Abstract

Representative profiles of the height distributions of electrons, positive ions and negative ions are presented as well as some critical ionospheric parameters such as the lumped electron loss coefficient ψ and the ratio of negative ions to electrons λ in the height range of 60 to 90 km for daytime polar cap absorption (PCA). A mere change of electron-ion production rate due to the enhanced particle precipitation was found insufficient to explain the behaviour of the D-region observed during PCA. To explain the observed decreases of ψ and the H +·(H 2O) n (NO + + O 2 +) ratio at 80 km, the profile of B, the lumped rate of conversion of NO + to H +·(H 2O) n had to be shifted by about 10 km downwards from the quiet daytime condition. While a decrease in the concentrations of O and O 3 was found to have a minor effect in the chemistry at 80 km, it had a profound effect in the negative ion region. To explain the observed decrease of λ (and hence ψ) from quiet to PCA condition at 60 km the concentrations of O and O 3 should be decreased by a factor of about 1.5–3. The effect of shifting the B profile at this height is negligible. At the intermediate region around 70 km both a shift in the B profile and a decrease in the concentrations of O and O 3 are necessary to explain the observed decrease of ψ and λ.

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