Day-to-day variations in the F2 critical frequency

Physics

Scientific paper

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Scientific paper

From a comparison of ionospheric changes at F1 and F2 heights it is found that most of the variations in [latin small letter f with hook]oF2 can be attributed to variations in the incident ionizing radiation and in the rate of electron recombination. The ionizing radiation follows fairly closely the 2800 Mc/s solar radio flux. The recombination rate is affected by ionospheric storms and travelling disturbances, and it also shows a steady drift over the period studied.

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