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aLRaqy1 rsmnto ,.verviaw<br />

An incrooairvgly important aoqpirawmt<br />

cnnc~rno tho rovimit intorval with which<br />

military rolovant sitae, mat Rxa obaeovdr<br />

typical value14 from few dmyo to ad hourer<br />

apply rsinly to fixed aaoota. Obeorvitq<br />

targeta variable in tino or apcico<br />

requieoo, however, much ohontor raviait<br />

Intorvalo, of the ordm 00 ton houro.<br />

Concariring ground resolutlon, 3 a are<br />

suffictont for detection, In none<br />

cases rocognitIon, of fJeIrQteqliC ally<br />

relevant fixed or low-mobility aoaata.<br />

Tactical applications nead, howewe,<br />

better resolutlons down to 2 tn or leos.<br />

The swath width , or instrntanooub fiold<br />

ol viow, must be commonoureto to tho<br />

thoaton: 20 CO 40 Km , depondlppgl from tho<br />

qround reoolutlon, are likely WQ~UO~. The<br />

swath m0t also be oloctronicnlly<br />

repositioned inside tho acconn anyls,<br />

providiq a high operational Blcnibility<br />

in gaehoring SAR images of aolectodl opots<br />

duriq oatollItee* overpassea. WdQo access<br />

anqlow FAYQ instrumental to :BOCU~B a<br />

covcrsqlo without *holes* and td n1nirsir.e<br />

tho con~utallation*o satellites nunhr.<br />

TIme dalay ninim1ratlon hotwoo; o reqluaet<br />

for dater and its wailability to tho onduser<br />

io of utmoot importance, apclally In<br />

8 taCtaCQl eituetion. Direct aCCOOa to tho<br />

satollitm~, during sites oworpmssca,<br />

followodl by 10~91 dnta fux~ooain9 and<br />

intarprotation by multlple,dmto atatlono<br />

doployed in the theater, pro nom am an<br />

ekfectlve answer to auch nemo.<br />

In a oeacteqic occnario thQK0 in the<br />

additional requirement of tming &$lo to<br />

oboorvo dintant nitan with a ohort<br />

turnaround time. Hclajinq lmegouy data vIa<br />

a Data Walsy Satollite network bn tho most<br />

logical and performant solutlon Ito the<br />

prob lei. 1 .<br />

3LCCNETELUTIONS DESIGN CRITERIA<br />

I<br />

WO must diatinquiah bctvcon syntono aimed<br />

at providing a global Earth covaraqe and<br />

thooo Intendod to covar a narrower<br />

latitude bclt around the equator.<br />

AD a mattor of fact, most Countrloo whera<br />

politicel instability is oxpectm! to occur<br />

also in Pueure are includod in tho SO' U<br />

to 50' 6 latltudo belt: which m y justify<br />

tailored constellations.<br />

3.1. Conetellationn for-qlobal cowsraqw-<br />

I<br />

A modul~lr solution &onsiete in injocting<br />

oquispacod lhqht6atn in olnqie plan0 munoynchronouo<br />

orbitnr the SAR con bo<br />

provided virh just ono or two antmnnem<br />

looking on both sides of tho flight path.<br />

Multipla raguispaced orbital planma Can<br />

cop. with vory stringent reviait Intorval<br />

rof~uirowntm, i.e. less than 12 hours.<br />

3.1.1. Ljalhtbat C-tolkat Iona u m o x<br />

sneonns<br />

The capability of e 6AR to inago tarpot<br />

oreas inaddo a wide oarth strip is<br />

proportional to the a-xoaa an910, dof1n.d<br />

polv tho alninun and rwximrr ole-nadir<br />

nerglleci. TRQ conetol lat ion daml@n -cr'itorib<br />

ohould peoi*ida for a contigypad, iarth<br />

covorag~, wIthIn the above'~on~trhinis. To<br />

thio and, the fundaQental inteeval is<br />

divided into U oubintarvala whose vidth<br />

corraaponde to the SAR antenn8 access<br />

angle projected mto the evator. If the<br />

ainimum and maximum off-nadir anglos<br />

cstiofy tho conotraints of Fig. 3.1.1..<br />

then tho strips accoroiblo to tho U<br />

astellitom vi11 bo contiguous.<br />

FLg. 3.1.1. SYSTEM GEOYETny<br />

right antenna<br />

accoee angle accoee anglo<br />

I i<br />

In ono orbit period, the N satellites vi11<br />

have covor-ed an Earth slico as vide as the<br />

fundamental interval, and the cycle will<br />

repeat providing a continuous Earth<br />

coverage up to a latitude close to the<br />

munsynchronoue orbit inclination.<br />

with tho constraint of keeping ha<br />

rainimum and maximum off-nadir angles close<br />

to 20' and 50' roapaxtlvely, the number of<br />

setallites N depends frota the orbit<br />

altitude and acceoo angle, as shown in<br />

tIp.3.1.2. and Table 1.1.1.<br />

* . . . .<br />

'I * U. .ll.I..ll. .*I.<br />

* .<br />

*. .

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