ebook img

Chemical and physical properties of the OH, CN and C2 jets in Comet Hale Bopp (1995 O1) PDF

171 Pages·2000·6.8 MB·English
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview Chemical and physical properties of the OH, CN and C2 jets in Comet Hale Bopp (1995 O1)

THECHEMICALANDPHYSICALPROPERTIES OCFOTMHEETOHH,ALCEN-BAONPDPC(219J9E5T0S1)IN By SUSANMARIALEDERER ADISSERTATIONPRESENTEDTOTHEGRADUATESCHOOL OFTHEUNIVERSITYOFFLORIDAINPARTIALFULFILLMENT OFTHEREQUIREMENTSFORTHEDEGREEOF DOCTOROFPHILOSOPHY UNIVERSITYOFFLORIDA 2000 Copyright2000 hv SusanMariaLederer Thisisdedicatedtomyfamily,whohassupportedmeduringeverystepof myeducationandmylife. ACKNOWLEDGEMENTS MysincerestthanksgotoDr. HumbertoCampinswhoagreedtoadviseme evenwhenhisschedulewasquitefull,andwhocontinuedhisroleasmyadvisorlong afterhiscommitmentstoUFhadpassed. Hetaughtmetothinkasanindependent scientist, yet guided me and encouraged me through the difficult times. He has remainedanactive,committedadvisorinmyresearch, andhisguidancehasbeen invaluable. IwouldalsoliketothankDrs. DavidSchleicher, DavidOsip, Michael A'Hearn,andStephenLarsonfortheirguidanceinobservationalastronomy,cometary science, andmyresearchproject. Myresearchwouldnothaveprogressedwithout theinputofallthesepeople. Iwouldliketothankmycommitteemembers,Drs. ElizabethLada,Richard Elston, StanleyDermott, andMartinVala. IparticularlythankDr. Ladaforher helpasmypseudo-advisorinDr. Campin'sabsence,Dr. Valawhoagreedtositon mycommitteeonlymonthsbeforemyfinaldefense,andDr. JonathanWilliamswho agreedtositinonmydefenseforDr. Ladawithlessthanaweek'snotice. IwouldalsoliketothankDr. CaseyLissewhowasalwayswillingtodiscuss myresearch, andwhospentmanyhoursfillingmythesiswithredinktoimprove itscontents. IwishtothankDrs. AmyLovellandNalinSamarasinhaforhelpful discussionsandtheirwillingnesstosharepiecesoftheirMonteCarlocodes. Ialso thankJeffJulianforhisamazingabilitytocreate3Dfigures,andforhiswillingness tohelpinanywayatamoment'snotice. Dr. LarryWasserman(LowellObservatory) alsodeservescreditforhelpingmesolvenever-before-seenproblemswhileobserving at 3 a.m. I alsothank him forsharinghis ephemerides program and alteringit togenerateadditionalinformationthatwascrucialtomyMonteCarloroutines. I IV wouldalsoliketoexpressmyappreciationforAmyNewberry, whoseexpertisein theEnglishlanguagehelpedimprovenotonlythegrammar,butalsocutdownthe infinitenumberofcommasscatteredthroughthisthesis. Any acknowledgement would be incomplete without mention ofall ofthe peopleat the University ofFlorida. Thanks tothededication ofouroffice staff, includingGlenda,Ann,AudreyandDebra-Iwasalwaysregisteredforclasseson time,wasalwayspaid,andwasabletotraveltodistantlands(andnot-so-distant lands). Myofficemates,Scott,James,Jim,andElisha,madethelonghoursinthe spacesciencesbuildingenjoyablewithenlighteningconversationsrangingfromGator