The relationship between 10 cm solar flux and electron concentration in the topside ionosphere

Details The relationship between 10 cm solar flux and electron concentration in the topside ionosphere The relationship between 10 cm solar flux and electron concentration in the topside ionosphere

Mar 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968jatp...30..431k&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 30, no. 3, pp. 431-437

Physics

Scientific paper

It is shown that the electron concentration at heights above the peak of the F2-layer increases by a factor of between 2 and 5 during periods of enhanced 10·7 cm solar flux. The effect is more pronounced at a latitude where the magnetic dip is 30° than above the magnetic equator. There is no obvious accompanying effect in the critical frequency of the F2-layer, and the combined evidence suggests that the entire topside electron distribution is displaced upwards during periods of enhanced solar flux.

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