190-193Electron density profiles from the Alouette-2 topside sounder are used to estimate the H+ flow velocity at latitudes above 50° geomagnetic. The flow velocity increases with latitude resulting in a clear peak at the latitude of the electron density trough beyond which the velocity starts decreasing. A detailed examination of the flow velocity, calculated from the data covering the period from Jan. 1966 to Dec. 1967, shows significant seasonal changes, with velocities larger in winter than in summer. Also the daytime values of the flow velocity are found to be smaller than the nighttime values. Effects of magnetic storms of the H+ flow velocity are also examined
To identify seasonal and latitudinal variations of F2 layer during magnetic storm, we examine the ch...
Nighttime thermospheric neutral wind velocities are determined at Arecibo, Puerto Rico, by using a F...
An interhemispheric plasma transport model has been used to study the flow characteristics of H+, He...
165-167The electron density profiles obtained by Alouette-II satellite have been used to study the p...
214-217The results of an analysis of the latitudinal variations of Ne are presented, with the data o...
134-138Electron density profiles from the Alouctte-II satellite are used to study the latitudinal di...
Large magnetic-storm-induced changes were detected in high-latitude topside vertical electron densit...
The latitudinal electron distribution at heights up to 3000 km are studied on the basis of the Aloue...
16-19The electron density profiles obtained by Alouette-II topside sounder satellite have been used ...
123-130Trans-equatorial passes of the Alouette-2 satellite covering ±60° dip are examined for latitu...
Data from the Fabry-Perot Interferometer and Dynasonde at Halley (75.5°S, 26.6°W, L ∼ 4.2), Antarcti...
We investigate the seasonal, local solar time, and geomagnetic activity variations of the average Do...
Abstract. The influence of the meridional wind velocity on the latitudinal location of the enhanced ...
Storm-time variations of the topside ionosphere in equatorial latitudes over the American zone are e...
Using DEMETER and DMSP satellite data, the spatial distribution of hydrogen ion (H+) in local daytim...
To identify seasonal and latitudinal variations of F2 layer during magnetic storm, we examine the ch...
Nighttime thermospheric neutral wind velocities are determined at Arecibo, Puerto Rico, by using a F...
An interhemispheric plasma transport model has been used to study the flow characteristics of H+, He...
165-167The electron density profiles obtained by Alouette-II satellite have been used to study the p...
214-217The results of an analysis of the latitudinal variations of Ne are presented, with the data o...
134-138Electron density profiles from the Alouctte-II satellite are used to study the latitudinal di...
Large magnetic-storm-induced changes were detected in high-latitude topside vertical electron densit...
The latitudinal electron distribution at heights up to 3000 km are studied on the basis of the Aloue...
16-19The electron density profiles obtained by Alouette-II topside sounder satellite have been used ...
123-130Trans-equatorial passes of the Alouette-2 satellite covering ±60° dip are examined for latitu...
Data from the Fabry-Perot Interferometer and Dynasonde at Halley (75.5°S, 26.6°W, L ∼ 4.2), Antarcti...
We investigate the seasonal, local solar time, and geomagnetic activity variations of the average Do...
Abstract. The influence of the meridional wind velocity on the latitudinal location of the enhanced ...
Storm-time variations of the topside ionosphere in equatorial latitudes over the American zone are e...
Using DEMETER and DMSP satellite data, the spatial distribution of hydrogen ion (H+) in local daytim...
To identify seasonal and latitudinal variations of F2 layer during magnetic storm, we examine the ch...
Nighttime thermospheric neutral wind velocities are determined at Arecibo, Puerto Rico, by using a F...
An interhemispheric plasma transport model has been used to study the flow characteristics of H+, He...