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- W2038435548 abstract "Variations in the electron density distribution of the topside ionosphere (including the height of the F2 peak) obtained from Alouette I during the great magnetic storm of 17–19 April 1965 are analyzed. Both enhancement and depletion of topside ionization are observed depending on the phase of the magnetic storm. Specifically, enhancement is associated with the positive phase and the asymmetric part of the main phase, while depletion of the topside ionosphere occurs during the symmetric part of the storm main phase over a latitude range corresponding to L values greater than 3. Associated with this depletion is a redistribution of ionization indicating that the topside ionosphere during the symmetric main phase consists primarily of O+ (with H+ being depleted). The enhancement of topside ionization during the positive phase of the storm appears to be associated with the compression of the daytime magnetosphere during that phase of the storm. The depletion seems to be associated with the expansion of field tubes due to the presence of the high energy-density ring current plasma as observed on satellites causing an upward flux from the topside ionosphere. A similar upward flux could also arise from a sink of thermal plasma in the magnetosphere due to the local energization of this plasma." @default.
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- W2038435548 date "1968-05-01" @default.
- W2038435548 modified "2023-09-27" @default.
- W2038435548 title "Behavior of the topside ionosphere during a great magnetic storm" @default.
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- W2038435548 doi "https://doi.org/10.1016/0032-0633(68)90104-9" @default.
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