Yoshihiro_Asano_042208_3
Title/Introduction: magnetotail response, IMF By Change, SW n, Vx change
Key Word: IMF By, SW n and Vx change
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 04:00
Dipole Tilt at Start in X-Z Plane: 15.0 deg.
Dipole Tilt in Y-Z GSE Plane: 0.0 deg.
Dipole Update With Time: no
Ionospheric Conductance: auroral
Corotation Velocity is Applied at The Inner Boundary. Corotation And Dipole Axis Are Aligned.
Radio Flux 10.7 cm: 150.
Coordinate System for the Output: GSM
- View solar wind input data
- View Magnetosphere
- View Ionosphere
