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NovorthdanfS high frograonq CIQBfi~Uda 0r-r<br />

conpnornen, 810 might Fm hducadl By<br />

fioxiblo oppndagdo aubjoctad BO eranniont<br />

forceo, auat bo minilsiaod duo to tho be8<br />

effect they may have on iInQq0 gyslity.<br />

6.3 Spacecraft platform rewironants<br />

WO outlino some3 platform aubnyatona design<br />

aspecto ROB~ relevant to SAR performance<br />

and operation.<br />

Low orbit altitudes will raqludra oloctric<br />

propulaion, which must be cosmaidlalrod an<br />

enabling technology [J] for thoso SAR<br />

lightnats missions, as alroady discussed.<br />

tJevertho1ese. flying satelhitan at lou<br />

altitudo has also positive offmts, in<br />

pdrticular concerning the more benign<br />

environment (5).<br />

The stiucture design, departihg from<br />

conventional, should adopt a highly<br />

integrated aQprOxh where a t avmt~ frame<br />

utilizoa important SAR payload copponents,<br />

like tho antenna or big boxm, ab part of<br />

the structure itself, in ordar to save<br />

mass. Since the bulk of tho heat is<br />

produced by the SAR HPA, heat rejection<br />

shc*ilci be by direct radiation Fo spaca as<br />

far as practical: this is certainly easier<br />

on down-dusk orbits. I<br />

The solar array design ia ntrongly<br />

dependant upon the SAR payload operating<br />

duty. Infact, since the SAR will normally<br />

operata for short intervals totalling 5 to<br />

10 8 of tho orbit poriod, payload supply<br />

can normally be from battgry, the solar<br />

array merving mainly for battery<br />

recharging. The orbit plane cholce, and<br />

the percentage of time spont In Enrthshadow<br />

p ~r orbit period, will alno impact<br />

the OOlkr array siting t0 provide the<br />

required energy. Bosidos, electric<br />

propulsion DC power requiresnnts, will<br />

also increase the solar army siting.<br />

Accordingly, the solar array hype may<br />

range Prom a fixed wings' configuration,<br />

suitablo for satellites in' sunaynchronoue<br />

down-dusk orbits, to a sun-tracking<br />

configuration for Spacecraft :n low to<br />

medium inclination orbits.<br />

On the above grounds, long lifetime<br />

operation of mass-efficient battories,<br />

subjected to rathor deep and pariodic (up<br />

to 30000) discharge-recharge cycles is an<br />

oustanding issue for. such L.E.O.<br />

obsorvation lightsats equipped with SAR<br />

sensors.<br />

Spacecraft tolocommand must bo oacuro, and<br />

possibly jam-proof, to avoid unauthorizod<br />

entries to the satellite nyntam. Data<br />

encryption must be also implenontrd, in<br />

SpacecraPt telemetry and SAR data<br />

transmission to ground, to prevent<br />

eavesdropping by unauthorized uners.<br />

!<br />

Lightreto in tho 500 to 800 Kg range can<br />

carry CUI nQnaora for high resolution (2<br />

to 3 m), short rovisit interval, tactical<br />

ObQQFJatiOn missions. Medium resolution<br />

(order of 5 m) missions, tor strategic<br />

and, in genaral, international law-<br />

onforcement applications, are also<br />

Poaeiblo. Such spacecraft can form<br />

priaan@nt constellations of, typically, 6<br />

to 8 satallite8 per orbit plane to provide<br />

global cbverage. Multiple orbit planes<br />

constellations can offer enhanced<br />

perfomanbe, allowing also a gradual<br />

system build-up. Smaller constellations<br />

of 4 to 6 spacecraft -can be alno<br />

implernentgd to cover a narrower latitude<br />

belt akound the equator, while<br />

eignif icahtly Improving the average<br />

revisit intervale at sites close to the<br />

orbits inclinations.<br />

In summary, SAR lightsats constellations<br />

can offer certain performance unmatched by<br />

existing, or plarlned, single and larger<br />

observation satellites and can provide a<br />

valuable answer to specific operational<br />

military needs in both tactical and<br />

strategic scenarios. The required<br />

technologies exist, with few exceptions<br />

needing an early in-orbit demonstration of<br />

d@vices being now developed. Nevertheless,<br />

advances in few fields wili certainly<br />

benrfit future generation lightsats.<br />

REFERENCES<br />

(1) C. Perrotta " SAR sensors on board<br />

small S8tQllitCfJ: problems and<br />

prospectives"; Proceedings of 1991<br />

International Conference on Radar; October<br />

1991, Beijinq, china:<br />

[2] F. Borrini " The Italian approach to<br />

tactical use of space": this Conference: I<br />

[3) G. Perrotta, G. Cirri, G. Matticari "<br />

Eloctric propulsion for liqhtsats: a<br />

review oP applications and advantages":<br />

this Conference:<br />

[4) D. Caeey, J. Way Orbit selection for<br />

the EOS mission and its synergism<br />

implications": IEEE Tranoacticns on<br />

Geoscience $and Remote Sensing: Vol 29 n'<br />

6, NOV. '91.*i<br />

' I<br />

[5] H.J.Schodol,T.Kutscheid I' The X-band<br />

CFRP WaVeqUidQ antenna for the Spaco Radar<br />

Lab.81: ESA Workshop on Antenna Technoloqy,<br />

Nov. 1830. ,,<br />

. ..<br />

\

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