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dc.contributor.authorPierrard, V.
dc.date2003
dc.date.accessioned2017-05-03T10:59:16Z
dc.date.available2017-05-03T10:59:16Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5165
dc.descriptionIn the present paper, a kinetic model of the transition region between the collision-dominated and the collisionless domains of the neutral planetary atmospheres is presented. The Boltzmann equation is solved to study the escape of hydrogen and helium from the terrestrial atmosphere through a background of oxygen. The escape of hydrogen atoms from the atmosphere of Mars is also considered. A spectral method, initially developed to study the polar wind, is used to solve the collisional Boltzmann equation. The effects of the planetary curvature and the gravitational force are taken into account. The escape flux is found to be reduced by a factor 0.9 for helium and 0.6 for hydrogen escaping from the terrestrial atmosphere compared with purely exospheric Jeans' flux. For hydrogen escaping from Mars, the factor is around 0.57. Density and temperature profiles are also provided. The results are compared with those of previous collisional models based on Monte Carlo simulations or on the Boltzmann equation with different assumptions.
dc.languageeng
dc.titleEvaporation of hydrogen and helium atoms from the atmospheres of Earth and Mars
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeComputer simulation
dc.subject.freeEarth (planet)
dc.subject.freeEarth atmosphere
dc.subject.freeExtraterrestrial atmospheres
dc.subject.freeHelium
dc.subject.freeHydrogen
dc.subject.freeMonte Carlo methods
dc.subject.freePlanets
dc.subject.freeTransition region
dc.subject.freeAstrophysics
dc.source.titlePlanetary and Space Science
dc.source.volume51
dc.source.issue4-5
dc.source.page319-327
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/S0032-0633(03)00014-X
dc.identifier.scopus2-s2.0-0037382882


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