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MHD Waves in the Solar Atmosphere PDF

530 Pages·2019·5.227 MB·English
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MHDWavesintheSolarAtmosphere This volume presents a full mathematical exposition of the growing field of coronal seis- mologywhichwillproveinvaluableforgraduatestudentsandresearchersalike.Roberts’ detailed and original research draws upon the principles of fluid mechanics and electro- magnetism, as well as observations from the TRACE and SDO spacecraft and key results insolarwavetheory.TheuniquechallengesposedbytheextremeconditionsoftheSun’s atmosphere,whichoftenfrustrateattemptstodevelopacomprehensivetheory,aretackled withrigourandprecision;complexmodelsofsunspots,coronalloopsandprominencesare presented, based on a magnetohydrodynamic (MHD) view of the solar atmosphere, and makinguseofFaraday’sconceptofmagneticfluxtubestoanalyseoscillatoryphenomena. The rapid rate of progress in coronal seismology makes this essential reading for those hopingtogainadeeperunderstandingofthefield. bernard roberts isEmeritusProfessorofSolarMagnetohydrodynamicsattheUni- versity of St Andrews. His important contributions to the field over the past forty years havebeenrecognizedwithanelectiontotheRoyalSocietyofEdinburghin1997,aSaltire Scottish Science Award in 1998, and, in 2010, the Royal Astronomical Society’s presti- giousChapmanMedal,awardedfor‘investigationsofoutstandingmeritinsolar-terrestrial physics’. MHD Waves in the Solar Atmosphere BernardRoberts UniversityofStAndrews,Scotland UniversityPrintingHouse,CambridgeCB28BS,UnitedKingdom OneLibertyPlaza,20thFloor,NewYork,NY10006,USA 477WilliamstownRoad,PortMelbourne,VIC3207,Australia 314–321,3rdFloor,Plot3,SplendorForum,JasolaDistrictCentre,NewDelhi–110025,India 79AnsonRoad,#06–04/06,Singapore079906 CambridgeUniversityPressispartoftheUniversityofCambridge. ItfurtherstheUniversity’smissionbydisseminatingknowledgeinthepursuitof education,learning,andresearchatthehighestinternationallevelsofexcellence. www.cambridge.org Informationonthistitle:www.cambridge.org/9781108427661 DOI:10.1017/9781108613774 ©BernardRoberts2019 Thispublicationisincopyright.Subjecttostatutoryexception andtotheprovisionsofrelevantcollectivelicensingagreements, noreproductionofanypartmaytakeplacewithoutthewritten permissionofCambridgeUniversityPress. Firstpublished2019 PrintedandboundinGreatBritainbyClaysLtd,ElcografS.p.A. AcataloguerecordforthispublicationisavailablefromtheBritishLibrary. LibraryofCongressCataloging-in-PublicationData Names:Roberts,Bernard,1946-author. Title:MHDwavesinthesolaratmosphere/BernardRoberts (UniversityofStAndrews,Scotland). Othertitles:Magnetohydrodynamicwavesinthesolaratmosphere Description:Cambridge;NewYork,NY:CambridgeUniversityPress,2019.| Includesbibliographicalreferencesandindex. Identifiers:LCCN2019002497|ISBN9781108427661(hardback:alk.paper) Subjects:LCSH:Helioseismology.|Magnetohydrodynamicwaves.|Fluid dynamics.|Solaratmosphere.|Electromagnetism. Classification:LCCQB539.I5R632019|DDC523.7/6–dc23 LCrecordavailableathttps://lccn.loc.gov/2019002497 ISBN978-1-108-42766-1Hardback CambridgeUniversityPresshasnoresponsibilityforthepersistenceoraccuracy ofURLsforexternalorthird-partyinternetwebsitesreferredtointhispublication anddoesnotguaranteethatanycontentonsuchwebsitesis,orwillremain, accurateorappropriate. TomywifeMargaretandoursonsAlastair,James,MichaelandRichard. Contents Preface pagexvii 1 GeneralPrinciples 1 1.1 Introduction 1 1.2 AVarietyofPlasmas 3 1.2.1 TheSun 4 1.3 TheMagnetohydrodynamicEquations 7 1.4 SomePropertiesoftheMHDEquations 9 1.4.1 FundamentalSpeeds 10 1.4.2 MagneticFluxTubes 13 1.4.3 TheInductionEquation 14 1.4.4 DiffusionofMagneticField (R (cid:2)1) 17 m 1.4.5 AdvectionofMagneticField(R (cid:3)1) 18 m 1.4.6 Thej×BForce 19 1.4.7 Energetics 21 1.5 AspectsofWavePropagation 22 1.5.1 Linearization 22 1.5.2 FourierRepresentation 23 1.5.3 DispersionRelations,PhaseSpeedandGroupVelocity 24 2 WavesinaUniformMedium 27 2.1 Introduction 27 2.2 WaveEquations 29 2.3 PlaneWaves 33 2.4 SoundWaves 35 2.5 MagnetohydrodynamicWaves 37 2.6 Alfve´nWaves 38 2.6.1 PhaseSpeedandGroupVelocity 38 2.6.2 PerturbationsinanAlfve´nWave 40 2.7 MagnetoacousticWaves 42 2.7.1 DispersionRelation 42 2.7.2 PhaseSpeedDiagrams 45 vii viii Contents 2.7.3 GroupVelocityofMagnetoacousticWaves 46 2.7.4 PerturbationsintheMagnetoacousticWaves 50 2.8 MagnetoacousticWaves:TheSpecialCasec =c 57 A s 2.9 TwoPhysicalExtremes 58 2.9.1 TheIncompressibleFluid 60 2.9.2 Theβ =0Plasma 63 3 MagneticallyStructuredAtmospheres 66 3.1 Introduction 66 3.1.1 WaveEquations 67 3.1.2 SoundWaves 70 3.1.3 TheAlfve´nWave 71 3.2 MagnetohydrodynamicWaves:CartesianSystem 71 3.2.1 UniformMedium 73 3.2.2 TheCasek =0 74 y 3.3 MagnetohydrodynamicWaves:CylindricalGeometrySystem 75 3.4 Singularities 77 3.5 PhaseMixingoftheAlfve´nWave 78 3.6 TwoSpecialCases 79 3.6.1 TheIncompressiblePlasma 80 3.6.2 Theβ =0Plasma 80 4 SurfaceWaves 83 4.1 Introduction 83 4.2 ParallelPropagation 85 4.2.1 BoundaryConditionsatanInterface 86 4.3 TheSurfaceWaveDispersionRelation 87 4.3.1 The Hydromagnetic Surface Wave of an Incompressible Medium 89 4.3.2 SurfaceWavesonaMagnetic–Non-MagneticInterface 89 4.3.3 Theβ =0Medium 93 4.3.4 PropertiesofSurfaceWaves 94 4.4 Non-ParallelPropagation 95 4.4.1 TheIncompressibleCase 97 4.4.2 Theβ =0Plasma 98 4.5 ResonantAbsorptionataSingleInterface:TheIncompressibleCase 99 5 MagneticSlabs 102 5.1 Introduction 102 5.2 TheIncompressibleCase:HydromagneticSurfaceWavesinaSlab 103 5.2.1 SausageandKinkModes 106 5.2.2 DispersionRelations 107 5.2.3 PressureandLongitudinalMotion 110 5.3 CompressibleEffects 113 5.4 TheIsolatedMagneticSlab 119

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