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Dust–Gas Interrelations In Comets: Observations And Theory

dc.contributor.authorCombi, Michael R.en_US
dc.contributor.authorKabin, Konstantinen_US
dc.contributor.authorDeZeeuw, Darren L.en_US
dc.contributor.authorGombosi, Tamas I.en_US
dc.contributor.authorPowell, Kenneth G.en_US
dc.date.accessioned2006-09-08T21:14:24Z
dc.date.available2006-09-08T21:14:24Z
dc.date.issued1997-01en_US
dc.identifier.citationCombi, Michael R.; KABIN, KONSTANTIN; DeZEEUW, Darren L.; Gombosi, Tamas I.; Powell, Kenneth G.; (1997). " Dust–Gas Interrelations In Comets: Observations And Theory ." Earth, Moon, and Planets 79 (1-3): 275-306. <http://hdl.handle.net/2027.42/43256>en_US
dc.identifier.issn0167-9295en_US
dc.identifier.issn1573-0794en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43256
dc.description.abstractThe development of the expanding atmospherefrom the evaporating cometary nucleus has traditionallyfocused on observing and modeling the separatedevelopment of two distinct components, gas and dust,which are coupled dynamically with one another atdistances out to a few tens of cometary radii. In the lastdecade or so, however, direct evidence from observationsand suggestions from theory suggest that the dusty-gascoma is a tightly coupled system where material is transferredbetween the solid and gaseous phase as an importantintegral part of the basic development of the coma.en_US
dc.format.extent281839 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.otherGeophysics/Geodesyen_US
dc.subject.otherPlanetologyen_US
dc.subject.otherRemote Sensing/Photogrammetryen_US
dc.subject.otherAstrophysicsen_US
dc.subject.otherCometsen_US
dc.subject.otherHale–Boppen_US
dc.subject.otherDynamicsen_US
dc.subject.otherPhotochemistryen_US
dc.titleDust–Gas Interrelations In Comets: Observations And Theoryen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumSpace Physics Research Laboratory, Department of Atmospheric Oceanic and Space Sciences, The University of Michigan, 1417 A Space Research Building, Ann Arbor, MI, 48109-2143, USAen_US
dc.contributor.affiliationumSpace Physics Research Laboratory, Department of Atmospheric Oceanic and Space Sciences, The University of Michigan, 1417 A Space Research Building, Ann Arbor, MI, 48109-2143, USAen_US
dc.contributor.affiliationumSpace Physics Research Laboratory, Department of Atmospheric Oceanic and Space Sciences, The University of Michigan, 1417 A Space Research Building, Ann Arbor, MI, 48109-2143, USAen_US
dc.contributor.affiliationumSpace Physics Research Laboratory, Department of Atmospheric Oceanic and Space Sciences, The University of Michigan, 1417 A Space Research Building, Ann Arbor, MI, 48109-2143, USAen_US
dc.contributor.affiliationumW. M. Keck Foundation CFD Laboratory, Department of Aerospace Engineering, The University ofMichigan, Ann Arbor, MI, 48109-2143, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43256/1/11038_2004_Article_239224.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/A:1006257922294en_US
dc.identifier.sourceEarth, Moon, and Planetsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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