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Astrophysics and Space Science Proceedings The Cluster Active Archive Studying the Earth’s Space Plasma Environment Harri Laakso Editor ESA/ESTEC,Noordwijk,TheNetherlands Matthew G.T.T. Taylor Editor ESA/ESTEC,Noordwijk,TheNetherlands C. Philippe Escoubet Editor ESA/ESTEC,Noordwijk,TheNetherlands 123 Editors Dr.HarriLaakso Dr.C.PhilippeEscoubet EuropeanSpaceAgency EuropeanSpaceAgency EuropeanSpaceResearch&Technology EuropeanSpaceResearch&Technology Centre(ESTEC) Centre(ESTEC) Keplerlaan1 Keplerlaan1 2200AGNoordwijk 2200AGNoordwijk Netherlands Netherlands [email protected] [email protected] Dr.MatthewTaylor EuropeanSpaceAgency EuropeanSpaceResearch&Technology Centre(ESTEC) Keplerlaan1 2200AGNoordwijk Netherlands [email protected] ISSN1570-6591 e-ISSN1570-6605 ISBN978-90-481-3498-4 e-ISBN978-90-481-3499-1 DOI10.1007/978-90-481-3499-1 SpringerDordrechtHeidelbergLondonNewYork LibraryofCongressControlNumber:2009934513 (cid:176)c SpringerScience+BusinessMediaB.V.2010 Nopartofthisworkmaybereproduced,storedinaretrievalsystem,ortransmittedinanyformorby anymeans,electronic,mechanical,photocopying,microfilming,recordingorotherwise,withoutwritten permissionfromthePublisher,withtheexceptionofanymaterialsuppliedspecificallyforthepurpose ofbeingenteredandexecutedonacomputersystem,forexclusiveusebythepurchaserofthework. Coverdesign:eStudioCalamarS.L. Printedonacid-freepaper SpringerispartofSpringerScience+BusinessMedia(www.springer.com) Preface Magnetospheric physics started more than 50 years ago when many of the first satellites carried detectors to explore the space environmentaround the Earth and made plenty of new discoveries. The first findings inspired the development of a plethoraof scientific satellites in the1960sand 1970sexploringnear-Earthspace, whichwasfoundtohaveseveraldistinctregionswiththeirownstructuralanddy- namicalcharacteristics. Since then magnetosphericphysicshas remained a strong space science discipline, not only for its own sake but also because near-Earth space providesus with a unique space laboratory where we can investigate phys- ical processes of tenuouscollisionless plasmas with in-situ instruments and apply the resulting understandingto physical phenomenaobserved in more exotic envi- ronmentsoftheSolarSystemandoftheUniverse. Forlongtimemagnetosphericresearchwascarriedoutonlybymeansofsingle spacecraft.Inthe1970sthesciencecommunityrealizedthatoneneedscoordinated simultaneousobservationsfromseveralsatellitesinordertomakeamajorstepfor- ward in magnetospheric and space plasma physics. In particular the ISEE (three satellites), GEOS(twosatellites) andDE(two satellites) programsprovidedmany newdiscoveriesthatsinglespacecraftmeasurementscouldnotachieve.Inparticular itwasthedualspacecraftconstellationofISEE-1andISEE-2thatofferedthefirst opportunity to improve the understanding of spatio-temporal features in physical processes of space environmentwhile the other previousmissions were separated byverylargedistancesandwereondifferentorbits,soonecouldnotseparatespatial andtemporalfeatures. Inearly1980sthesciencecommunitystarteddreamingaboutthenextgeneration ofmulti-satelliteconstellationmission,theculminationofwhichcamein1982when agroupofscientistsproposedafour-satellitemission,calledCluster,toESA.After theassessmentstudies,theClustermission,togetherwiththeSOHOmission,were selected as the first cornerstone of the ESA’s Horizons2000 Programmein 1986. Unfortunately,after 10yearsof hardworktheCluster satellites were dramatically destroyedbythe failureof thefirst flightof Ariane5 on4 June1996.However,it wasdecidedsoonafterthatthemissionwasofsuchhighimportancetothescience communitythatthesatellitesandpayloadmustberebuilt,and4yearslaterthefour ClusterspacecraftweresuccessfullylaunchedinpairsontwoSoyuzrocketsinJuly andAugust2000.After1yearofsuccessfuloperations,themissionwasextended v vi Preface for an additional35 months, up to December 2005.Later the mission was further extendedfor4yearsuntiltheendof2009,andanewextensionproposalhasbeen submittedtorequestfurtheroperationsbeyond2009. Duringthefirstextension,ESAdecidedtoestablishtheClusterActiveArchive (CAA)tocontainallprocessedandvalidatedhigh-resolutionscientificdata,aswell as raw data, calibration data and documentation from all the Cluster instruments. ThisisessentialinordertopreserveallClusterobservationsinastable,long-term archiveforscientificanalysiswellbeyondtheendofthemission.TheCAAactivi- tiesstartedin2004and2yearslaterinFebruary2006,theCAAopenedservicesto thecommunity. TheClustermissionhasheldscienceworkshopstwiceayearsinceautumn2001, whichhashelpedbringtogetherscientiststocompareandexchangetheirobserva- tions and begin new collaborations. Before the CAA, scientists got access to the ClusterobservationsviatheirpersonalcontactswiththeinstrumentPrincipalInves- tigatorsandCo-Investigators.Nowandinthefuture,theCAAprovidestheprimary access route to the Cluster observations.Soon after the CAA openingit was real- ized thatwhile someof the Cluster datasets are quiteeasy to use, thereare plenty ofcomplexdatasetswhoseusagemaynotalwaysbeobvious.Thereforeitwasde- cidedtoorganizeaschoolfortheusersoftheCAAdatasets,whichwasorganized togetherwiththe15thClusterscienceworkshopinordertoattractasmanyusersas possible.ThedetailsofthisandotherworkshopscanbefoundattheCAAwebsite http://caa.estec.esa.int/. The15thCluster workshop,attendedby(cid:2)120people,washeldin HotelPlaya la Arena (Puerto Santiago), Tenerife, Canary Islands, on 9–15 March 2008. The workshopprovidedtheattendingcommunitywithanin-depthoverviewoftheCAA data products and tools. In addition, attendees were able to discuss with instru- ment team developers, the core CAA team and software developers. The packed scheduleincludedpresentationsofinstrumentdatasets,softwaretoolsandtheCAA infrastructureandwasinterspersedwithinvitedscientifictalksandseveraldedicated sciencesessionsonthebowshock,solarwind,magnetopauseandcusp,themagne- totailandinnermagnetosphere.Thefactthattheworkshop/schoolwashostedinthe samelocationastheaccommodationwasfundamentalinthesuccessofthemeeting, allowingattendeestocontinueworkingwithcolleaguesanddiscussingworkinand aroundtheworkshophours. This bookcontainspresentationsmade at the workshop,includingseveral arti- clesabouttheCAAanditsdatasetsaswellasafewoverviewpapersontheCluster mission. In addition all participants were offered an opportunity to publish their scientificresultsonsolarwind/magnetosheath,magnetopause,andmagnetotail,pre- sentedduringtheworkshopinthisbook. Wewouldliketothankthefollowingpeoplefortheircontributionsinreviewing the articles in this book: O. Alexandrova, A. Allen, M. Andre´, T. Asikainen, A. A˚snes, R. Benson, J. Blecki, J. Borovsky, D. Burgess, J. Cao, N. Cornilleau- Wehrlin, P. Daly, I. Dandouras, J. Davies, M. Dunlop, J. Eastwood, S. Elkington, A. Eriksson, J. Faden, A. Fazakerley, J. Fennell, R. Friedel, T. Fritz, S. Fung, E. Gamby, V. Ge´not, M. Goldstein, E. Grigorenko, B. Grison, M. Hapgood, Preface vii C.Harvey,R.Horne,C.Jacquey,Y.Khotyaintsev,L.Kistler,H.Kucharek,G.Le, E.Lucek,J.McFadden,S.Milan,F.Mozer,J.Mukherjee,H.Opgenoorth,C.Owen, G. Parks, M. Parrot, A. Pedersen, C. Perry, J. Pickett, P. Puhl-Quinn, J. Rae, J.L. Rauch, A. Retino, A. Roux, V. Sergeev, A. Tjulin, K. Torkar, K. Trattner, A.Walsh,Y.Wang,J.Weygand,J.Wild,andQ.Zong. May2009 HarriLaakso,MatthewG.T.TTaylor,andPhilippeEscoubet ViewontheTenerifeIsland Contents Preface............................................................................... v PartI ProductsandServicesoftheClusterActiveArchive 1 ClusterActiveArchive:Overview.......................................... 3 H.Laakso,C.Perry,S.McCaffrey,D.Herment,A.J.Allen, C.C.Harvey,C.P.Escoubet,C.Gruenberger,M.G.G.T.Taylor, andR.Turner 2 ASPOCDataProductsintheClusterActiveArchive.................... 39 K.TorkarandH.Jeszenszky 3 ClusterIonSpectrometry(CIS)DataintheClusterActive Archive(CAA)................................................................ 51 I.Dandouras,A.Barthe,E.Penou,S.Brunato,H.Re`me, L.M. Kistler, M.B. Bavassano-Cattaneo, A. Blagau, andtheCISTeam 4 DigitalWaveProcessorProductsintheClusterActive Archive......................................................................... 73 K.H. Yearby, H.St.C. Alleyne, S.N. Walker, I. Bates, M.P.Gough,A.Buckley,andT.D.Carozzi 5 EDIDataProductsintheClusterActiveArchive ........................ 