A zonally and annually averaged study of potential early Martian atmospheres

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dc.contributor.advisorFew, Arthur A., Jr.en_US
dc.creatorSchmunk, Robert Bradleyen_US
dc.date.accessioned2009-06-04T00:06:31Zen_US
dc.date.available2009-06-04T00:06:31Zen_US
dc.date.issued1993en_US
dc.description.abstractObservations of the surface of Mars suggest a high probability of surface water activity in that planet's past. Consequently, many studies of Mars' early atmosphere have attempted to estimate the carbon dioxide level by requiring that surface temperatures be high enough to support surface liquid water. In the main, these studies have employed one-dimensional, radiative-convective climate models capable of considering only a single solar zenith angle, typically chosen to represent a global and annual average. Such models are hence not well suited for considering meridional variations in the temperature profile, which are affected by variations in the orbital obliquity and the meridional redistribution of heat by dynamic processes. I describe modifications to a more complex model, the multi-level energy balance model designed at NASA's Goddard Laboratory for Atmospheric Sciences, which make it suitable for study of an atmosphere with varying carbon dioxide levels. Vertically and meridionally defined, the model includes heating and cooling by radiation, mean meridional circulation, large-scale (baroclinic) and small-scale (convective) eddies, and surface turbulent flux. I present annually-averaged results for an examination of potential atmospheres of early Mars, given that its carbon dioxide level may range from 0 to 500 Pa and the orbital obliquity from 0$\sp\circ$ to 50$\sp\circ.$ These results are compared with those obtained from a radiative-convective model.en_US
dc.format.extent91 p.en_US
dc.format.mimetypeapplication/pdfen_US
dc.identifier.callnoThesis Sp. Sci. 1993 Schmunken_US
dc.identifier.citationSchmunk, Robert Bradley. "A zonally and annually averaged study of potential early Martian atmospheres." (1993) Diss., Rice University. <a href="https://hdl.handle.net/1911/16664">https://hdl.handle.net/1911/16664</a>.en_US
dc.identifier.urihttps://hdl.handle.net/1911/16664en_US
dc.language.isoengen_US
dc.rightsCopyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.subjectAtmospheric sciencesen_US
dc.titleA zonally and annually averaged study of potential early Martian atmospheresen_US
dc.typeThesisen_US
dc.type.materialTexten_US
thesis.degree.departmentSpace Scienceen_US
thesis.degree.disciplineNatural Sciencesen_US
thesis.degree.grantorRice Universityen_US
thesis.degree.levelDoctoralen_US
thesis.degree.nameDoctor of Philosophyen_US
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