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Diffusion and heat flow equations for the mid-latitude topside ionosphere

dc.contributor.authorSt. -Maurice, J. -P.en_US
dc.contributor.authorSchunk, Robert W.en_US
dc.date.accessioned2006-04-07T17:08:39Z
dc.date.available2006-04-07T17:08:39Z
dc.date.issued1977-10en_US
dc.identifier.citationSt.-Maurice, J. -P., Schunk, R. W. (1977/10)."Diffusion and heat flow equations for the mid-latitude topside ionosphere." Planetary and Space Science 25(10): 907-920. <http://hdl.handle.net/2027.42/22836>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V6T-46YJY43-1BD/2/7494d689ad47037e34ba1a8c381601a5en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/22836
dc.description.abstractFor application to the mid-latitude topside ionosphere, we have derived diffusion and heat flow equations for a gas mixture composed of two major ions, electrons and a number of minor ions. These equations were derived by expanding the velocity distribution of each constituent about its 13 lower order velocity moments. As a consequence, each constituent was allowed to have its own temperature and drift velocity. The restriction to mid-latitudes results because we have assumed that the species temperature and drift velocity differences were small. In deriving the diffusion and thermal conduction equations, we have discovered some new transport effects. For the major ions, we have found that: (1) a temperature gradient in either gas causes thermal diffusion in both gases; (2) a temperature gradient in either gas causes heat to flow in both gases; and (3) a relative drift between the major ion gases induces a heat flow in both gases. Similar transport effects have also been found for the minor ions.en_US
dc.format.extent1265767 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleDiffusion and heat flow equations for the mid-latitude topside ionosphereen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Atmospheric and Oceanic Science, The University of Michigan, Ann Arbor, MI 48109, U.S.A.; Aeronomy Center, Utah State University, Logan, UT 84322, U.S.A.en_US
dc.contributor.affiliationumDepartment of Atmospheric and Oceanic Science, The University of Michigan, Ann Arbor, MI 48109, U.S.A.; Aeronomy Center, Utah State University, Logan, UT 84322, U.S.A.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/22836/1/0000396.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0032-0633(77)90003-4en_US
dc.identifier.sourcePlanetary and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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