Latitudinal variation of foF2 hysteresis of solar cycles 20, 21 and 22 and its application to the analysis of long-term trends
N. Ortiz de Adler
A. G. Elias
- Publisher: Copernicus Publications
(issn: 0992-7689, eissn: 1432-0576)
Geophysics. Cosmic physics | Q | Science | Physics | QC1-999 | QC801-809
arxiv: Physics::Space Physics
Noon <I>fo</I>F2 monthly median values for equinoctial months of solar cycles 20, 21 and 22, were analyzed for 37 worldwide stations. For each solar cycle and for a given <I>R<sub>z</sub></I>, the difference between <I>fo</I>F2 in the falling branch of the cycle and the corresponding value of the rising branch is evaluated. The maximum difference, considered as the hysteresis magnitude, varies systematically with geomagnetic latitude. The pattern is similar for every cycle, with greater hysteresis magnitudes for stronger solar cycles. It is positive between 45° S and 45° N, with minimum values at equatorial latitudes and maximum at around 25°–30° on either side of the equator. For latitudes greater than 50° negative values are observed. At around 25°–30° and at high latitudes the hysteresis magnitude reaches 2 MHz for solar cycle with high activity levels, which represents around 20% of <I>fo</I>F2. The effects of <I>fo</I>F2 hysteresis on the analysis of long-term data sequences is analyzed. In the case of long-term trend analysis, the hysteresis behavior may induce spurious trends as a consequence of the filtering processes applied to <I>fo</I>F2 time series previous to trend values estimation. This problem may be solved by considering time series covering several solar cycles.