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• W2042045380 abstract "The F-region changes associated with three severe magnetic storms during the IGY period are studied. The relevant h′f data from Washington (D.C.), Panama, Talara, and Huancayo, which lie approximately along the 75°W meridian, are converted to electron-density-true-height profiles. From the N-h profiles the storm changes in NmF, h(0.9NmF), NT, the total electron contents up to 200 and 300 km, and the thickness parameters [h(0.9.NmF) - h(05NmF)] are determined and studied. The storm changes in NmF and h(0.9NmF) indicate that large height variations of the order of 200 km may occur during severe storms. It is shown that the changes in NmF and h(0.9NmF) during given storms could be separated into two parts: one due to polar ionospheric DS currents, and one (Dst) due to current systems well above the ionosphere. These have general features similar to those derived for averages of storms, although several significant departures are observed. It is found that the total electron content up to 200 km is relatively unaffected by storms; NmF the electron content between 200 and 300 km, and the subpeak electron content are, in general, found to decrease during strong storms from middle latitudes to the equatorial region. The thickness of the F region is also found to increase after the SC during the first day of the storm. The DS part of the ionospheric storm effects is explainable by Martyn's drift theory. The Dst part can be explained as being due to an enhanced loss coefficient at relevant height levels. The increase in the loss coefficient is believed to be caused by ionospheric heating during storms as inferred from recent satellite drag data." @default.
• W2042045380 created "2016-06-24" @default.
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• W2042045380 date "1963-04-01" @default.
• W2042045380 modified "2023-10-18" @default.
• W2042045380 title "Changes in theFregion during magnetic storms" @default.
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• W2042045380 doi "https://doi.org/10.1029/jz068i007p01899" @default.
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