I have written the Surface flux transport code in FORTRAN77.
It seems to be working fine when I load an input with a single Bipolar Magnetic Region(BMR) placed near the equator. The diffusion seems to blow up the sunspots in size, and the meridional flow(11m/s) carries the poloidal component of the flux to the poles.
The above figures are contour plots of the radial magnetic field on the surface of the Sun. The X-axis is the azimuthal angle(phi) and the Y-axis is the polar angle(theta).
It seems to be working fine when I load an input with a single Bipolar Magnetic Region(BMR) placed near the equator. The diffusion seems to blow up the sunspots in size, and the meridional flow(11m/s) carries the poloidal component of the flux to the poles.
The above figures are contour plots of the radial magnetic field on the surface of the Sun. The X-axis is the azimuthal angle(phi) and the Y-axis is the polar angle(theta).
No comments:
Post a Comment