Michael_Kosch_121707_IT_1

Title/Introduction: This run is to verify a new technique of measuring neutral wind speeds using the drift of artificial aurora technique. Artificial auroras may be generated using powerful radiowaves from ionospheric Heaters.

Key Word: HIPAS

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

Initial Parameters:

SW Density: 3.626 n/cc
SW Temperature [Kelvin]: 28.16 Kelvin
X Component of SW Velocity: -448.374 km/sec
Y Component of SW Velocity: -2.022 km/sec
Z Component of SW Velocity: -33.831 km/sec
IMF Bx: 0.000 nT
IMF By: -1.985 nT
IMF Bz: -1.015 nT
IMF |B|: 2.229 nT
IMF Clock Angle: 242.928 deg.
Dipole Tilt at Start in X-Z Plane: 1.836 deg.
Dipole Tilt in Y-Z GSE Plane: 12.8 deg.

Year: 2007
Day of the year: 77
Radio Flux 10.7 cm: 69.8
Electric Field Model: Weimer
Hemispheric Power Index (Activity Level): 9189
Hemispheric Power in gigawatts: 16540.0

• 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
• View 2D Height-Integrated and Height-Independent Ionosphere Variables