Michael_Kosch_041810_IT_1

Title/Introduction: Conjugate thermospheric winds We use 3 Fabry-Perot interferometers in the northern Scandinavian sector and 2 Fabry-Perot interferometers in the southern Antarctic sector to study interhemispheric conjugate winds during the equinox. On this day we find strong evidence for the interhemispheric being

Key Word: Conjugate thermospheric winds

Model Type: IT
Model: CTIP
Dipole Update With Time: yes
Coordinate System for the Output: GEO

Initial Parameters:

SW Density: 2.505 n/cc
SW Temperature [Kelvin]: 49.67 Kelvin
X Component of SW Velocity: -617.218 km/sec
Y Component of SW Velocity: 7.906 km/sec
Z Component of SW Velocity: 4.665 km/sec
IMF Bx: 0.000 nT
IMF By: 2.496 nT
IMF Bz: 1.828 nT
IMF |B|: 3.093 nT
IMF Clock Angle: 53.781 deg.
Dipole Tilt at Start in X-Z Plane: -0.569 deg.
Dipole Tilt in Y-Z GSE Plane: -33.4 deg.

Year: 2008
Day of the year: 277
Radio Flux 10.7 cm: 67.2
Electric Field Model: Weimer
Hemispheric Power Index (Activity Level): 8
Hemispheric Power in gigawatts: 55.0000

• View Input: Hemispheric Power Index (Activity Level)
• View Input: Hemispheric Power in GW
• View Input: Solar Wind Parameters (|B|, IMF Clock Angle, Dipole Tilt, |V|)

• View 3D Ionosphere/Thermosphere
• Create Timeseries in 3D Ionosphere/Thermosphere
• View 2D Height-Integrated and Height-Independent Ionosphere Variables