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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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