• Imaging Vector Magnetogram at the MEES Solar Observatory in Hawaii

• 512x512 CCD with a resolution of 1.1 arcseconds

• 80 individual magnetograms of AR8210 spanning 4 hours with a cadence of three minutes

• I used 15 time averaged magnetograms to reduce noise and to account for solar oscillations

• For each magnetogram I have the x,  y, and z components of the magnetic field (B) on the photosphere

Uncertainty

• Used a gaussian fit on the distribution of Bz and Bt

• Found sigma values

• Calculated the B_z and B_t uncertainty at each time finding it to be relatively small