Results on heating the ionospheric F region above Tromso, Norway are presen
ted. The ionosphere was monitored by satellite tomography and amplitude sci
ntillation methods as well as the EISCAT incoherent scatter radar. No effec
t of heating was observed in the daytime. In the evening and in the pre-mid
night sector, noticeable tilts of the F region were observed during heating
periods. The tilts overlapped the heating cone, where the electron density
decreased and irregularities exceeding 10 km in size appeared. Between the
heating periods the F layer was restored to its horizontal shape. The anis
otropic parameters of small-scale irregularities with scale lengths of hund
reds of metres were also determined. It was found that the perpendicular an
isotropy points in the direction of F region plasma flow. In some cases the
results can be explained by assuming that the small-scale irregularities w
ere generated within the heating cone and drifted out of the heating region
where they were subsequently observed.