The effect of eastward zonal wind speed (EZWS) on vertical drift velocity (E × Bdrift) that mainly controls the equatorial ionospheric irregularities has been explained theoretically and through numerical models. However, its effect on the seasonal and longitudinal variations of E × B and the accompanying irregularities has not yet been investigated experimentally due to lack of F‐layer wind speed measurements. Observations of EZWS from GOCE and ion density and E × B from C/NOFS satellites for years 2011 and 2012 during quite times are used in this study. Monthly and longitudinal variations of the irregularity occurrence, E × B, and EZWS show similar patterns. We find that at most 50.85% of longitudinal variations of E × B can be explained ...
International audienceData from the Jicamarca digisonde and the ROCSAT-1 satellite are employed to s...
We describe variations in total electron content (TEC) in the North American sector exhibiting prono...
We present the first complete study of the dynamics of the equatorial upper atmosphere (180-350 km) ...
We have used extensive radar measurements from the Jicamarca Observatory during low solar flux perio...
F-region vertical velocities are derived from the ground-based ionosonde data for Ibadan (7.4°N, 3.9...
International audienceWe use a digisonde at Jicamarca and a chain of GPS receivers on the west side ...
International audienceA seasonally dependent total neutral wind model obtained from experimental dat...
The study of long term variation of drift and anisotropy parameters of E region irregularities is pa...
In this study we used observations from the CHAMP and ROCSAT-1 satellites to investigate the solar w...
International audienceWe used ion drift observations from the DE-2 satellite to study for the first ...
International audienceWith a well-selected data set, the various events of the vertical E × B drift ...
In the modern world, we increasingly depend on space-based systems for our communication, positionin...
International audienceAnnual and seasonal variations in the low-latitude topside ionosphere are inve...
The diurnal variation of peak electron density, NmF2, of five stations for different seasons, solar ...
Study of the dynamic nature of low-latitude ionosphere during geomagnetically disturbed conditions, ...
International audienceData from the Jicamarca digisonde and the ROCSAT-1 satellite are employed to s...
We describe variations in total electron content (TEC) in the North American sector exhibiting prono...
We present the first complete study of the dynamics of the equatorial upper atmosphere (180-350 km) ...
We have used extensive radar measurements from the Jicamarca Observatory during low solar flux perio...
F-region vertical velocities are derived from the ground-based ionosonde data for Ibadan (7.4°N, 3.9...
International audienceWe use a digisonde at Jicamarca and a chain of GPS receivers on the west side ...
International audienceA seasonally dependent total neutral wind model obtained from experimental dat...
The study of long term variation of drift and anisotropy parameters of E region irregularities is pa...
In this study we used observations from the CHAMP and ROCSAT-1 satellites to investigate the solar w...
International audienceWe used ion drift observations from the DE-2 satellite to study for the first ...
International audienceWith a well-selected data set, the various events of the vertical E × B drift ...
In the modern world, we increasingly depend on space-based systems for our communication, positionin...
International audienceAnnual and seasonal variations in the low-latitude topside ionosphere are inve...
The diurnal variation of peak electron density, NmF2, of five stations for different seasons, solar ...
Study of the dynamic nature of low-latitude ionosphere during geomagnetically disturbed conditions, ...
International audienceData from the Jicamarca digisonde and the ROCSAT-1 satellite are employed to s...
We describe variations in total electron content (TEC) in the North American sector exhibiting prono...
We present the first complete study of the dynamics of the equatorial upper atmosphere (180-350 km) ...