be used less<br />

efficiently. <strong>The</strong> excess electrical power would not be<br />

drawn from the array, which merely results <strong>in</strong> a slightly<br />

higher array temperature.<br />

CThis assumes that power is supplied at a constant<br />

rate to the spacecraft loads over the entire low altitude<br />

orbit and that the battery capacity is adequate to<br />

store the energy required over the period the array is<br />

occulted.<br />

d<strong>The</strong> power bus is rated for 1200 W maximum, limit<strong>in</strong>g<br />

the total load that can be supplied.<br />

however, optimiz<strong>in</strong>g the array power output is not likely to prove necessary.<br />

Thus, there is a clear dichotomy <strong>in</strong> emphasiz<strong>in</strong>g peak power track<strong>in</strong>g<br />

for efficiency <strong>in</strong> a multipurpose vehicle.<br />

Some of the ±7 V variation of the MMS bus must be due to series<br />

voltage drop <strong>in</strong> the PRU.<br />

In addition to this slow dc variation, there<br />

is a superimposed 70 Hz ripple caused by hunt<strong>in</strong>g of the peak power<br />

tracker about the optimum. While this has been measured to be about

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