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23-2<br />
.<br />
- missile wnrninq, e.g. against tactical h\Iistic<br />
missilcs, to possibly improve thc cfficicncy of<br />
dcfcnsivc actions<br />
- nnviir.ntion_ to contributc to thc provision of<br />
-<br />
highly accuratc navigation data<br />
ohscrvntion. survcillans and verificatinn, c.5. to<br />
chcck disllrmamcnt trcaty tiolation or - in a<br />
battlc ficld sccnario - to monitor [orcc dcploy-<br />
mcnts and to provide target rccognition. tbcatcr<br />
targctins and vcrification<br />
As a conscqucncc of thc gcncral mission objcctivcs<br />
oiillincd abovc, opcratiod rind performancc rc-<br />
quircrncnts. cncironnrcntal conditions and son-<br />
straints arc imposcd on thc Attitude- and Orbit<br />
Control Systcm. which arc subscqucntlv outlincd to<br />
establish thc gcncral framc for thc AOCS.<br />
2.1 hllssinn rind Faylaad Kcquiremcnls<br />
For varinus rcisons likc launch cost. in;m in orbit.<br />
imasc rcsolution or powcr rixpircmcnls of obscrvntion<br />
payloads thc spacecraft undcr discussion<br />
will hc injcctcd into rclativciy low cnrth orbits<br />
(about 300 to 1Mn) km). In gcncrd near pol;ir. sunsynchronous.<br />
cirulw orbits arc prcfcrrcd, which arc<br />
charactcrizcd by thc condition that lhc .product of<br />
three orhit paramctcrs, i.e. orbit scmi-mnjor ;~l(is.<br />
cxccntricity, and inclination has a spccific numcri.<br />
cal vduc. cntrining thc orbit node to rotatc t\ith<br />
onc rcvolution pcr ycar. For optical obscwation<br />
pavlaods "dawn orbits' arc particularly suited. In<br />
this casc the S/C will always view thc surfacc of thc<br />
carth at any given latitud: at thc siunc local time<br />
(sce e.g. rcf. 1, p. 68). A graphical rcprcscntation<br />
of thc orbit pararnetcrs 'inclination" (in dcg.), rhc<br />
"orbit pcriod" (in minutcs) ;ind thc "SIC velocity"<br />
.(in rnfscc) as a function of altitudc (in km) for<br />
circular sun synchronous orbi~s is givcn in ligs.<br />
2.1-la to 2.1-lc of Anncx I. r,:spectivcly.<br />
For such orbits thc revisit period of spccihc tcrrc.<br />
strial locations in equatorial regions or ot law earth<br />
latitude for ;I sin& S/C m;iv bc unaccctahlv long<br />
for tactical earth obscrvation rcquircmcnts. whcrcas<br />
the rcvisit pcriod in mostly unintcrcstiny polar<br />
regions in principle equals thc orbit rcvoltltion<br />
pcriod. This situation can tic improved as follows:<br />
- For obscrvation of a particular re+n on earth<br />
the SIC is launched into n dcdicatcd orbit. thc<br />
revohtion period of which is an intcgcr fraction<br />
of 24 hours. Thc revisit limc will then bc at<br />
lcasl mcc or cven scvcral limes a clay. For in-<br />
stance (ref. figs. 2.1-la and -1b) a satcllitc in<br />
-<br />
sun-synchronous orbit of (about) 570 km altitudc<br />
and 97.6 dcg inclination will have an orbit pe-<br />
riod of 96 min aid p~ over the same area<br />
cvcry 15'" revolution. 16 orbits per 24 h (orbit<br />
period ol M mh) would cvcn allow to revisit the<br />
same targct cvcry 12 hours (in thc descending<br />
N/S and ascending SM orbit crossing) but rcqui-<br />
re an altitudc of 275 km (inclination 96.56 dcg)<br />
and the S/C would experience sigificant air<br />
drag as wil? bc discussed latcr (fig. 2.1-3, AMCX<br />
1).<br />
A numbcr of payloads can provide large ranges<br />
of "sidc looking" capability, cnabliag observation<br />
of a local arc3 undcr different aspect angles in<br />
succcssivc orbits. Exccpt when phased am/<br />
antcnnas arc crnploycd this generally rcquircs<br />
nicch;inical slcwing of optics, mirrors ;rnd/or<br />
rcflcctors and in turn inay givcn risc to sipifi-<br />
cm intcrnnl torques and associated attitude<br />
pcrturb;itiocs.<br />
- Selection of low inclination orbits instead of<br />
quasi-polar orbits with inclination angles covc-<br />
ring the rqc of gcographical latitude of parti-<br />
-<br />
cular intcrcst.<br />
Pkicing ii sufficicnt numbcr of satcuitcs into<br />
appropriatcly inclined. mutually synchronizcd<br />
orbit to cnsurc r,hc dcsircd covcragc probability.<br />
Thc rchtionship lictwccn thc numbcr of satcllitcs<br />
rccjuircd to cnsurc continuous coveragc from any<br />
point on thc carrrh undcr a local elcvatim andc of<br />
at Icast IO dcg as a function of circular orhit dtitu-<br />
dc is shown in fig. 2.1-2 (rcf. 2 ) of Anncx 1. Pro-<br />
per sclcction of orbit inclin:ition and phasing of thc<br />
cirbitiny satcllitcs is rcquircd. Particular cxamplcs of<br />
Low Earth Orbit (LEO) Communication Satcllitc<br />
Systems c.g. MOTOROLNIRIDIUM or TRW-<br />
ODYSSEY rcquiriny 77/19, satellites at 735/10350<br />
km dtitudc arc schematically indicated in this hgu-<br />
rc. Thc numbcr of satcllitcs Jccrcascs, of course if<br />
poliir covcraqr is not rcquircd. In any casc orbit<br />
inclination ;ind phasing of individual SIC forming<br />
p;irt of a satellite syctcm hnvc to bc rclaincd or<br />
respectively corrcctcd in c;rsc of dcvintions from<br />
nominal during opcrational lirc timc.<br />
For thc asscssmcnt of the amount (m,) of rnono-<br />
propellant hydrazinc rcquircd to maintain a circular<br />
orbit of givcn, rclativcly low altitudc, rcfcrcncc is<br />
made to Eg. 2.1-3 (Anncx l), where thc drag factor<br />
(9 pcr day (d) and unit cross-sclcctional iirca (0)<br />
of thc S/C is plottcd. The propellant mass is thcn<br />
givcn by