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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

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