ABSTRACT
It is well known that radiophysical methods allow finding and studying of the WD electron concentration N. At the same time, for performance of the dynamic physical-mathematical model of the whole complex of processes caused by SV launches and flights, knowledge of spatiotemporal variations not only of N but also of other parameters of plasma is required. Complex diagnostics of the ionospheric plasma can be carried out using the results of incoherent scatter (IS) radar (ISR) measurement [12-15].
