1. Stokes profiles Swedish 1m Solar Telescope, perfect seeing

3. Stokes Profiles - Micropore

4. G-band & Magnetic Field Contours:.5, 1, 1.5 kG (gray) 20 G (red/green)

5. G-band Bright Points = large B, but some large B dark

6. Future Plans Supergranule scale magneto-convection 48 Mm wide x 20 Mm deep, include surface shear layer Quiet Sun - magnetic network, flux emergence, dispersal Active region - extrapolate surface vector magnetogram down as well as up as initial state High resolution meso-granule scale magneto-convection, plage region 6 Mm wide x 3 Mm deep 6 km horizontal & vertical resolution at surface Similar models by Schusler/Vogler et al. Need: code or IDL procedure to calculate Stokes profiles