Samir_Naitamor_062807_1

Title/Introduction: the result is important to know how the magnetosphere interact with the solar wind during CME ejection

Key Word: solar wind, Dst

3D MHD Model: BATSRUS
Real Event Simulation
Inflow Boundary Conditions: Fixed
Start Time: 2003/10/29 00:00
End Time: 2003/10/29 12:00
Dipole Tilt at Start in X-Z Plane: -17.5 deg.
Dipole Tilt in Y-Z GSE Plane: -8.8 deg.
Dipole Update With Time: yes
Ionospheric Conductance: auroral
Corotation Velocity is Applied at The Inner Boundary. Corotation Axis Tilt is Consistent With The Real Time.
Radio Flux 10.7 cm: 275.4
Coordinate System for the Output: GSM
Initial Solar Wind (SW) Parameters in GSM Coordinates:

SW Density: 60 n/cc
SW Temperature [Kelvin]: 532100. Kelvin
X Component of SW Velocity: -900. km/sec
Y Component of SW Velocity: 200. km/sec
Z Component of SW Velocity: 100. km/sec
IMF Bx: 15. nT
IMF By: -15. nT
IMF Bz: -50. nT
IMF |B|: 54.31 nT
IMF Clock Angle: 196.7 deg.

• View Magnetosphere
• View Ionosphere
• View Ring Current H+ ion data
• View Ring Current electron data

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