83 E.Georgescu,P.Puhl-Quinn,H.Vaith,M.Chutter,J.Quinn, G.Paschmann,andR.Torbert 6 TheEFWDataintheCAA.................................................. 97 Y.Khotyaintsev,P.-A.Lindqvist,A.Eriksson,andM.Andre´ 7 FGMDataProductsintheCAA............................................109 J.M. Gloag, E.A. Lucek, L.-N. Alconcel, A. Balogh, P.Brown,C.M.Carr,C.N.Dunford,T.Oddy,andJ.Soucek ix x Contents 8 PEACEDataintheClusterActiveArchive ...............................129 A.N. Fazakerley,A.D. Lahiff, R.J. Wilson, I. Rozum, C.Anekallu,M.West,andH.Bacai 9 RAPIDProductsattheClusterActiveArchive...........................145 PatrickW.DalyandElenaA.Kronberg 10 STAFF Instrument Products Distributed Through theClusterActiveArchive...................................................159 N. Cornilleau-Wehrlin,L.Mirioni,P. Robert,V. Bouzid, M.Maksimovic,Y.deConchy,C.C.Harvey,andO.Santol´ık 11 ClusterWidebandDataProductsintheClusterActive Archive.........................................................................169 J.S.Pickett,J.M.Seeberger,I.W.Christopher,O.Santol´ık, andK.M.Sigsbee 12 TheWHISPERRelaxationSounderandtheCLUSTER ActiveArchive.................................................................185 J.G.Trotignon,P.M.E.De´cre´au,J.L.Rauch,X.Vallie`res, A.Rochel,S.Kougble´nou,G.Lointier,G.Facsko´,P.Canu, F.Darrouzet,andA.Masson 13 ESOCDataProductsintheCAA...........................................209 J.VolppandD.Sieg PartII ToolsfortheCAADataAnalysis 14 QSAS,QMScienceAnalysisSoftware.....................................225 A.J.Allen 15 FlexibleToolsforAccessingtheClusterArchives ........................233 E.Gamby,J.DeKeyser,andM.Roth 16 AMDA,AutomatedMulti-DatasetAnalysis:AWeb-Based ServiceProvidedbytheCDPP..............................................239 C.Jacquey,V.Ge´not,E.Budnik,R.Hitier,M.Bouchemit, M.Gangloff,A.Fedorov,B.Cecconi,N.Andre´,B.Lavraud, C. Harvey,F. De´riot, D. Heulet, E. Pallier, E. Penou, andJ.L.Pinc¸on 17 ClusterCAAModuleforPaPCo............................................249 J. Faden,A.A˚snes, R. Friedel,M.Taylor,S. McCaffrey, C.Perry,andM.L.Goldstein Contents xi PartIII MeasurementTechniquesandCalibrationRoutines 18 Electron Density Estimation in the Magnetotail: aMulti-InstrumentApproach...............................................261 A.Masson,O.Santol´ık,M.G.G.T.Taylor,C.P.Escoubet, A.N.Fazakerley,J.Pickett,A.A˚snes,X.Vallie`res,H.Laakso, andJ.-G.Trotignon 19 Cluster-PEACEIn-flightCalibrationStatus ..............................281 A.N.Fazakerley,A.D.Lahiff,I.Rozum,D.Kataria,H.Bacai, C.Anekallu,M.West,andA.A˚snes 20 Generation and Validation of Ion Energy Spectra BasedonClusterRAPIDandCISMeasurements........................301 Elena A. Kronberg,PatrickW. Daly, IannisDandouras, SteinHaaland,andEditaGeorgescu PartIV MagnetosphericMissions 21 TheClusterMission:SpacePlasmainThreeDimensions...............309 M.G.G.T.Taylor,C.P. Escoubet,H. Laakso,A. Masson, andM.L.Goldstein 22 DoubleStar:Mission,InstrumentsandJointObservations.............331 M.W.Dunlop,C.P.Escoubet,Z.-X.Liu,C.Shen,H.Laakso, M.G.G.T.Taylor,A.N.Fazakerley,andtheDoublestarPIs PartV ObservationsofSolarWindandMagnetosheath 23 Effect of Shock Normal Orientation Fluctuations onField-AlignedBeamDistributions.......................................349 K.Meziane,A.M.Hamza,M.Wilber,M.A.Lee,C.Mazelle, E.A.Lucek,T.Hada,andA.Markowitch 24 WaveNumberSpectraintheSolarWind,theForeshock, andtheMagnetosheath ......................................................363 Y. Narita,K.-H. Glassmeier,S.P. Gary,M.L. Goldstein, andR.A.Treumann 25 ClusterHotFlowAnomalyObservationsDuringSolar CycleMinimum...............................................................369 G.Facsko´,M.Ta´trallyay,G.Erdo˝s,andI.Dandouras

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Since the year 2000 the ESA Cluster mission has been investigating the small-scale structures and processes of the Earth's plasma environment, such as those involved in the interaction between the solar wind and the magnetospheric plasma, in global magnetotail dynamics, in cross-tail currents, and i
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