As shown by ground-based absorption measurements, the lower ionospheric plasma is markedly controlled by the structure of the IMF. Whereas in high auroral and subauroral latitudes this effect is very pronounced, in midlatitudes its influence is less important. A comparison of these results with satellite data of the IMF and the solar wind speed confirms the important role of these components, not only during special events but also for the normal state of the ionospheric D region plasma
15th MST Radar WorkshopSession M3: Ionospheric irregularities and IS experimentsMay 27 (Sat), Poster...
International audienceWe have analysed a database of ?300 h of tristatic ionospheric velocity measur...
The convection of plasma in the high-latitude ionosphere is strongly a2ected by the interplanetary m...
The precipitation of high energetic electrons during and after strong geomagnetic storms into height...
Superposed epoch studies have been carried out in order to determine the ionospheric response at mi...
The Influence of the north–south component (Bz) of the interplanetary magnetic field (IMF) on geomag...
The Sun’s corona expands outward, populating the solar system with plasma. This plasma is known as t...
Study of the dynamic nature of low-latitude ionosphere during geomagnetically disturbed conditions, ...
In this paper we study the influence of the interplanetary magnetic field (IMF) polarity changes cau...
Treated jointly, two recent results imply that the distribution of winds in the polar ionosphere sho...
We investigate the variations in the ionosphere during a small geomagnetic storm on June 23, 2000, u...
Results are presented from two multi-instrument case studies showing patches of cold, long-lived pl...
International audienceIn this work an attempt to identify the role of the interplanetary magnetic fi...
Results are presented from two multi-instrument case studies showing patches of cold, long-lived pla...
The structure of the Interplanetary Magnetic Field (IMF) is responsible for an essential part of the...
15th MST Radar WorkshopSession M3: Ionospheric irregularities and IS experimentsMay 27 (Sat), Poster...
International audienceWe have analysed a database of ?300 h of tristatic ionospheric velocity measur...
The convection of plasma in the high-latitude ionosphere is strongly a2ected by the interplanetary m...
The precipitation of high energetic electrons during and after strong geomagnetic storms into height...
Superposed epoch studies have been carried out in order to determine the ionospheric response at mi...
The Influence of the north–south component (Bz) of the interplanetary magnetic field (IMF) on geomag...
The Sun’s corona expands outward, populating the solar system with plasma. This plasma is known as t...
Study of the dynamic nature of low-latitude ionosphere during geomagnetically disturbed conditions, ...
In this paper we study the influence of the interplanetary magnetic field (IMF) polarity changes cau...
Treated jointly, two recent results imply that the distribution of winds in the polar ionosphere sho...
We investigate the variations in the ionosphere during a small geomagnetic storm on June 23, 2000, u...
Results are presented from two multi-instrument case studies showing patches of cold, long-lived pl...
International audienceIn this work an attempt to identify the role of the interplanetary magnetic fi...
Results are presented from two multi-instrument case studies showing patches of cold, long-lived pla...
The structure of the Interplanetary Magnetic Field (IMF) is responsible for an essential part of the...
15th MST Radar WorkshopSession M3: Ionospheric irregularities and IS experimentsMay 27 (Sat), Poster...
International audienceWe have analysed a database of ?300 h of tristatic ionospheric velocity measur...
The convection of plasma in the high-latitude ionosphere is strongly a2ected by the interplanetary m...