View Item 

Show simple item record

Magnetospheric and Plasma Science with Cassini-Huygens

dc.contributor.authorMaurice, S.en_US
dc.contributor.authorEsposito, L. W.en_US
dc.contributor.authorTsurutani, B. T.en_US
dc.contributor.authorNeubauer, Fritz M.en_US
dc.contributor.authorLiewer, Paulett C.en_US
dc.contributor.authorBlanc, M.en_US
dc.contributor.authorBolton, S.J.en_US
dc.contributor.authorBradley, J.en_US
dc.contributor.authorBurton, M.en_US
dc.contributor.authorCravens, Tom E.en_US
dc.contributor.authorDandouras, I.en_US
dc.contributor.authorDougherty, M. K.en_US
dc.contributor.authorFestou, M. C.en_US
dc.contributor.authorFeynman, J.en_US
dc.contributor.authorJohnson, R. E.en_US
dc.contributor.authorGombosi, Tamas I.en_US
dc.contributor.authorKurth, Williamen_US
dc.contributor.authorMauk, B. H.en_US
dc.contributor.authorMitchell, D. G.en_US
dc.contributor.authorRichardson, J. D.en_US
dc.contributor.authorShemansky, D. E.en_US
dc.contributor.authorSittler, E. C.en_US
dc.contributor.authorZarka, P.en_US
dc.contributor.authorGrün, E.en_US
dc.contributor.authorKliore, A. J.en_US
dc.contributor.authorKrimigis, S. M.en_US
dc.contributor.authorSouthwood, David J.en_US
dc.contributor.authorYoung, D. T.en_US
dc.contributor.authorWaite, J. Hunteren_US
dc.contributor.authorGurnett, D. A.en_US
dc.date.accessioned2006-09-11T13:47:38Z
dc.date.available2006-09-11T13:47:38Z
dc.date.issued2002-03en_US
dc.identifier.citationBlanc, M.; Bolton, S.; Bradley, J.; Burton, M.; Cravens, T.E.; Dandouras, I.; Dougherty, M.K.; Festou, M.C.; Feynman, J.; Johnson, R.E.; Gombosi, T.G.; Kurth, W.S.; Liewer, P.C.; Mauk, B.H.; Maurice, S.; Mitchell, D.; Neubauer, F.M.; Richardson, J.D.; Shemansky, D.E.; Sittler, E.C.; Tsurutani, B.T.; Zarka, Ph.; Esposito, L.W.; Grün, E.; Gurnett, D.A.; Kliore, A.J.; Krimigis, S.M.; Southwood, D.; Waite, J.H.; Young, D.T.; (2002). "Magnetospheric and Plasma Science with Cassini-Huygens." Space Science Reviews 104 (1-4): 253-346. <http://hdl.handle.net/2027.42/43757>en_US
dc.identifier.issn0038-6308en_US
dc.identifier.issn1572-9672en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43757
dc.description.abstractMagnetospheric and plasma science studies at Saturn offer a unique opportunity to explore in-depth two types of magnetospheres. These are an `induced' magnetosphere generated by the interaction of Titan with the surrounding plasma flow and Saturn's `intrinsic' magnetosphere, the magnetic cavity Saturn's planetary magnetic field creates inside the solar wind flow. These two objects will be explored using the most advanced and diverse package of instruments for the analysis of plasmas, energetic particles and fields ever flown to a planet. These instruments will make it possible to address and solve a series of key scientific questions concerning the interaction of these two magnetospheres with their environment.en_US
dc.format.extent2325428 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherExtraterrestrial Physics, Space Sciencesen_US
dc.subject.otherAstronomy, Astrophysics and Cosmologyen_US
dc.titleMagnetospheric and Plasma Science with Cassini-Huygensen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAerospace Engineeringen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michiganen_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michiganen_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, Californiaen_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, Californiaen_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, Californiaen_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, Californiaen_US
dc.contributor.affiliationotherCESR, Toulouse, Franceen_US
dc.contributor.affiliationotherObservatoire Midi-Pyrénées, Toulouse, Franceen_US
dc.contributor.affiliationotherUniversity of Virginia, Charlottesville, Virginiaen_US
dc.contributor.affiliationotherDepartment of Physics and Astronomy, University of Iowa, Iowa City, Iowaen_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, Californiaen_US
dc.contributor.affiliationotherApplied Physics Laboratory, The Johns Hopkins University, Laurel, Marylanden_US
dc.contributor.affiliationotherObservatoire Midi-Pyrénées, Toulouse, Franceen_US
dc.contributor.affiliationotherApplied Physics Laboratory, The Johns Hopkins University, Laurel, Marylanden_US
dc.contributor.affiliationotherInstitute for Geophysics and Meteorology, Köln University, Köln, Germanyen_US
dc.contributor.affiliationotherCenter for Space Research, MIT, Cambridge, Massachusettsen_US
dc.contributor.affiliationotherDepartment of Aerospace Engineering, University of Southern California, Los Angeles, Californiaen_US
dc.contributor.affiliationotherGoddard Space Flight Center, Greenbelt, Marylanden_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, Californiaen_US
dc.contributor.affiliationotherDESPA, Observatoire de Paris-Meudon, Meudon, Franceen_US
dc.contributor.affiliationotherLaboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Coloradoen_US
dc.contributor.affiliationotherMax-Planck-Institut für Kernphysik, Heidelberg, Germanyen_US
dc.contributor.affiliationotherDepartment of Physics and Astronomy, University of Iowa, Iowa City, Iowaen_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, Californiaen_US
dc.contributor.affiliationotherApplied Physics Laboratory, The Johns Hopkins University, Laurel, Marylanden_US
dc.contributor.affiliationotherThe Blackett Laboratory, Imperial College, London, U.Ken_US
dc.contributor.affiliationotherSouthwest Research Institute, San Antonio, Texasen_US
dc.contributor.affiliationotherThe Blackett Laboratory, Imperial College, London, U.Ken_US
dc.contributor.affiliationotherUniversity of Kansas, Lawrence, Kansasen_US
dc.contributor.affiliationotherObservatoire Midi-Pyrénées, Toulouse, Franceen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43757/1/11214_2004_Article_5106942.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/A:1023605110711en_US
dc.identifier.sourceSpace Science Reviewsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Name:
11214_2004_Article_5106942.pdf
Size:
2.217MB
Format:
PDF
View/Open

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.