The time-lag between magnetic and ionospheric changes

Physics

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Scientific paper

The above time-lag is investigated for summer months (November-February) from summer 1953/1954 to summer 1960/1961. It is found that the 1 day delay reported by and (1961) is in fact only predominant during periods of high solar activity and absent during sunspot minimum. A 2 day lag seems to persist throughout the solar cycle but is overshadowed during sunspot maximum by the 1 day delay. The nocturnal behaviour of maximum electron density in the F2-region is studied during a year of high solar activity in relation to the K-indices of the preceding day. A recombinative type of electron removal is found to correlate more consistently with magnetic changes than does an attachment type of removal.

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