Results 101 to 110 of about 118,766 (238)
Space weather phenomena in the equatorial ionosphere [PDF]
Our increasing dependence on space-based technological systems requires that we understand the factors that determine "space weather", which affects the operation of satellites as well as space-based communication and navigation systems. The latter are particularly vulnerable to conditions in the dip equatorial ionosphere where geometry of the ...
openaire +1 more source
Spatial Relationship Between the Midlatitude Ionospheric Trough and Plasmaspheric Plumes
Abstract The plasmasphere, a subsystem of the complex geospace environment, is a torus of cold plasma “frozen” into Earth's magnetic field and sourced from the ionosphere. Plasmaspheric plumes–drainage channels formed during geospace storms–have primarily been observed near the equator.
Balázs Heilig +2 more
wiley +1 more source
Improved Ionospheric Correction for Dual Frequency and Differential GPS Positioning Methods [PDF]
A new three dimensional (3-D) electron density model has been developed that can give a very accurate description of the real ionospheric variation; latitudinally,longitudinally and altitudinally.
Nagarajoo, Karthigesu
core +2 more sources
Altitudinal Gradients of Plasma Drifts in The Equatorial Ionosphere
The Earth\u27s ionosphere is the weakly ionized region of the upper atmosphere extending from about 90 km to 800 km. Electrodynamic processes driven by ionospheric electric fields can significantly affect the propagation of radiowaves used in ...
Hui, Debrup
core +1 more source
Is there a hole in the topside, equatorial ionosphere?
AbstractA paper in 2000 (Huba, 2000) found a depression in electron density in the topside ionosphere near the magnetic equator, based on the SAMI-2 physical ionospheric model. The model showed, for the first time, the formation of a hole in electron density in the altitude range 1500–2500km at geomagnetic equatorial latitudes.
openaire +2 more sources
Statistics of Orientation of Nightside Auroral Arcs and Interplanetary Conditions
Abstract We present statistics and dependence on interplanetary conditions of the orientation of nightside auroral arcs in the equatorward part of the auroral oval. The results related to the arcs essentially represent the orientation and dynamics of the equatorial boundary of the nightside auroral oval.
A. Kozlovsky +3 more
wiley +1 more source
We present the observations of field‐aligned currents and the equatorial electrojet during the 23 March 2023 magnetic storm, focusing on the effect of the drastic decrease of the solar wind dynamic pressure occurred during the main phase.
Guan Le +6 more
doaj +1 more source
Abstract At subauroral latitudes, discrete auroras, such as strong thermal emission velocity enhancement and stable auroral red arcs, have been extensively studied. On the other hand, diffuse emissions at subauroral latitudes have not been studied well.
M. Gomi +25 more
wiley +1 more source
The ionosphere, as an essential component of the Earth’s space environment, contains free electrons that influence the amplitude and phase of radio signals.
Ziyi Zhao +6 more
doaj +1 more source
Abstract Ionospheric currents and their associated magnetic perturbations are difficult to predict due to the high variability of their driving mechanisms. In addition, the 3D structure of the currents is challenging to unravel due to the lack of direct observations within the current flow region, particularly in the E $E$‐layer.
P. Alken +6 more
wiley +1 more source

