Mass spectrometer satellite observations show that a narrow region with steep latitudinal gradients of neutral composition is formed in the subauroral winter thermosphere during magnetic storms. In order to analyze the relative importance of individual terms in the continuity equation for atomic oxygen, a two-dimensional model was used to simulate the thermospheric disturbance formation in response to intense Joule heating imposed in the auroral oval. Such an approach allowed three characteristic zones to be distinguished in the high-latitude thermosphere at heights of about 250 km. It was shown that vertical transport is of greatest importance within the local heating region. Horizontal transport dominates at subauroral latitudes ...
A model of the dynamics of magnetic storms is proposed which describes the effects of magnetospheric...
The thermospheric neutral wind and ionospheric layer conductance at latitudes higher than 45 degrees...
We study the role of substorms and steady magnetospheric convection (SMC) in magnetic flux transport...
Low-latitude dynamics, electrodynamics, and plasma density structure are closely linked. Dynamically...
Energy and diffusive mass transport associated with the thermospheric circulation are considered in ...
In this paper, we use data from the Dynamics Explorer 2 (DE 2) satellite and a theoretical simulatio...
A time-dependent calculation has been done to study dynamical and compositional structure of the the...
We investigate the sources of the variation of the high-latitude thermospheric neutral mass density ...
During the period October to December 1981, the Dynamics Explorer-2 (DE-2) spacecraft successively o...
Thermospheric wind circulation excited during magnetic storm shown as effective mechanism for removi...
Current theories of F-layer storms are discussed using numerical simulations with the Upper Atmosph...
The low-density cell structure in the high-latitude thermosphere is referred to as the density depl...
A considerable fraction of the solar wind energy that crosses the magnetopause ends up in the hi...
Hemispheric differences in the structure and dynamics of the polar regions of the thermosphere and i...
A thermospheric circulation model in meridian plane (TCMMP) is introduced and a case study on the va...
A model of the dynamics of magnetic storms is proposed which describes the effects of magnetospheric...
The thermospheric neutral wind and ionospheric layer conductance at latitudes higher than 45 degrees...
We study the role of substorms and steady magnetospheric convection (SMC) in magnetic flux transport...
Low-latitude dynamics, electrodynamics, and plasma density structure are closely linked. Dynamically...
Energy and diffusive mass transport associated with the thermospheric circulation are considered in ...
In this paper, we use data from the Dynamics Explorer 2 (DE 2) satellite and a theoretical simulatio...
A time-dependent calculation has been done to study dynamical and compositional structure of the the...
We investigate the sources of the variation of the high-latitude thermospheric neutral mass density ...
During the period October to December 1981, the Dynamics Explorer-2 (DE-2) spacecraft successively o...
Thermospheric wind circulation excited during magnetic storm shown as effective mechanism for removi...
Current theories of F-layer storms are discussed using numerical simulations with the Upper Atmosph...
The low-density cell structure in the high-latitude thermosphere is referred to as the density depl...
A considerable fraction of the solar wind energy that crosses the magnetopause ends up in the hi...
Hemispheric differences in the structure and dynamics of the polar regions of the thermosphere and i...
A thermospheric circulation model in meridian plane (TCMMP) is introduced and a case study on the va...
A model of the dynamics of magnetic storms is proposed which describes the effects of magnetospheric...
The thermospheric neutral wind and ionospheric layer conductance at latitudes higher than 45 degrees...
We study the role of substorms and steady magnetospheric convection (SMC) in magnetic flux transport...