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of the number of sunspots visible on the disk, the rate at which flares occur, or the intensity of the 10-cm radio flux, also affects the ionosphere because of variations in the intensity of the ionizing radiations in the X-ray and EUV bands." The F2 layer also exhibits anomalies due to diurnal variation and seasonal variation. Additionally, the F2 layer at mid-latitudes does not disappear

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