Post on 20-Dec-2015
Utilizing CISM MHD Results in SEP Modeling
S. A. Ledvina, D. Odstrcil, J. G. Luhmann, D. Krauss-Varban, and I. Roth
What the SEP simulations need from the MHD results
• The shock location
• The shock strength, MA,
• The shock normal angle Bn
• The MHD variables– Density– Temperature– Magnetic field– Velocity
The SEP code uses the guiding center approximation:
• We only need to store the MHD variable along the magnetic field lines that originates from the Earth and traces back to the Sun.
• Since this is the only field line we need we can save the MHD values along this line often (~5 minutes).
To meet these requirements we have added a field line tracing output routine to ENLIL
Finding the Shock
• Normalize the dynamic pressure by r2.
• Calculate the gradients in the normalized pressure.
Finding the Shock Cont.• Calculate the gradient of the
normalized pressure along the field line.
• Starting from the Earth find the largest magnitude of the gradient. That is the shock location.
• Find where the gradients change by some value (~20%) from the background. Use the values midway between these points to find:– Shock strength– Shock jump conditions
Gradient along field line
Finding the shock normal angle
• Minimum variance analysis?
Remaining Code Issues
• Adding a field line tracing output routine to MAS
• Tracing field lines across the MAS-ENLIL boundary
• Tracing field lines across processors in parallel computations
Model Interface