Abstract. We have investigated the solar flare effects on
ionospheric absorption with the systematic analysis of ionograms measured at
midlatitude and low-latitude ionosonde stations under different solar zenith
angles. The lowest recorded ionosonde echo, the minimum frequency (fmin, a
qualitative proxy for the “nondeviative” radio wave absorption occurring
in the D-layer), and the dfmin parameter (difference between the value of
the fmin and the mean fmin for reference days) have been considered. Data
were provided by meridionally distributed ionosonde stations in Europe and
South Africa during eight X- and M-class solar flares in solar cycle 23.
Total and partial radio fade-out was experienced at every ionospheric
station during intense solar flares (> M6). The duration of the
total radio fade-out varied between 15 and 150 min and it was highly
dependent on the solar zenith angle of the ionospheric stations.
Furthermore, a solar-zenith-angle-dependent enhancement of the fmin (2–9 MHz) and dfmin (1–8 MHz) parameters was observed at almost every station.
The fmin and dfmin parameters show an increasing trend with the enhancement
of the X-ray flux. Based on our results, the dfmin parameter is a good
qualitative measure for the relative variation of the “nondeviative”
absorption, especially in the case of the less intense solar flares, which do
not cause total radio fade-out in the ionosphere (class < M6).
Low-latitude ionosphericDregion dependence on solar zenith angle