dc.contributor.advisor Cloutier, Paul A. McGary, John Edward 2009-06-03T23:53:50Z 2009-06-03T23:53:50Z 1988 http://hdl.handle.net/1911/16168 The Pioneer Venus observations show a peak in the O$\sb2\sp+$ concentration at $\sim$170 km altitude in the dayside ionosphere of Venus. In this thesis, the 2-dimensional MHD equations are solved in a self-consistent manner, as an extension to the 1-dimensional model by Cloutier et al. (1987), to present a global model of the Venus dayside ionosphere for solar zenith angles (SZA) $\leq$ 60$\sp\circ$. The model describes, by calculating vertical profiles at different SZA, ion densities, magnetic field magnitudes, and ion velocities. The model shows that the O$\sb2\sp+$ peak, at $\sim$170 km altitude, occurs throughout the dayside ionosphere as observed by the Orbiter Ion Mass Spectrometer (OIMS). The velocity field, which affects the ion distributions, is mainly tangential near the ionopause and radial for altitudes below 200 km. The downward flow accelerates, near 170 km altitude, due to collisional interactions with the neutral atmosphere, and removes the O$\sb2\sp+$ densities to lower altitudes, thus, producing the bump observed in the altitude profile. 108 p. application/pdf eng Atmospheric sciencesAstronomyAstrophysics A two-dimensional model of the Venus ionosphere Thesis Text Physics Natural Sciences Rice University Doctoral Doctor of Philosophy McGary, John Edward. "A two-dimensional model of the Venus ionosphere." (1988) Diss., Rice University. http://hdl.handle.net/1911/16168.
﻿