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Composition and temperatures of the topside ionosphere over Arecibo
Authors:M.C. Ho  D.R. Moorcroft
Affiliation:Department of Physics, Nanyang University, Jurong Road, Singapore 22, Republic of Singapore;Centre for Radio Science and Department of Physics, University of Western Ontario, London, Ontario, Canada
Abstract:Results of analysis of about 150 autocorrelation functions are presented for the period from about 2300 hr on 5 October to about 1200 hr on 7 October 1967. A large percentage concentration of helium ions are observed. It reaches a value as high as 50 per cent with a maximum at around 800 km. Downward heat fluxes deduced from the temperature variations yield a value of about 2–2.5 × 109 eV cm?2 sec?1 during the period 1200–1600 hr and a value of about 1.5 × 108 eV cm?2 sec?1 during the period 0100–0400 hr at night. These agree well with other measurements. The O+ ions are found not to be in diffusive equilibrium, and from the O+ fluxes and the electron density profiles, the O+ drift velocity has been estimated. It is found that the speed can be as high as 1–5 × 103 cm sec?1 even at altitudes as high as 700 km.
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