¥Develop better MHD solution algorithms
that are
optimized for conditions in the solar atmosphere
¥Find longer vector magnetogram
sequences so can
run simulation longer
¥Greatly expand the simulation box size;
extend to
spherical chunks
¥Include a shearing of vx, vy in z direction in boundary
code to account for observed changes
in Bx and By.
¥Experiment with using LOS magnetograms