**IMAGE COALIGNMENT AND A FLOW MAP
CALCULATION**

By tracking the MDI intensity structures with this time interval we primarily measure displacements of pores and small spots and reduce contributions from the motions of shorter lived granules. Compared to the granulation, pores and sunspots are large and high contrast features, which makes them more easy to track.

*
Our error estimate is based on spatial and temporal consistency of the
flow maps. Using a 44 hour intensity movie, we selected an extended
area which showed a stable flow pattern. The error is defined as the
minimum velocity value for which the velocity vector is guaranteed to
be in the correct quadrant. Our estimation is that the solar noise is
less than 30 m s ^{-1}. The final map was derived from the 44 hour
average (136 flow maps) of the local cross correlation, which
eliminated all short-term oscillations in the horizontal velocity field
as well as reducing noise.
*

*©BBSO/NJIT 2001*