Abstract
IT has long been known that magnetic storms may be associated with major changes in the F2 region of the ionosphere. Recently interest has been concentrated on the relationship between the level of magnetic activity, and three ionospheric parameters, namely NT, the total electron content; NM, the maximum ionization density; and T=NT/NM, the “equivalent slab thickness”. The exact nature of the relationship is not yet clear, and published results are to some extent conflicting. It has been shown, however1,2, that a moderate or severe storm is often accompanied by the following effects, (a) During the first day after the start—a “sudden commencement” or “gradual commencement” — NT is unusually high. It may remain so for 12–24 h, and then change fairly rapidly to become unusually low. It may then take as long as 24 – 36 h to return to a normal value. (b) NM follows a similar pattern to that of NT, although the effect is not always so pronounced, (c) The slab thickness increases considerably during the day after the commencement of a storm. The amount and duration of the increase are very variable.
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References
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SMITH, D., NELSON, G. & PYKE, J. Abnormal Diurnal Variation of Total Ionization. Nature 219, 1144–1145 (1968). https://doi.org/10.1038/2191144a0
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DOI: https://doi.org/10.1038/2191144a0
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