Tuesday, 1 November 2011

Work up till now

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).

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