Large-scale features of the ionospheric disturbances which lead to the occurrence of gigahertz scintillation events at midlatitudes are re-examined using h'Fdata at five ionosonde stations and HF Doppler measurements at Kokubunji. From these analyses, it is recognized that ionospheric dynamics during the events are generally characterized by a two-stage process, despite case-dependent quantitative differences in the appearance of each event. In this construction, an increase and subsequent decrease of virtual heights occur simultaneously at five stations in the first stage, with the rapid fluctuations of HF Doppler around the apex of h'F. On the contrary, virtual heights increase again in the second stage with time shifts that indicate a motion from north to south. It is shown that the second stage is responsible for the plasma instabilities which cause the gigahertz scintillation event at midlatitudes, whereas the first stage which corresponds to the enhancement stage of equatorial anomalies, is not unstable. From these features, important conclusions are derived that electric field reversals are expected during the events and westward electric fields seem more important for gigahertz scintillations at midlatitudes. Some other pieces of evidence are also shown which support the electric field reversals. As the cause of the two-stage process, a push-pull mechanism between ionized and neutral atmospheres is proposed.At midlatitude regions around Japan, severe gigahertz scintillations are very rare phenomena and appear only during geomagnetic storms. In a previous paper (hereinafter referred to as paper I), TANAKA (1981) has clarified characteristic features of magnetospheric and ionospheric disturbances which lead to the occurrence of midlatitude gigahertz scintillations. In paper I, the following picture was constructed for the condition to generate severe gigahertz scintillations at midlatitudes. During the main phase of geomagnetic storms, an eastward electric field of magnetospheric origin occasionally penetrates toward low latitudes in the dusk meridian, associated with the development of low-latitude asymmetric disturbance fields. This electric field causes sudden enhancements of equatorial anomalies to create strong positive ionospheric storms at subequatorial regions and negative ionospheric storms at the equator. After these intervals, some plasma instabilities are triggered in the midlatitude ionosphere as the results of modifications in ionospheric