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dc.contributor.authorNicolet, M.
dc.coverage.temporal20th century
dc.date1960
dc.date.accessioned2016-03-07T17:14:03Z
dc.date.accessioned2021-12-09T09:52:37Z
dc.date.available2016-03-07T17:14:03Z
dc.date.available2021-12-09T09:52:37Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/8355
dc.descriptionA physical picture of the upper atmosphere cannot be obtained without determining whether vertical distribution depends on mixing or diffusion or on a chemical or photochemical equilibrium. It is necessary to determine how dissociation and recombination of molecular and atomic oxygen and nitrogen are distributed with height. The structure of the atmosphere deduced from density measurements is related to the variation of the mean molecular mass depending on diffusion effects. In addition, it is necessary to know how the heat budget is affected by conduction.
dc.languageeng
dc.publisherIRM
dc.publisherKMI
dc.publisherRMI
dc.relation.ispartofseriesContributions, n° - Bijdragen, nr.
dc.titleConstitution of the atmosphere at ionospheric levels
dc.typeBook
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceGeneral Public
dc.audienceScientific
dc.subject.freeAtmosphere
dc.subject.freeChemical Equilibrium
dc.subject.freePhotochemical Equilibrium
dc.subject.freeMolecular Oxygen
dc.subject.freeAtomic Oxygen
dc.subject.freeNitrogen
dc.source.volume56
dc.source.page12
Orfeo.peerreviewedYes


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