Lutz_Rastaetter_041106_1

Title/Introduction: Influence of ionosphere conductance on energy flows

Key Word: Conductance Effects Energy Flows

3D MHD Model: BATSRUS
Simulation With Modeled Conditions
Inflow Boundary Conditions: Time-Dependent
Start Time: 2000/01/01 00:00
End Time: 2000/01/01 03:00
Dipole Tilt at Start in X-Z Plane: 0.0 deg.
Dipole Tilt in Y-Z GSE Plane: 0.0 deg.
Dipole Update With Time: no
Ionospheric Conductance: auroral
No Corotation Velocity is Applied at The Inner Boundary.
Radio Flux 10.7 cm: 150.
Coordinate System for the Output: GSM
Initial Solar Wind (SW) Parameters in GSM Coordinates:

SW Density: 5 n/cc
SW Temperature [Kelvin]: 200000 Kelvin
X Component of SW Velocity: -400 km/sec
Y Component of SW Velocity: 0. km/sec
Z Component of SW Velocity: 0. km/sec
IMF Bx: 0. nT
IMF By: 0. nT
IMF Bz: -5 nT
IMF |B|: 5.00 nT
IMF Clock Angle: 180.0 deg.

• View solar wind input data
• View Magnetosphere
• View Ionosphere
• View Ring Current H+ ion data
• View Ring Current electron data

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