Diffusion and heat flow equations for the mid-latitude topside ionosphere
dc.contributor.author | St. -Maurice, J. -P. | en_US |
dc.contributor.author | Schunk, Robert W. | en_US |
dc.date.accessioned | 2006-04-07T17:08:39Z | |
dc.date.available | 2006-04-07T17:08:39Z | |
dc.date.issued | 1977-10 | en_US |
dc.identifier.citation | St.-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.uri | http://www.sciencedirect.com/science/article/B6V6T-46YJY43-1BD/2/7494d689ad47037e34ba1a8c381601a5 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/22836 | |
dc.description.abstract | For 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.extent | 1265767 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.title | Diffusion and heat flow equations for the mid-latitude topside ionosphere | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Atmospheric, Oceanic and Space Sciences | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department 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.affiliationum | Department 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.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/22836/1/0000396.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0032-0633(77)90003-4 | en_US |
dc.identifier.source | Planetary and Space Science | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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