OrbitalPropagation:PartII
轨道外推:第二部分
Inourlastcolumn,wecoveredthebasicsofmodelingastheyapplytopredictingthepositionof
anymodel,thecomplexityoftheorbitalmodelwechoo
dependsuponveralfactors,chiefamongthebeingtheaccuracyofthedesiredpredictions.
Atthesametime,sincewewillbecalculatingpredictionsfromthisorbitalmodelonacomputer,
unately,the
twogoalsconflict,sowewillekamodelwhichstrikesanappropriatebalancebetweenthe
model'sfidelity(accuracy)andthecomputationalburdenofproducingaprediction.
Inordertoobtaintheappropriatelevelofmodelfidelity,itwillbenecessarytodeterminethe
orbitalmodel,the
includethegravityoftheearthalongwithperturbationsduetothenonuniformmass
distributionoftheearth,gravitationalattractionofthesun,moon,andplanets,andatmospheric
ftheforcesaremostimportantwilldependnotonlyontheirrelativemagnitude
butuponwhethertheireffectsareperiodicorcular.
Aperiodiceffect,suchasyourcar'santennawhippingbackandforthasyoudrivedowntheroad,
haslittleeffectonthepositionofthetipoftheantennaovertime,eventhoughtheforces
nlyneedtoknowthepositionoftheantennatiptowithin
onemeter,r,aculareffect,onewhichconsistently
increasordecreasovertime,mayhaveaconsiderableeffecteventhoughtheforceinvolved
pleofaculareffectwouldbethatofalightwindblowingasailboat
acrossthewater.
Asfarascomputationalcomplexityisconcerned,wenotedatthecloofthelastcolumnthat
therto
startwithasatellite'spositionandvelocityandtosum,orintegrate,alloftheforcesactingon
talforceisassumedtoactonthesatelliteoversomesmalltimespan,atthe
endof
implementedonacomputer,antageof
thisapproachisthatifsufficientdetailisgiventotheforcesactinguponthesatelliteandsmall
enoughtimestepsareud,nsideto
numericalintegrationisthatwemustcalculatethesatellite'spositionandvelocityforeachtime
stepbetweenourknowninitialconditionsandourdesiredpredictiontime.
Dependinguponthesizeofthetimestepandthelengthofthetimeinterval,thecomputational
,multiplythisproblembytheapproximately
7,500objectscurrentlytrackedbyNORAD(theNorthAmericanAerospaceDefenCommand)
andyou'dprefertohaveamodel
whichprovidesananalyticalsolution,thatis,asolutionwhereinifweknowthetimeofinterest
wecandirectlycalculatethestateofthesatellite'sorbitatthattimewithouttheneedto'step'
ourcondcomputationalmethodofimplementinganorbitalmodel.
Duringthe1970s,NORADcameupwithjustsuchasolution:
thismodel,knownasSGP(forSimplifiedGeneralPerturbation),aurcancalculateasatellite's
positionandvelocityataparticulartimedirectly,
resultisaconsiderablereductionincomputationalburdentosupporttrackingthegrowing
populationofearth-orbitingsatellites.
Obviously,anymodel,
certainsimplificationshadtobemadeandthesimplificationsplacerestrictionsuponhowthe
icular,themassofthesatelliterelativetothemassoftheearthis
tion,thesatelliteisassumedtobeinalow-eccentricity,
onditionsweretrueforalarge
percentageofthesatellitepopulationatthetimeSGPwasdevelopedandallowedamodeltobe
formulatedaccountingonlyfortheprimaryperturbationsonthesatellitesduetotheearth's
nonuniformmassdistributionandatmosphericdrag.
SubquentrefinementstoSGPextendedthistheorytoincludeami-analytictreatmentof
histheorydoesdependtosomeextent
uponnumericalintegration,akat
225minutes(about6,000kmaltitude)istheresultofasomewhatnaturalgapwhichhasresulted
fromhistoricalchoicesoforbitsforvarioussatellitemissionsandacrossoverinsignificant
perturbingeffects;abovethegaptheprimaryperturbingforcesarenolongeratmosphericdrag
andtheearth'snonuniformdensity,butorbitalresonanceswiththeearth'snonuniform
gravitationalfield,solarandlunargravitationalforces,w
modelisreferredtoasSGP4andisthemodelcurrentlyinubyNORADandtheUnitedStated
SpaceCommand.
Youmaybewondering,atthispoint,nly,there
aremanyothermodels,4hasonething
goingforitthatnoneoftheothersdo:iketheadventofautomobilesrunningon
unleadedgasoline,itdidn'tmakeanydifferencehowslickanewcaryouhadifyoucouldn'tfind
herorbitalmodelsonlyprovidedataforalimitednumberofsatellites
(suchasthespaceshuttle).NORAD,ontheotherhand,isresponsiblefortrackingallsatelliteson
ansthatorbitaldataforthismodelisavailable
forallearth-orbitingobjectscapableofbeingtrackedbytheUSSpaceSurveillanceNetwork.
Butwe''tallorbitalelementts
alike?Afterall,theyallmeasurethingslikeinclinationandmi-majoraxis(termswe'lldefine
furtherinafuturecolumn)'tItaketheNORADelements
andutheminmyfavoritetrackingprogram(whichdoesn'tutheSGP4model)?Allowmeto
uacomputeranalogyheretoexplain.
ryouknowthem
bytheirformalnames,suchasrun-lengthencoding,HuffmanorLZWcompression,orbythe
termsudbysomeofthepopulararchivingpackages,suchassqueezing,imploding,crushing,
orthelike,youwouldn'tbetoohappywiththeresultifsomeonentyoudatacompresdby
,yoursoftwarewouldprobably
reportanerror,butthat'resultwillbethesame:errors.
Thetwo-lineorbitalelementtsmadeavailablebyNORAD(andredistributedbyNASA)are
nvaluesforeachelementaregeneratedusingthe
ectsofthemajorperturbingforcesareincorporatedintothemean
valuesinaveryspecificwayusingSGP4andSGP4mustbeudtogenerateaccuratepredictions.
Failuretodosowillresultinerrors,themagnitudeofwhichwilldependheavilyonthetypeof
rrorsaretypicallymanifestedaslargetimeerrorsinsatellitesignal
orvisualacquisitionorbeingunabletolocatethesatelliteatall.
youwouldn'texpectto
ension,theonlydata
distributom
othersourcesshouldneverbereformattedintothetwo-lineformatjustsoitcanbefedintoa
particularsoftwarepackageunlessyoudon'tcareabouttheaccuracyoftheresults(justasyou
wouldn'tsoyoucoulduPKUNZIP).
Manypopularcommercial,shareware,andpublicdomainsatellitetrackingpackagesimplement
SGP4andyousho
,ifyouareconcernedaboutthe
sourceofyourdata,pdatesofNORAD-generated
two-lineorbitalelementtsareavailableviaInternet(anonymousftp,gopher,ormosaic)on
hedirectorypub/spaceorontheCelestialBBSat205/409-9280[Neitherof
nnowbefoundonlyontheCelesTrakWWWsite.].
Bothrvicesareavailablefreeofchargetoallurs.
Inournextcolumn,wewillexplorehowtheNORADtwo-lineelementtsaregeneratedand
givesomenumericalexamplestoillustratethemagnitudeoftheerrorswhichcanresultfrom
orwardtoeingyouherenexttime!
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