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23-8<br />
tional and storzge capacity aad TM-lwiority<br />
during ground station contact.<br />
4. AOCS BASELINE CONCEPT<br />
In the past SIC design has oftcn been pcrformed<br />
with thc emphasis placed primarily on mecltankid<br />
and structural configurdtion aspccts wit bout taking<br />
into account thc impact on othcr subsystems to the<br />
ncccssary cxtcnt. As far as the AOCS is concer-<br />
ncd. it is of course understood that its SIC intcrnal<br />
and cncrnd communication- and ~CCCSS capahili-<br />
tics can providc the ncccsary flcx&ilitv for adapta-<br />
tions to a givcn environment hut disrccarding<br />
ccrtain demands from thc AOCS on thc S.'C hus<br />
and cquipmrnt configuration would entrain thc<br />
nc+cssiiy to establish a dedicated A( ICS-concept<br />
;ind mnkc ;I special dcsign hir cnch misTicm Ihicc-<br />
live and associatcd payload undcr cliscussion hcrc.<br />
Thc approach outlincd suhscqucntiv .time ,I! rna-<br />
king hcct possiblc usc I)! the inhcrcnt Ilcubilitv<br />
fcaturc\ of thc AOCS for Ihc bcnctit id thc ovcrall<br />
systcm and is c.rpcctcd to rncct thc different mis-<br />
sion rcquircrncnts without rn;ijnr modifications.<br />
tkncral Ccaturcs of the concept in cluestion arc:<br />
a The AOCS shall hc dcsiuncd to incorporatc<br />
scnsor and actuator equipmrn! altcrnalivclv o r<br />
in cornhination as rcquircd to mccr the pointinp<br />
and LOS sthilitv pcrform;incc of labl:: 3 - 1 .<br />
The Data ,Managcmcnt and Ccintrol (DMC)<br />
functions of section 2.3 shall he intcarntcd with<br />
thc AOCS (Intcgratcd Control and Data llrrna-<br />
-<br />
-<br />
pcmcnt System - ICDSI.<br />
Data transmission within :hc SIC shall 1% pcr-<br />
formcd hv mcans of a tiiy.itai scriai iI:ita hus.<br />
HAV and S/W implementation shall bc b:iscd.<br />
Thc capability of pcrforminu ortiit c!orrcctions<br />
shall be prcwidcd.<br />
Payload Ja~a managcrncnt (and prcproccwnc).<br />
which rnav nccesitatc cxtr-mclv high cornputd.<br />
tional and storage efforts is rcpardcd ;IS ;I lark<br />
complctcly scpruatcd from the ICDS.<br />
4.1 Srnsnr Conngumlon<br />
It is undcrstood that the wholc scale id ni. *ssions<br />
under discussioo hcrc cur bc best scmcd. if the<br />
highest pcrformancc attitude mcasurcrncni quipmcnt<br />
is xlcctcd. i.e. prccision star scmors a1.d ratc<br />
inlegratin8 gyros in strapdinvn mdc of opcration.<br />
This will. however. bc thc most cxpcnsive<br />
solution and rcprcuni M ovcrdcsip Cor less omhitious,<br />
e.g. communication applications. Subscqucnt-<br />
i<br />
ly the attempt is made to dcfme a sensor configu-<br />
ration. which could cover dl situations, but incvita-<br />
bly imposes restrictions on the system layout.<br />
It is assumed that TACSATS on request of strate-<br />
gic demands shall operated in bctwcen near polar<br />
(sun synchronous) down to near equatorial low<br />
earth orbits. the sun incidence mgk with rcspect to<br />
thc orbit normal also possibly varying between zero<br />
and M". If it is furthermore iusumcd that thc array<br />
dcsign provides thc double axis orientation capabili-<br />
ty discusscd earlier, an orientation of the solar<br />
array axis of rotation approximately parallcl to the<br />
dircction of motion is favourable (see fig. 4.1-la)<br />
for vcry low altitude orbits (e Soc) km) due to<br />
-<br />
air drag (sce fig. 2.1-3)<br />
if the sun is in 3 region around the normal fo<br />
Ihc orbit planc (say 2 45 dcg)<br />
- hi low inclinations of thc orbit planc w.r.1. thc<br />
cqu;l(Or<br />
An owntation ol thc SA. xis of rotation pcrpcn-<br />
ilicular to thc dircction of S/C motion (parallcl to<br />
the earth surface) is more favourablc (sec fig. 4.1-<br />
Ibl<br />
- for high altitude. high inclination (near polar)<br />
orbits<br />
- lor low sun incidcncc angles w.r.1. the orbit<br />
planc<br />
Thc highest flcxibilitv would bc cnsurcd. if - for<br />
rcspcctivc application orbits - the SIC orientation<br />
w.r.1. flight dircction could be sclcctcd cithcr way<br />
.id thc payload (pointins in nabr dircction) alter-<br />
nativclv rotatcd by 'XI dcgrccs around its line of<br />
si*t in the S/C.<br />
A icasiblc uranpcmcnt of all (optical) ;il!itudc<br />
rnc3surcrncnt cquipmcnt. is schematically indicatcd<br />
in fig. 4.1-2. The S/C axes arc dcnotcd bv x. y, z<br />
(roll. pitch. yaw). whcrc the yaw-axis is always<br />
nadir-pointing. Thc schematic of optical scnsor<br />
;irranpcrncnt on thc S/C body surfacc of fig. 4.1-2<br />
shall not postulate that all scnsors indicatcd hmc to<br />
hc available simultancouslv in thc s;imc S!C. For<br />
ccimmur.ication missions e.g. thc cxpcnsivc sensor is<br />
not rcquircd. in hi@ performance missions with<br />
stcllar-incrtial rcfcrcncc on the other hand thc IRS<br />
is obsolctc.<br />
Thc conical scan IRS points 'into S/C y-direction<br />
(or opposite to it. depending on thc sun incidence<br />
angle w.r.1. the orbit). which is tbc dircction of<br />
motion in fhc CSC of fig. 4.1-la and scans thc earth<br />
undcrneath wdcr 0 JS dcg cone angJe. Thc star<br />
sensor is mounted on the -z face (nwoy from the<br />
earth) inched into the pducction (or opposite IO<br />
it) scanning the sky as the S/C rotates around its X-<br />