Negative F2-layer storms related to geomagnetic activity and quiet-time disturbances (Q-disturbances) belong to different classes of events and exhibit different morphology. Mid-latitude daytime Q-disturbances, unlike the usual negative F2-layer storms, demonstrate NmF2 and hmF2 in-phase variations. An analysis of Millstone Hill ISR observations for usual and Q-disturbances has shown the difference in the controlling aeronomic parameter variations for the two classes of events. The decrease in atomic oxygen concentration provides the main contribution to the hmF2 decrease below the monthly median level during Q-disturbance events. Unlike the usual negative storms, the negative effect takes place in the whole topside ionosphere un...
International audienceThe mechanism of the NmF2 peak formation at different levels of solar activity...
Storm effects at F1-layer heights (160–200 km) were analyzed for the first time using Millstone Hi...
To identify seasonal and latitudinal variations of F2 layer during magnetic storm, we examine the ch...
International audienceNegative F2-layer storms related to geomagnetic activity and quiet-time distur...
Earlier revealed seasonal/latitudinal variations of the occurrence for positive and negative F2-lay...
The observed NmF2 and NmE variations were analyzed for the periods of positive and negative quiet-t...
Abstract. Earlier revealed seasonal/latitudinal variations of the occurrence for positive and negati...
A self-consistent method for daytime F-region modelling was applied to EISCAT observations during t...
A critical analysis of recent publications devoted to the NmF2 pre-storm enhancements is performed....
A critical analysis of recent publications devoted to the NmF2 pre-storm enhancements is performed....
Daytime F2-layer positive storm effects at middle and lower latitudes in the winter thermosphere ar...
Abstract. A self-consistent method for daytime F-region modelling was applied to EISCAT observations...
International audienceIn this paper, the ionospheric quiet-time disturbances otherwise known as Pre-...
The global evolutions of foF2 anomalies were examined for three very intense geomagnetic storms, na...
The storm-time effects in the F2-region during the period of 1989–2001, at Ahmedabad (23.2°N, 72.4°E...
International audienceThe mechanism of the NmF2 peak formation at different levels of solar activity...
Storm effects at F1-layer heights (160–200 km) were analyzed for the first time using Millstone Hi...
To identify seasonal and latitudinal variations of F2 layer during magnetic storm, we examine the ch...
International audienceNegative F2-layer storms related to geomagnetic activity and quiet-time distur...
Earlier revealed seasonal/latitudinal variations of the occurrence for positive and negative F2-lay...
The observed NmF2 and NmE variations were analyzed for the periods of positive and negative quiet-t...
Abstract. Earlier revealed seasonal/latitudinal variations of the occurrence for positive and negati...
A self-consistent method for daytime F-region modelling was applied to EISCAT observations during t...
A critical analysis of recent publications devoted to the NmF2 pre-storm enhancements is performed....
A critical analysis of recent publications devoted to the NmF2 pre-storm enhancements is performed....
Daytime F2-layer positive storm effects at middle and lower latitudes in the winter thermosphere ar...
Abstract. A self-consistent method for daytime F-region modelling was applied to EISCAT observations...
International audienceIn this paper, the ionospheric quiet-time disturbances otherwise known as Pre-...
The global evolutions of foF2 anomalies were examined for three very intense geomagnetic storms, na...
The storm-time effects in the F2-region during the period of 1989–2001, at Ahmedabad (23.2°N, 72.4°E...
International audienceThe mechanism of the NmF2 peak formation at different levels of solar activity...
Storm effects at F1-layer heights (160–200 km) were analyzed for the first time using Millstone Hi...
To identify seasonal and latitudinal variations of F2 layer during magnetic storm, we examine the ch...