Abstract
A comparison covering more than three decades is made between the seasonal variation of radar meteor influx and seasonal variations in the occurrence probabilities of ionosonde sporadic- E parameters ƒ 0E s and ƒ bE s for different diurnal intervals at two Southern Hemisphere stations. The analyses show that for medium intensity 3 E m type sporadic- E no clear correlation with major Southern Hemisphere meteor shower activity exists. This finding which does not support some earlier shorter period surveys suggests the need for further work into the aeronomy of E s source ions.
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