Potential effects of the IMF-orientation on the mid-latitude ionosphere are further investigated using critical frequencies foF2 from six ionosonde stations. For a period of 15 days around each inversion of B-Z, excluding all days with Ap >=6, a quiet standard diurnal variation was determined by day-by-day averaging for each hour UT. The regular diurnal, seasonal and solar cycle variations were then removed from the data by substracting from these the quiet standard value. The so obtained differences ofoF2 were sorted after the INF polarity. Distinct effects of northward and southward inversions were found so that a large part of the day-to day variability may be attributed to IMF B-Z polarity changes
he F-region variability of the ionosphere during high solar activity periods have been studied using...
We examine the ionospheric F2-layer electron density variation by solar activity in middle latitude ...
Saturation in the dependence of foF2 on solar flux is a phenomenon more pronounced in the equatorial...
Using criticaI frequencies, f0F2 from the Uppsala, Lannion and Dourbes ionosonde stations, the possi...
The possible effects of the orientation of the IMF on the ionosphere has been studied by Tulunay (19...
Using critical frequencies, f0F2 from the Lannion, Slough, Poitiers, Garchy, Dourbes, Rome, Juliusru...
46-50The critical frequency of the ionosphere, apart from the diurnal and annual variations exhibit ...
Geomagnetic activities frequently occur in varying degrees. Strong geomagnetic activities, which hav...
In this study a comparison is made of the Utah State University Time-Dependent Ionospheric Model (TD...
International audienceNoontime monthly median values of F2-layer critical frequency foF2 (m) for som...
The data on ionospheric total electron content and the peak density of the mid-latitude F2 layer (Nm...
Noontime monthly median values of F2-layer critical frequency foF2 (m) for some ionospheric statio...
124-129This paper presents diurnal, seasonal and solar activity effects on the variability of ionos...
The structure of the Interplanetary Magnetic Field (IMF) is responsible for an essential part of the...
The ionosphere displays variations on a wide range of time-scales, ranging from operational time-sca...
he F-region variability of the ionosphere during high solar activity periods have been studied using...
We examine the ionospheric F2-layer electron density variation by solar activity in middle latitude ...
Saturation in the dependence of foF2 on solar flux is a phenomenon more pronounced in the equatorial...
Using criticaI frequencies, f0F2 from the Uppsala, Lannion and Dourbes ionosonde stations, the possi...
The possible effects of the orientation of the IMF on the ionosphere has been studied by Tulunay (19...
Using critical frequencies, f0F2 from the Lannion, Slough, Poitiers, Garchy, Dourbes, Rome, Juliusru...
46-50The critical frequency of the ionosphere, apart from the diurnal and annual variations exhibit ...
Geomagnetic activities frequently occur in varying degrees. Strong geomagnetic activities, which hav...
In this study a comparison is made of the Utah State University Time-Dependent Ionospheric Model (TD...
International audienceNoontime monthly median values of F2-layer critical frequency foF2 (m) for som...
The data on ionospheric total electron content and the peak density of the mid-latitude F2 layer (Nm...
Noontime monthly median values of F2-layer critical frequency foF2 (m) for some ionospheric statio...
124-129This paper presents diurnal, seasonal and solar activity effects on the variability of ionos...
The structure of the Interplanetary Magnetic Field (IMF) is responsible for an essential part of the...
The ionosphere displays variations on a wide range of time-scales, ranging from operational time-sca...
he F-region variability of the ionosphere during high solar activity periods have been studied using...
We examine the ionospheric F2-layer electron density variation by solar activity in middle latitude ...
Saturation in the dependence of foF2 on solar flux is a phenomenon more pronounced in the equatorial...