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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 />
*. .