Time delays in the correlation between solar activity and the F2 region plasma frequency

Details Time delays in the correlation between solar activity and the F2 region plasma frequency Time delays in the correlation between solar activity and the F2 region plasma frequency

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jastp..73..623t&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 73, Issue 5-6, p. 623-626.

Physics

Scientific paper

The upper ionosphere electron density characterized by the critical frequency foF2 is correlated with solar activity when using monthly medians or averages from longer intervals. When shorter intervals are studied, time delays of different lengths in solar activity effects in the ionosphere are observed. The correlation between the foF2 values and the solar radiation intensity, given by the F10.7 index, is studied using the 1967-2003 data of mid-latitude ionosonde stations spaced at distances greater than 100° in geographical longitude. At which longitude the reaction of foF2 to the changes in solar activity appears sooner depends on the position of the interval studied in the 22-year solar cycle.

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