1964
DOI: 10.1029/jz069i021p04537
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Studies of planetary atmospheres: 1. The distribution of electrons and ions in the Earth's exosphere

Abstract: The factors which govern the distribution of electrons and ions in a planet's exosphere under diffusive equilibrium are discussed. The theory takes into account the effect of the electric field that arises from charge separation, the centrifugal force arising from the rotation of the planet, and the effect of the planet's gravitational field. It is assumed that the charged particles are constrained to move only along the direction of the planet's magnetic lines of force. The modifications that result in the el… Show more

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Cited by 338 publications
(154 citation statements)
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“…At higher levels, the diffusion problem becomes complicated due to the presence of more than one species. The diffusive equilibrium theory was first described by Dungey [1955] for two ion species and for multiconstituent plasma by Angerami and Thomas [1964]. Also, the dynamical nature of the topside ionosphere and plasmasphere is quite complex owing to the relatively large time constants associated with the plasma flow characteristics and the frequent occurrences of plasma disturbances caused by various sources.…”
Section: Discussionmentioning
confidence: 99%
“…At higher levels, the diffusion problem becomes complicated due to the presence of more than one species. The diffusive equilibrium theory was first described by Dungey [1955] for two ion species and for multiconstituent plasma by Angerami and Thomas [1964]. Also, the dynamical nature of the topside ionosphere and plasmasphere is quite complex owing to the relatively large time constants associated with the plasma flow characteristics and the frequent occurrences of plasma disturbances caused by various sources.…”
Section: Discussionmentioning
confidence: 99%
“…This approach yields a first approximation, which is qualitatively useful, although ion composition is likely to vary during this second time interval. Actually, the diffusive equilibrium model (Angerami and Thomas, 1964; see also Sonwalkar et al, 2011b) indicates that the effective ion mass is increasing with decreasing distance along the line of force (from a base level of 500 km) which is the case here, from time interval I to time interval II, and in a more significant manner, during interval II (altitudes in the range 1600-1200 km). If this is indeed the case, then the plasma frequency profile indicates a lower threshold of local electron density along the orbit.…”
Section: Specific Situation Encountered On Clustermentioning
confidence: 99%
“…To estimate the contribution of the plasmaspheric region to the observed TEC value, we employ a simple diffusive equilibrium model proposed by Angerami and Thomas [22]. According to this model we assume the electron density distribution in the plasmasphere n(h) is decreasing exponentially from the top of the ionospheric region (h 0 = 700 km) with the scale length H s up to the satellite orbits (h sat = 20200 km).…”
Section: Some Issues Specific To the Ct Of The Ionospheric Electron Dmentioning
confidence: 99%