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dc.contributor.authorNicolet, M.
dc.date1968
dc.date.accessioned2017-08-21T12:58:58Z
dc.date.available2017-08-21T12:58:58Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5962
dc.descriptionFifty years ago Chapman (1917) found in the course of his work on the general kinetic theory of gases the phenomenon of thermal diffusion (earlier discovered in a special case by Enskog 1911); this is the relative motion of the components of a mixture arising from a temperature gradient. There has been much experimental study of thermal diffusion since the first experimental confirmation (Chapman & Dootson 1917). in the terrestrial atmosphere where the principal constituents of air are molecular nitrogen and oxygen the thermal‐diffusion flux is practically negligible compared with the diffusive flux due to the pressure gradient. Thermal diffusion is, however, important in the thermosphere where helium and hydrogen diffuse through a region with high temperature gradients.
dc.languageeng
dc.titleOn the Thermal‐Diffusion Effect in the Thermosphere
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleGeophysical Journal of the Royal Astronomical Society
dc.source.volume15
dc.source.issue1-2
dc.source.page157-161
Orfeo.peerreviewedYes
dc.identifier.doi10.1111/j.1365-246X.1968.tb05755.x
dc.identifier.scopus2-s2.0-84977252637


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