Solar cycle hysteresis on F-region electron concentration peak heights over Tucuman.

Details Solar cycle hysteresis on F-region electron concentration peak heights over Tucuman. Solar cycle hysteresis on F-region electron concentration peak heights over Tucuman.

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..15...83o&link_type=abstract

Advances in Space Research, Vol. 15, No. 2, p. 83 - 88

Physics

Earth Ionosphere: Solar Activity Cycles

Scientific paper

Ionospheric models (or numerical maps) usually depend on a solar activity index. The relevant relations are, however, not always the same in the ascending and descending parts of a solar cycle. Cycle 21, distinct from cycle 20, shows a strong "hysteresis" of foF2. In the present paper the authors analyse the behaviour of the parameter M(3000)F2 for the same cycles 20 and 21. The results may be used in a revision of current prediction models and maps.

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