Abstract
A mathematical model of the
high-latitude ionosphere, developed earlier in the Polar Geophysical Institute,
is utilized to calculate three-dimensional distributions of ionospheric
parameters, modified by the action of the ionospheric heater. The model takes
into account the convection of the ionospheric plasma, strong magnetization of
the plasma at F-layer altitudes, and geomagnetic field declination. The
calculations were made for two cases. Firstly, we simulated the distributions
of the ionospheric parameters under natural conditions without a powerful
high-frequency wave effect. Secondly, the distributions of the ionospheric
parameters were calculated on condition that an ionospheric heater, situated at
the point with geographic coordinates of the HF heating facility near Tromso,
Scandinavia, has been operated, with the ionospheric heater being located on
the night side of the Earth. The results of the numerical simulation indicate
that artificial heating of the ionosphere by powerful high-frequency waves
ought to influence noticeably on the spatial structure of the nighttime
high-latitude F-region ionosphere in the vicinity of the ionospheric heater.