footballtothepossibilityoflifeexistingintheuniverse,andeverythinginbetween. Icannotbegintolistallthefriendswhohavegivenmesupportthroughout thisthesis. I amverygratefulforDavid, Teresa, Alexesand KrystinaCiardifor makingmepartoftheirfamily,alwayskeepingthedooropenforme, andfeeding memanyhealthymealsthroughoutthelasttwoyears. IthankJoannaLevinefor manystress-relievingmochabreaks. Iamalsoindebtedtothemanyfriendswho havecontinuouslyencouragedmefromafar,includingBobThompson,SeanPowell, SheilaSnow,JamieBallard,andMelissaBenedict. Thislistwouldnotbecomplete withoutmentioningBarbColba(myfavoriteteacher),whotaughtmethatlearning wasfunandschoolwascoolattheripeoldageof5,andcontinuestosupportme fromafareventoday. Iamdeeplygratefulformyextendedfamilywhosupportedmethroughout myentireeducation. Ithankmyfather, Ken,andmother, Kath (whosespiritwill alwaysbewithme),forencouragingmetolearnfromchildhoodthroughgraduate school. Theywillalwaysbeclosefriendsaswellasparents. Iparticularlythankmy dadforencouragingmetofollowmyinsatiablecuriosityaboutthephysicalworld and heavens andentertheworldofresearch. Heknew Iwould be happiest in a professionwherelearningneverends. Mymomtaughtmethatexcellingtobeyour best is always the most rewarding, despite peer pressure. She was always there withacomfortinghugorsmile,despitethedifficulties. Ithankmysister,Jennifer, forplayingtheroleofconfidant,ineveryrespect,throughoutmylifeandoftenafter midnight;mybrother,Matthew,forchallengingmetothinkandgrow;andmysister, Katie,forheropennessinlifeandherenvelopinghugs. Iwouldalsoliketothank LouforshowingmesupportwhenIbarelyknewhim,andforemanatingapassion forlifethathasinfluencedusall. IalsowishtoexpressmygratitudetomyActive family,Karin,Dave,Katie,Ben,andMeghanOlson,whohasbeenmysecondfamily throughoutmyentirelife. Ialsowishtothankmyparents; grandparents, Walter SchneiderandMaryLederer;andmyauntanduncle,RuthandDeanTwedt-their generosityandsupportallowedmetogainthefullesteducationpossible. Without them,I'msuremyeducationalendevourswouldhavelastedyearslonger. Finally,I wishtothankDavidSchwenkforhisinfinitepatiencethroughoutthefinalstagesof mydissertation;forhissupportofmyworkandmylife;andforhisinfectioussmile, energy,andlove. Thesearethepeoplewhohelpedmemaintainmysanityanddrive, andtowhomIwillalwaysbeindebted. VI TABLEOFCONTENTS ACKNOWLEDGEMENTS iv LISTOFTABLES ix LISTOFFIGURES x ABSTRACT xii CHAPTERS 1 INTRODUCTION 1 1.1 TheOortCloudandKuiperBelt 5 1.2 PropertiesoftheComa 5 1.2.1 CometaryJets 6 1.2.2 CometHale-Bopp 8 1.2.3 OHasaTracerofH2 10 1.2.4 JetSource: GasorGrain? 