A prediction model of foF2 over periods of severe geomagnetic activity

The procedure is based on an empirical relationship between the ratio log(NmF2(t)/NmF2M(t)) and ap(τ), where NmF2(t) is the hourly maximum electron density at the F2 peak layer and NmF2M(t) is its 'quiet' value. The prediction of foF2 has been calculated during periods of severe magnetic activity in the current solar cycle 23 using data processed at the Rome ionospheric observatory. The performance of the model, during negative ionospheric storms, can be considered satisfactory, given that the root mean square (r.m.s.), calculated between measured and forecasted foF2, ranged between 0.74-2.0 MHz.