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Particle acceleration at comets

dc.contributor.authorGombosi, Tamas I.en_US
dc.date.accessioned2011-11-15T15:57:58Z
dc.date.available2011-11-15T15:57:58Z
dc.date.issued1992-08-05en_US
dc.identifier.citationGombosi, Tamas I. (1992). "Particle acceleration at comets." AIP Conference Proceedings 264(1): 267-272. <http://hdl.handle.net/2027.42/87298>en_US
dc.identifier.otherAPCPCS-264-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87298
dc.description.abstractThis paper compares calculated and measured energy spectra of implanted H+ and O+ ions on the assumption that the pick‐up geometry is quasi‐parallel and about 1% of the waves generated by the cometary pickup process propagates backward (towards the comet). The model provides a good description of the implanted O+ and H+ energy distribution near the pickup energies.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleParticle acceleration at cometsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_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, Ann Arbor, Michigan 48109en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87298/2/267_1.pdf
dc.identifier.doi10.1063/1.42739en_US
dc.identifier.sourceParticle acceleration in cosmic plasmasen_US
dc.owningcollnamePhysics, Department of


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