12 1.3 Synopsis 14 2 OBSERVATIONSANDDATAREDUCTION 15 2.1 FacilitiesandInstrumentation 15 2.2 DataReduction 16 2.2.1 InitialDataReduction 16 2.2.2 AbsoluteCalibration 23 2.2.3 ImageProcessingandEnhancementRoutines 25 2.3 ProjectedExpansionVelocities 26 2.4 Summary 30 3 MONTECARLOMODELING 31 3.1 Introduction 31 3.1.1 HaserModel 32 3.1.2 VectorialModel 32 3.1.3 HydrodynamicModels 33 3.1.4 MonteCarloModel 34 3.2 MonteCarloModelsDevelopedforThisWork 34 3.2.1 GasSourceVersusGrainSource 35 3.2.2 Non-collisionalIsotropicModel 36 3.2.3 Collisions 40 3.2.4 CollisionalJetModels 47 vn 3.3 Summary 50 4 ANALYSISANDDISCUSSION 53 4.1 Introduction 53 4.2 DataAnalysis 54 4.2.1 JetIdentification 54 4.2.2 ComparingtheMorphologyofOH,CN,andC2 62 4.2.3 JetWidths 67 4.2.4 EvolutionoftheJetswithTime 68 4.3 MonteCarloModelAnalysis 70 4.3.1 GasversusCHONGrainSource 73 4.3.2 InitialParentVelocityandAlphaParameter 83 4.3.3 RangeofInitialParentVelocities 86 4.3.4 DaughterVelocity 86 4.3.5 LifetimesofParentandDaughter 89 4.3.6 RadiationPressure 94 44..33..87 NPhuamsbeerAngalned,PPoAsistuino,nSsuonf'sthCeomAcettiovceenAtrreiacsLocation.... 9948 4.3.9 OpeningAngleoftheActiveAreas 101 4.3.10 StrengthoftheJetsandSolarInsolation 102 4.4 Results 103 4.4.1 ExpansionVelocitiesandJetWidths 103 44..44..23 PJertojSeocutrecde:LoGcaastivosnsGrofaiAnctiveAreasontheNucleus . . . 111067 4.5 Discussion 129 4.5.1 Morphology 129 4.5.2 EffectonProductionRates 132 4.5.3 Compositionofthenucleusandextendedsource 133 4.5.4 ImplicationsfortheHeterogeneityoftheNucleus 134 4.6 Summary 136 5 CONCLUSIONS 137 5.1 Introduction 137 5.2 NewResults 138 5.3 DirectionsforFutureWork 140 APPENDIXES A DUSTPRODUCTION(A/p) 143 B THEHASERMODEL 145 REFERENCES 147 BIOGRAPHICALSKETCH 155 Vlll LISTOFTABLES 1-1 Branchingratiosofwater 11 2-1 Narrowbandfiltercharacteristics 17 2-2 CometHale-Boppobservingdetails 17 3-1 MonteCarlomodelparameterspace 38 3-2 Collisionalcrosssections 46 4-1 Species-dependentmodelinputparameters 72 4-2 Modelinputparameters 72 4-3 Projectedexpansionvelocities 104 4-4 Projectedjetwidths 107 4-5 Locationsofmodelactiveareas 109 4-6 Hasermodelproductionrates 134 IX LISTOFFIGURES 2-1 Marchtimesequence 28 3-1 MonteCarlomodel: Collisionalandnon-collisionalmodels 48 3-2 Radialprofilesofdataandbest-fitmodels(April26,1997) 51 4-1 OH,CN,andC2data(March6,1997) 55 4-2 OH,CN,andC2data(April26,1997) 56 4-3 OHdatawithvariousimageprocessingtechniquesapplied 58 4-4 CNdatawithvariousimageprocessingtechniquesapplied 59 4-5 C2datawithvariousimageprocessingtechniquesapplied 60 4-6 Continuumdatawithvariousimageprocessingtechniquesapplied . . 61 4-7 Gasimagesbeforeandaftercontinuumcorrection(March6,1997) . . 63 4-8 Gasimagesbeforeandaftercontinuumcorrection(April26,1997) . . 64 4-9 CNcontinuumcontaminationanalysis 66 4-10 Radialprofileofjets 69 4-11 OHdataandmodelswithgasandtriangularCHONgrainjetsources 74 4-12 CNdataandmodelswithgasandtriangularCHONgrainjetsources 75 4-13 C2dataandmodelswithgasandtriangularCHONgrainjetsource . 76 4-14 Radialprofilesofthedataandbest-fitmodelsforallgasspecies ... 77 4-15 RadialprofilesofOHdataandmodelsinthesunwarddirection ... 78 4-16 RadialprofilesofOHdataandmodelsintheanti-sunwarddirection . 79 4-17 RadialprofilesofCNdataandmodelsinthesunwarddirection ... 80 x

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.