Thermospheric neutral winds exhibit strong altitudinal and latitudinal variation during geomagnetically quiet and active times. We use daytime middle and low-latitude neutral winds measured by the Wind Imaging Interferometer (WINDII) instrument on board the Upper Atmosphere Research Satellite (UARS) over the 90–275 km height range to study the altitude and season dependent climatology of disturbance winds (i.e., with quiet time patterns removed) in magnetic coordinates. The daytime perturbations winds are generally equatorward and westward and decrease toward the magnetic equator. Both the zonal and meridional components decrease sharply below 120 km and are essentially insignificant below 100 km. The seasonal dependence of the disturbance ...
International audienceIn the context of space weather, we investigate the effect of geomagnetic acti...
We have studied mid- and low-latitude electrodynamic and neutral thermospheric dynamic processes usi...
Winds in the upper atmosphere vary with time, location and geomagnetic activity among other causes. ...
Thermospheric neutral winds exhibit strong altitudinal and latitudinal variation during geomagnetica...
Thermospheric neutral winds play important roles on the dynamics of the upper atmosphere. We use ext...
We studied the global climatology of mid- and low-latitude F region daytime neutral winds using exte...
We have modeled the global climatology of middle- and low-latitude F region daytime disturbance neut...
Altitude dependence of middle and low-latitude daytime thermospheric disturbance winds measured by W...
We use 630.0 nm nightglow Fabry-Perot measurements over Millstone Hill from 1989–1999 to study the c...
This study is focused on improving the poorly understood seasonal dependence of northern high-latitu...
Midlatitude nighttime thermospheric neutral winds are strongly dependent on season, solar activity, ...
We analyze upper thermospheric (∼250 km) nighttime horizontal neutral wind patterns, during geomagne...
This paper investigates the large-scale seasonal dependence of geomagnetically quiet time, northern ...
We analyze ground-based Fabry-Perot interferometer observations of upper thermospheric (∼250 km) hor...
In this project we have studied the climatology and storm-time dependence of longitude-averaged mid-...
International audienceIn the context of space weather, we investigate the effect of geomagnetic acti...
We have studied mid- and low-latitude electrodynamic and neutral thermospheric dynamic processes usi...
Winds in the upper atmosphere vary with time, location and geomagnetic activity among other causes. ...
Thermospheric neutral winds exhibit strong altitudinal and latitudinal variation during geomagnetica...
Thermospheric neutral winds play important roles on the dynamics of the upper atmosphere. We use ext...
We studied the global climatology of mid- and low-latitude F region daytime neutral winds using exte...
We have modeled the global climatology of middle- and low-latitude F region daytime disturbance neut...
Altitude dependence of middle and low-latitude daytime thermospheric disturbance winds measured by W...
We use 630.0 nm nightglow Fabry-Perot measurements over Millstone Hill from 1989–1999 to study the c...
This study is focused on improving the poorly understood seasonal dependence of northern high-latitu...
Midlatitude nighttime thermospheric neutral winds are strongly dependent on season, solar activity, ...
We analyze upper thermospheric (∼250 km) nighttime horizontal neutral wind patterns, during geomagne...
This paper investigates the large-scale seasonal dependence of geomagnetically quiet time, northern ...
We analyze ground-based Fabry-Perot interferometer observations of upper thermospheric (∼250 km) hor...
In this project we have studied the climatology and storm-time dependence of longitude-averaged mid-...
International audienceIn the context of space weather, we investigate the effect of geomagnetic acti...
We have studied mid- and low-latitude electrodynamic and neutral thermospheric dynamic processes usi...
Winds in the upper atmosphere vary with time, location and geomagnetic activity among other causes. ...